327 results on '"Khurana, K."'
Search Results
2. Energetic Electron Precipitation Driven by Electromagnetic Ion Cyclotron Waves from ELFIN’s Low Altitude Perspective
- Author
-
Angelopoulos, V., Zhang, X.-J., Artemyev, A. V., Mourenas, D., Tsai, E., Wilkins, C., Runov, A., Liu, J., Turner, D. L., Li, W., Khurana, K., Wirz, R. E., Sergeev, V. A., Meng, X., Wu, J., Hartinger, M. D., Raita, T., Shen, Y., An, X., Shi, X., Bashir, M. F., Shen, X., Gan, L., Qin, M., Capannolo, L., Ma, Q., Russell, C. L., Masongsong, E. V., Caron, R., He, I., Iglesias, L., Jha, S., King, J., Kumar, S., Le, K., Mao, J., McDermott, A., Nguyen, K., Norris, A., Palla, A., Roosnovo, A., Tam, J., Xie, E., Yap, R. C., Ye, S., Young, C., Adair, L. A., Shaffer, C., Chung, M., Cruce, P., Lawson, M., Leneman, D., Allen, M., Anderson, M., Arreola-Zamora, M., Artinger, J., Asher, J., Branchevsky, D., Cliffe, M., Colton, K., Costello, C., Depe, D., Domae, B. W., Eldin, S., Fitzgibbon, L., Flemming, A., Frederick, D. M., Gilbert, A., Hesford, B., Krieger, R., Lian, K., McKinney, E., Miller, J. P., Pedersen, C., Qu, Z., Rozario, R., Rubly, M., Seaton, R., Subramanian, A., Sundin, S. R., Tan, A., Thomlinson, D., Turner, W., Wing, G., Wong, C., and Zarifian, A.
- Published
- 2023
- Full Text
- View/download PDF
3. Identification of a Dynamic Atmosphere at Enceladus with the Cassini Magnetometer
- Author
-
Dougherty, M. K., Khurana, K. K., Neubauer, F. M., Russell, C. T., Saur, J., Leisner, J. S., and Burton, M. E.
- Published
- 2006
4. Cassini Magnetometer Observations during Saturn Orbit Insertion
- Author
-
Dougherty, M. K., Achilleos, N., Andre, N., Arridge, C. S., Balogh, A., Bertucci, C., Burton, M. E., Cowley, S. W. H., Erdos, G., Giampieri, G., Khurana, K. K., Leisner, J., Neubauer, F. M., Russell, C. T., Smith, E. J., Southwood, D. J., and Tsurutani, B. T.
- Published
- 2005
5. Localized Reconnection in the Near Jovian Magnetotail
- Author
-
Russell, C. T., Khurana, K. K., Huddleston, D. E., and Kivelson, M. G.
- Published
- 1998
6. A Magnetic Signature at Io: Initial Report from the Galileo Magnetometer
- Author
-
Kivelson, M. G., Khurana, K. K., Walker, R. J., Russell, C. T., Linker, J. A., Southwood, D. J., and Polanskey, C.
- Published
- 1996
7. Effects of radial motion on interchange injections at Saturn
- Author
-
Paranicas, C., Thomsen, M.F., Achilleos, N., Andriopoulou, M., Badman, S.V., Hospodarsky, G., Jackman, C.M., Jia, X., Kennelly, T., Khurana, K., Kollmann, P., Krupp, N., Louarn, P., Roussos, E., and Sergis, N.
- Published
- 2016
- Full Text
- View/download PDF
8. Properties of Quiet Magnetotail Plasma Sheet at Lunar Distances.
- Author
-
Runov, A., Angelopoulos, V., Khurana, K., Liu, J., Balikhin, M., and Artemyev, A. V.
- Subjects
SOLAR wind ,THERMODYNAMICS ,MOON ,GEOMAGNETISM ,PLASMA temperature ,LUNAR orbit - Abstract
The Earth's magnetotail at lunar distances (R ≈ 60 RE) serves as a unique laboratory to study plasma dynamics in a weak, highly fluctuating magnetic field with a strong magnetic field gradient. In particular, studies of the of quiet‐time plasma in the lunar‐distant magnetotail can inform us about plasma entry to the magnetosphere and sources of magnetospheric plasma populations. We use the data collected by the two lunar‐orbiting Acceleration, Reconnection, Turbulence and Electrodynamics of Moon's Interaction with the Sun (ARTEMIS) spacecraft during its 2013–2019 magnetotail traversals to infer the average thermodynamic and spectral properties of plasma populations in the quiet‐time (i.e., low geomagnetic activity and absence of fast plasma flows) magnetotail at lunar distances. We found that plasma temperature and density in the quiet‐time magnetotail at R ≈ 60 RE are organized by the magnetic field. Three distinct regions with plasma β ≫ 1, β ∼ 1, and β ≪ 1, the central plasma sheet (CPS), outer plasma sheet (OPS), and lobes are sampled. We found that temperatures and energy spectra of ion populations in CPS, OPS, and lobes regimes are different: the hotter CPS temperatures scale with the kinetic energy of solar wind protons; cold OPS/lobe ions are, likely, of ionospheric origin. The ion and electron particle spectra in CPS, OPS, and lobes are nonthermal and reasonably well fitted by the Kappa function, with κ exponent varying between 2.5 and 3.5. Plain Language Summary: Earth's only natural satellite, the Moon orbits around the Earth at a distance of about 239,000 miles (385,000 km). The two lunar‐orbiting Acceleration, Reconnection, Turbulence and Electrodynamics of Moon's Interaction with the Sun (ARTEMIS) spacecraft orbit around the Moon in stable equatorial, high‐eccentricity orbits, of 100‐km × 19,000‐km altitude. The Moon and the ARTEMIS satellites spend about 25 days in the solar wind and 3–4 days inside the Earth's magnetosphere in the magnetotail. Using the comprehensive instrumentation of the ARTEMIS satellites, we study properties of the plasma and the magnetic field in the Earth's magnetotail at lunar distances. Our statistical results are valuable for the NASA Lunar Gateway HERMES mission preparation. Key Points: We examine the properties of plasma populations in the magnetotail at R ≈ 60 RE under quiet conditionsNon‐Maxwellian ion and electron populations dominate at βi ≤ 1 and βi > 1 regimesAverage ion and electron equatorial temperatures scale with solar wind kinetic energy [ABSTRACT FROM AUTHOR]
- Published
- 2023
- Full Text
- View/download PDF
9. Pitch Angle Distributions of Energetic Particles Near Callisto.
- Author
-
Krupp, N., Roussos, E., Fränz, M., Kollmann, P., Paranicas, C., Clark, G., Khurana, K., and Galli, A.
- Subjects
PARTICLE detectors ,ELECTRON distribution ,PLASMA Alfven waves ,ANGLES ,ELECTRON beams ,PLASMA interactions - Abstract
The Galileo spacecraft performed close flybys of the moon Callisto between 1996 and 2001. We reanalyzed particle data of the energetic particles detector onboard Galileo and derived pitch angle distributions in the energy range of several keV to MeV during Callisto flybys C3, C9, C10, and C30. We establish that field‐aligned beams observed during the flyby periods are more likely to originate from Callisto's magnetospheric interaction rather than by independent magnetospheric processes. These beams are prominent only during flyby C3, they come mainly from the North, and connect the moon and the ionosphere of Jupiter. For short intervals they have also been observed propagating from the South. The beams are regularly unidirectional and typically extend to 300 keV in energy, occasionally reaching above 600 keV. Energetic particle depletions in Callisto's wake during the downstream flybys are not at all obvious, even at low altitudes and in the wake center. The signature of the wake becomes more apparent when energetic particle observations are organized in pitch angle. In that case, pitch angle distribution minima at 90 deg can be discerned in some flybys, however, not always associated with a profound drop in the absolute signal intensity. They instead indicate that field‐aligned particle flux within the wake is higher. Outside the wake these minima continue in an energy‐dependent disturbed region toward Jupiter which seems to be at least partially collocated with Alfvén‐wing structures as predicted from magnetohydrodynamic simulation results or simple flyby geometry considerations. Plain Language Summary: Pitch angle distributions of energetic electrons and ions during four close Callisto encounters of the Galileo spacecraft are analyzed and clear signatures of electron beams were found only for one of the four flybys. The beam energies extend up to 300 keV at least. The origin of those beams lies in the interaction between the plasma in the Jovian magnetosphere and the exosphere of Callisto. The electron beams were observed in regions of changing density and magnetic field values where the electrons are accelerated to maintain the current flow. The acceleration itself is most probably related to Alfvén waves. Key Points: Pitch angle distributions of electrons are used to establish field‐aligned beams near Callisto from the moon‐magnetosphere interactionClose to the moons, field‐aligned electron are accelerated in regions with changing density and magnetic field to maintain the current flowThere is evidence that at Callisto Alfvén waves could have accelerated electrons along field lines up to several hundreds of keV [ABSTRACT FROM AUTHOR]
- Published
- 2023
- Full Text
- View/download PDF
10. Energetic electron precipitation driven by electromagnetic ion cyclotron waves from ELFIN's low altitude perspective
- Author
-
Angelopoulos, V., Zhang, X. -J., Artemyev, A. V., Mourenas, D., Tsai, E., Wilkins, C., Runov, A., Liu, J., Turner, D. L., Li, W., Khurana, K., Wirz, R. E., Sergeev, V. A., Meng, X., Wu, J., Hartinger, M. D., Raita, T., Shen, Y., An, X., Shi, X., Bashir, M. F., Shen, X., Gan, L., Qin, M., Capannolo, L., Ma, Q., Russell, C. L., Masongsong, E. V., Caron, R., He, I., Iglesias, L., Jha, S., King, J., Kumar, S., Le, K., Mao, J., McDermott, A., Nguyen, K., Norris, A., Palla, A., Roosnovo, Tam, J., Xie, E., Yap, R. C., Ye, S., Young, C., Adair, L. A., Shaffer, C., Chung, M., Cruce, P., Lawson, M., Leneman, D., Allen, M., Anderson, M., Arreola-Zamora, M., Artinger, J., Asher, J., Branchevsky, D., Cliffe, M., Colton, K., Costello, C., Depe, D., Domae, B. W., Eldin, S., Fitzgibbon, L., Flemming, A., Frederick, D. M., Gilbert, A., Hesford, B., Krieger, R., Lian, K., McKinney, E., Miller, J. P., Pedersen, C., Qu, Z., Rozario, R., Rubly, M., Seaton, R., Subramanian, A., Sundin, S. R., Tan, A., Thomlinson, D., Turner, W., Wing, G., Wong, C., and Zarifian, A.
- Subjects
Plasma Physics (physics.plasm-ph) ,Physics - Space Physics ,FOS: Physical sciences ,Space Physics (physics.space-ph) ,Physics - Plasma Physics - Abstract
We review comprehensive observations of electromagnetic ion cyclotron (EMIC) wave-driven energetic electron precipitation using data from the energetic electron detector on the Electron Losses and Fields InvestigatioN (ELFIN) mission, two polar-orbiting low-altitude spinning CubeSats, measuring 50-5000 keV electrons with good pitch-angle and energy resolution. EMIC wave-driven precipitation exhibits a distinct signature in energy-spectrograms of the precipitating-to-trapped flux ratio: peaks at 0.5 MeV which are abrupt (bursty) with significant substructure (occasionally down to sub-second timescale). Multiple ELFIN passes over the same MLT sector allow us to study the spatial and temporal evolution of the EMIC wave - electron interaction region. Using two years of ELFIN data, we assemble a statistical database of 50 events of strong EMIC wave-driven precipitation. Most reside at L=5-7 at dusk, while a smaller subset exists at L=8-12 at post-midnight. The energies of the peak-precipitation ratio and of the half-peak precipitation ratio (our proxy for the minimum resonance energy) exhibit an L-shell dependence in good agreement with theoretical estimates based on prior statistical observations of EMIC wave power spectra. The precipitation ratio's spectral shape for the most intense events has an exponential falloff away from the peak (i.e., on either side of 1.45 MeV). It too agrees well with quasi-linear diffusion theory based on prior statistics of wave spectra. Sub-MeV electron precipitation observed concurrently with strong EMIC wave-driven 1MeV precipitation has a spectral shape that is consistent with efficient pitch-angle scattering down to 200-300 keV by much less intense higher frequency EMIC waves. These results confirm the critical role of EMIC waves in driving relativistic electron losses. Nonlinear effects may abound and require further investigation.
- Published
- 2022
11. Intraoperative Management of Renal Allograft Venous-Calyceal Fistula and Incidental Renal Cell Carcinoma During Renal Transplantation: A Case Report
- Author
-
Khurana, K. and Modlin, C.
- Published
- 2013
- Full Text
- View/download PDF
12. Europa's Magnetic Signature: Report from Galileo's Pass on 19 December 1996
- Author
-
Kivelson, M. G., Khurana, K. K., Joy, S., Russell, C. T., Southwood, D. J., Walker, R. J., and Polanskey, C.
- Published
- 1997
13. Lo's Interaction with the Plasma Torus: Galileo Magnetometer Report
- Author
-
Kivelson, M. G., Khurana, K. K., Walker, R. J., Warnecke, J., Russell, C. T., Linker, J. A., Southwood, D. J., and Polanskey, C.
- Published
- 1996
14. Nanomechanical sensing of the endothelial cell response to anti-inflammatory action of 1-methylnicotinamide chloride
- Author
-
Kolodziejczyk AM, Brzezinka GD, Khurana K, Targosz-Korecka M, and Szymonski M
- Subjects
Medicine (General) ,R5-920 - Abstract
AM Kolodziejczyk,1 GD Brzezinka,1 K Khurana,1,2 M Targosz-Korecka,1 M Szymonski11Research Centre for Nanometer-Scale Science and Advanced Materials, NANOSAM, Faculty of Physics, Astronomy and Applied Computer Science, Jagiellonian University, Krakow, Poland; 2Centre for Environmental Risk Assessment and Remediation (CERAR), University of South Australia, AustraliaBackground: There is increasing evidence that cell elastic properties should change considerably in response to chemical agents affecting the physiological state of the endothelium. In this work, a novel assay for testing prospective endothelium-targeted agents in vitro is presented.Materials and methods: The proposed methodology is based on nanoindentation spectroscopy using an atomic force microscope tip, which allows for quantitative evaluation of cell stiffness. As an example, we chose a pyridine derivative, 1-methylnicotinamide chloride (MNA), known to have antithrombotic and anti-inflammatory properties, as reported in recent in vivo experiments.Results: First, we determined a concentration range of MNA in which physiological parameters of the endothelial cells in vitro are not affected. Then, cell dysfunction was induced by incubation with tumor necrosis factor-alpha (TNF-α) and the cellular response to MNA treatment after TNF-α incubation was studied. In parallel to the nanoindentation spectroscopy, the endothelium phenotype was characterized using a fluorescence spectroscopy with F-actin labeling, and biochemical methods, such as secretion measurements of both nitric oxide (NO), and prostacyclin (PGI2) regulatory agents.Conclusion: We found that MNA could reverse the dysfunction of the endothelium caused by inflammation, if applied in the proper time and to the concentration scheme established in our investigations. A surprisingly close correlation was found between effective Young's modulus of the cells and actin polymerization/depolymerization processes in the endothelium cortical cytoskeleton, as well as NO and PGI2 levels. These results allow us to construct the physiological model of sequential intracellular pathways activated in the endothelium by MNA.Keywords: endothelium, cell stiffness, 1-methylnicotinamide chloride, atomic force microscopy, nanomechanical sensing
- Published
- 2013
15. Sources of Local Time Asymmetries in Magnetodiscs
- Author
-
Arridge, C. S., Kane, M., Sergis, N., Khurana, K. K., and Jackman, C. M.
- Published
- 2015
- Full Text
- View/download PDF
16. Measurement and QCD analysis of double-differential inclusive jet cross sections in proton-proton collisions at root s=13 TeV
- Author
-
Tumasyan, A., Adam, W., Rejkovic, J. W., Bergauer, T., Chatterjee, S., Damanakis, K., Dragicevic, M., Escalante Del Valle, Fruhwirth, A., Jeitler, R., Krammer, M., Lechner, N., Liko, L., Mikulec, D., Paulitsch, I., Pitters, P., Schieck, F. M., Schofbeck, J., Schwarz, R., Templ, D., Waltenberger, S., Wulz, W., C. -E., Chekhovsky, V., Litomin, A., Makarenko, V., Darwish, M. R., Wolf, De, Janssen, E. A., Kello, T., Lelek, T., Rejeb, Sfar, Van, Mechelen, Van, Putte, Van, Remortel, Blekman, N., Bols, F., D'Hondt, E. S., Delcourt, J., Faham, El, Lowette, H., Moortgat, S., Morton, S., Muller, A., Sahasransu, D., Tavernier, A. R., Van, Doninck, Beghin, W., Bilin, D., Clerbaux, B., Lentdecker, De, Favart, G., Grebenyuk, L., Kalsi, A., Lee, A. K., Mahdavikhorrami, K., Makarenko, M., Moureaux, I., Petre, L., Popov, L., Postiau, A., Starling, N., Thomas, E., L. V., Bemden, En, M. V., Velde, Er, Vanlaer, C., Cornelis, P., Dobur, T., Knolle, D., Lambrecht, J., Mestdach, L., Niedziela, G., Roskas, M., Samalan, C., Skovpen, A., Tytgat, K., Vermassen, M., Wezenbeek, B., Benecke, L., Bethani, A., Bruno, A., Bury, G., Caputo, F., David, C., Delaere, P., Donertas, C., Giammanco, I. S., Jaffel, A., Jain, K., Lemaitre, Sa., Mondal, V., Prisci, K., Aro, J., Taliercio, A., Teklishyn, M., Tran, T. T., Vischia, P., Wertz, S., Alves, G. A., Hensel, C., Moraes, A., Alda, Junior, W. L., Alves Gallo Pereira, Barroso Ferreira Filho, Br, M., Malbouisson, Ao, Carvalho, H., Chinellato, W., Costa, Da, E. M., Silveira, Da, G. G., De Jesus Damiao, Fonseca De Souza, Mora, Herrera, Mota, Amarilo, Mundim, K., Nogima, L., Rebello, Teles, Santoro, P., Silva Do Amaral, Sznajder, S. M., Thiel, A., Torres Da Silva De Araujo, Vilela, Pereira, Bernardes, A., Calligaris, C. A., Fern, L., ez Perez Tomei, Gregores, T. R., Lemos, E. M., Mercadante, D. S., Novaes, P. G., Padula, S. F., S, Ra, S., Aleks, Rov, Antchev, A., Hadjiiska, G., Iaydjiev, R., Misheva, P., Rodozov, M., Shopova, M., Sultanov, M., Dimitrov, G., Ivanov, A., Litov, T., Pavlov, L., Petkov, B., Petrov, P., Cheng, A., Javaid, T., Mittal, T., Yuan, M., Ahmad, L., Bauer, M., Dozen, G., Hu, C., Martins, Z., Wang, J., Yi, Y., Chapon, K., Chen, E., Chen, G. M., Chen, H. S., Iemmi, M., Kapoor, F., Leggat, A., Liao, D., Liu, H., Z. -A., Milosevic, V., Monti, F., Sharma, R., Tao, J., Thomas-Wilsker, J., Zhang, H., Zhao, J., Agapitos, A., An, Y., Ban, Y., Chen, C., Levin, A., Li, Q., Lyu, X., Mao, Y., Qian, S. J., Wang, D., Wang, Q., Xiao, J., Lu, M., You, Z., Gao, X., Okawa, H., Zhang, Y., Lin, Z., Xiao, M., Avila, C., Cabrera, A., Florez, C., Fraga, J., Mejia, Guisao, Ramirez, J., Ruiz, Alvarez, J. D., Salazar, Gonzalez, Giljanovic, C. A., Godinovic, D., Lelas, N., Puljak, D., Antunovic, I., Kovac, Z., Sculac, M., Brigljevic, T., Ferencek, V., Majumder, D., Roguljic, D., Starodumov, M., Susa, A., Attikis, T., Christoforou, A., Erodotou, K., Ioannou, E., Kole, A., Kolosova, G., Konstantinou, M., Mousa, S., Nicolaou, J., Ptochos, C., Razis, F., Rykaczewski, P. A., Saka, H., Finger, H., Finger, M., r. M., J, Kveton, A., Ayala, E., Carrera, Jarrin, Assran, E., Ellithi, Kamel, Mahmoud, A., Mohammed, M. A., Bhowmik, Y., Dewanjee, S., Ehataht, R. K., Kadastik, K., M. N., An, S., Nielsen, C., Pata, J., Raidal, M., Tani, L., Veelken, C., Eerola, P., Forthomme, L., Kirschenmann, H., Osterberg, K., Voutilainen, M., Bharthuar, S., Brucken, E., Garcia, F., Havukainen, J., Kim, M. S., Kinnunen, R., Lampen, T., Lassila-Perini, K., Lehti, S., Linden, T., Lotti, M., Martikainen, L., Myllymaki, M., Ott, J., Siikonen, H., Tuominen, E., Tuominiemi, J., Luukka, P., Petrow, H., Tuuva, T., Amendola, C., Besancon, M., Couderc, F., Dejardin, M., Denegri, D., Faure, J. L., Ferri, F., Ganjour, S., Gras, P., Hamel de Monchenault, Jarry, G., Lenzi, P., Locci, B., Malcles, E., J. R., Er, J., Rosowsky, A., Sahin, M. O., Savoy-Navarro, A., Titov, M., G. B., Yu, Ahuja, S., Beaudette, F., Bonanomi, M., Buchot, Perraguin, Busson, A., Cappati, P., Charlot, A., Davignon, C., Diab, O., Falmagne, B., Ghosh, G., Granier de Cassagnac, Hakimi, R., Kucher, A., Motta, I., Nguyen, J., Och, M., O, C., Paganini, P., Rembser, J., Salerno, R., Sarkar, U., Sauvan, J. B., Sirois, Y., Tarabini, A., Zabi, A., Zghiche, A., Agram, J. -L., Rea, J., Apparu, D., Bloch, D., Bourgatte, G., Brom, J. -M., Chabert, E. C., Collard, C., Darej, D., Fontaine, J. -C., Goerlach, U., Grimault, C., Bihan, Le, A. -C., Nibigira, E., Van, Hove, Asilar, P., Beauceron, E., Bernet, S., Boudoul, C., Camen, G., Carle, C., Chanon, A., Contardo, N., Depasse, D., Mamouni, El, Fay, H., Gascon, J., Gouzevitch, S., Ille, M., Laktineh, B., Lattaud, I. B., Lesauvage, H., Lethuillier, A., Mirabito, M., Perries, L., Shchablo, S., Sordini, K., Torterotot, V., Touquet, L., G. V., Donckt, Er, Viret, M., Lomidze, S., Toriashvili, I., Tsamalaidze, T., Botta, Z., Feld, V., Klein, L., Lipinski, K., Meuser, M., Pauls, D., Rowert, A., Schulz, N., Teroerde, J., Dodonova, M., Eliseev, A., Erdmann, D., Fackeldey, M., Fischer, P., Ghosh, B., Hebbeker, S., Hoepfner, T., Ivone, K., Mastrolorenzo, F., Merschmeyer, L., Meyer, M., Mocellin, A., Mondal, G., Mukherjee, S., Noll, S., Novak, D., Pook, A., Pozdnyakov, T., Rath, A., Reithler, Y., Roemer, H., Schmidt, J., Schuler, A., Sharma, S. C., Vigilante, A., Wiedenbeck, L., Zaleski, S., Dziwok, S., Flugge, C., Haj, Ahmad, Hlushchenko, W., Kress, O., Nowack, T., Pistone, A., Pooth, C., Roy, O., Sert, D., Stahl, H., Ziemons, A., Zotz, T., Aarup, Petersen, Aldaya, Martin, Asmuss, M., Baxter, P., Bayatmakou, S., Behnke, M., Bermudez, Martinez, Bhattacharya, A., Bin, Anuar, Borras, A. A., Brunner, K., Campbell, D., Cardini, A., Colombina, C., Consuegra, Rodriguez, Correia, Silva, Danilov, G., Silva, De, Didukh, M., Eckerlin, L., Eckstein, G., Eren, D., Estevez, Banos, Filatov, L. I., Gallo, O., Gao, E., Geiser, J., Giraldi, A., Grohsjean, A., Guthoff, A., Jafari, M., Jomhari, A., Jung, N. Z., Kasem, H., Kasemann, A., Kaveh, M., Kleinwort, H., Kruecker, C., Lange, D., Lidrych, W., Lipka, J., Lohmann, K., Maekelae, W., Mankel, T., Melzer-Pellmann, R., I. -A., Mendizabal, Morentin, Metwally, M., Meyer, J., Meyer, A. B., Mnich, M., Mussgiller, J., Otarid, A., Perez, Adan, Pitzl, D., Raspereza, D., Ribeiro, Lopes, Ruebenach, B., Saggio, J., Saibel, A., Savitskyi, A., Scham, M., Scheurer, M., Schnake, V., Schuetze, S., Schwanenberger, P., Shchedrolosiev, C., Sosa, Ricardo, Stafford, R. E., Tonon, D., Van De Klundert, Walsh, M., Walter, R., Wen, D., Wichmann, Y., Wiens, K., Wissing, L., Wuchterl, C., Zlebcik, S., Aggleton, R., Albrecht, R., Bein, S., Benato, S., Connor, L., Leo, De, Eich, K., Feindt, M., Froehlich, F., Garbers, A., Garutti, C., Gunnellini, E., Hajheidari, P., Haller, M., Hinzmann, J., Kasieczka, A., Klanner, G., Kogler, R., Kramer, R., Kutzner, T., Lange, V., Lange, J., Lobanov, T., Malara, A., Nigamova, A., Pena, Rodriguez, Rieger, K. J., Schleper, O., Schroeder, P., Schw, M., T, J., Sonneveld, J., Stadie, H., Steinbrueck, G., Tews, A., Zoi, I., Bechtel, J., Brommer, S., Burkart, M., Butz, E., Caspart, R., Chwalek, T., Boer, De, Dierlamm, W., Droll, A., Morabit, El, Faltermann, K., Giffels, N., Gosewisch, M., Gottmann, J. o., Hartmann, A., Heidecker, F., Husemann, C., Keicher, U., Koppenhoefer, P., Maier, R., Metzler, S., Mitra, M., Mueller, S., Neukum, Th., Nuernberg, M., Quast, A., Rabbertz, G., Rauser, K., Savoiu, J., Schnepf, D., Seith, M., Shvetsov, D., Simonis, I., Ulrich, H. J., Van Der Linden, Von, Cube, Wassmer, R. F., Weber, M., Wiel, M., Wolf, S., Wozniewski, R., Wunsch, S., Anagnostou, S., Daskalakis, G., Geralis, G., Kyriakis, T., Loukas, A., Stakia, D., Diamantopoulou, A., Karasavvas, M., Karathanasis, D., Kontaxakis, G., Koraka, P., Manousakis-Katsikakis, C. K., Panagiotou, A., Papavergou, A., Saoulidou, I., Theofilatos, N., Tziaferi, K., Vellidis, E., Vourliotis, K., Bakas, E., Kousouris, G., Papakrivopoulos, K., Tsipolitis, I., Zacharopoulou, G., Adamidis, A., Bestintzanos, K., Evangelou, I., Foudas, I., Gianneios, C., Katsoulis, P., Kokkas, P., Manthos, P., Papadopoulos, N., Strologas, I., Csanad, J., Farkas, M., Gadallah, K., Lokos, M. M. A., Major, S., P. M., Al, K., Mehta, A., Pasztor, G., Radl, A. J., Suranyi, O., Veres, G. I., Bartok, M., Bencze, G., Hajdu, C., Horvath, D., Sikler, F., Veszpremi, V., Czellar, S., Karancsi, J., Molnar, J., Szillasi, Z., Teyssier, D., Raics, P., Trocsanyi, Z. L., Ujvari, B., Csorgo, T., Nemes, F., Novak, T., Choudhury, S., Komaragiri, J. R., Kumar, D., Panwar, L., Tiwari, P. C., Bahinipati, S., Kar, C., Mal, P., Mishra, T., Muraleedharan Nair Bindhu, Nayak, V. K., Saha, A., Sur, P., Swain, N., Vats, S. K., Bansal, D., Beri, S., Bhatnagar, S. B., Chaudhary, V., Chauhan, G., Dhingra, S., Gupta, N., Kaur, R., Kaur, A., Kaur, M., Kumari, S., Meena, P., M. S., Eep, K., Singh, J. B., Virdi, A. K., Ahmed, A., Bhardwaj, A., Choudhary, B. C., Gola, M., Keshri, S., Kumar, A., Naimuddin, M., Priyanka, P., Ranjan, K., Shah, A., Bharti, M., Bhattacharya, R., Bhattacharya, S., Bhowmik, D., Dutta, S., Gomber, B., Maity, M., Palit, P., Rout, P. K., Saha, G., Sahu, B., Sarkar, S., Sharan, M., Singh, B., Thakur, S., Behera, P. K., Behera, S. C., Kalbhor, P., Muhammad, A., Pradhan, R., Pujahari, P. R., Sharma, A., Sikdar, A. K., Dutta, D., Jha, V., Kumar, V., Mishra, D. K., Naskar, K., Netrakanti, P. K., Pant, L. M., Shukla, P., Aziz, T., Dugad, S., Kumar, M., Banerjee, S., Chudasama, R., Guchait, M., Karmakar, S., Kumar, S., Majumder, G., Mazumdar, K., Alpana, K., Dube, S., Kansal, B., Laha, A., P, Ey, Rane, S., Rastogi, A., Bakhshiansohi, S., Khazaie, H., Zeinali, E., Chenarani, M., Etesami, S., Khakzad, S. M., Mohammadi, Najafabadi, Grunewald, M., Abbrescia, M., Aly, M., Aruta, R., Colaleo, C., Creanza, A., Filippis, De, Palma, De, Florio, Di, Pilato, Di, Elmetenawee, A., Fiore, W., Gelmi, L., Gul, A., Iaselli, M., Ince, G., Lezki, M., Maggi, S., Maggi, G., Margjeka, M., Mastrapasqua, I., My, V., Nuzzo, S., Pellecchia, S., Pompili, A., Pugliese, A., Ramos, G., Ranieri, D., Selvaggi, A., Silvestris, G., Simone, L., Venditti, F. M., Verwilligen, R., Abbiendi, P., Battilana, G., Bonacorsi, C., Borgonovi, D., Brigliadori, L., Campanini, L., Capiluppi, R., Castro, P., Cavallo, A., Cuffiani, F. R., Dallavalle, M., Diotalevi, G. M., Fabbri, T., Fanfani, F., Giacomelli, A., Giommi, P., Gr, L., I, C., Guiducci, L., Meo, Lo, Lunerti, S., Marcellini, L., Masetti, S., Navarria, G., Perrotta, F. L., Primavera, A., Rossi, F., Rovelli, A. M., Siroli, T., Albergo, G. P., Costa, S., Mattia, Di, Potenza, A., Tricomi, R., Tuve, A., Barbagli, C., Cassese, G., Ceccarelli, A., Ciulli, R., Civinini, V., D'Aless, C., Ro, R., Focardi, E., Latino, G., Lizzo, M., Meschini, M., Paoletti, S., Seidita, R., Sguazzoni, G., Viliani, L., Benussi, L., Bianco, S., Piccolo, D., Bozzo, M., Ferro, F., Mulargia, R., Robutti, E., Tosi, S., Benaglia, A., Boldrini, G., Brivio, F., Cetorelli, F., Guio, De, Dinardo, F., Dini, M. E., Gennai, P., Ghezzi, S., Govoni, A., Guzzi, P., Lucchini, L., Malberti, M. T., Malvezzi, M., Massironi, S., Menasce, A., Moroni, D., Paganoni, L., Pedrini, M., Pinolini, D., Ragazzi, B. S., Redaelli, S., Tabarelli de Fatis, Valsecchi, T., Zuolo, D., Buontempo, D., Carnevali, S., Cavallo, F., Iorio, De, Fabozzi, A., Iorio, F., Lista, A. O. M., Meola, L., Paolucci, S., Rossi, P., Sciacca, B., Azzi, C., Bacchetta, P., Bisello, N., Bortignon, D., Bragagnolo, P., Carlin, A., Checchia, R., Dorigo, P., Dosselli, T., Gasparini, U., Gasparini, F., Grosso, U., Hoh, G., Layer, S. Y., Lusiani, L., Margoni, E., Meneguzzo, M., Pazzini, A. T., Ronchese, J., Rossin, P., Simonetto, R., Strong, F., Tosi, G., Yarar, M., Zanetti, H., Zotto, M., Zucchetta, P., Zumerle, A., Aime, G., Braghieri, C., Calzaferri, A., Fiorina, S., Montagna, D., Ratti, P., S. P., Re, Riccardi, V., Salvini, C., Vai, P., Vitulo, I., Asenov, P., Bilei, P., Ciangottini, G. M., Fano, L., Lariccia, P., Magherini, M., Mantovani, G., Mariani, V., Menichelli, M., Moscatelli, F., Piccinelli, A., Presilla, M., Rossi, A., Santocchia, A., Spiga, D., Tedeschi, T., Azzurri, P., Bagliesi, G., Bertacchi, V., Bianchini, L., Boccali, T., Bossini, E., Castaldi, R., Ciocci, M. A., D'Amante, V., Dell'Orso, R., Domenico, Di, Donato, M. R., Giassi, S., Ligabue, A., Manca, F., Orli, G., Matos, Figueiredo, Messineo, D., Palla, A., Parolia, F., Ramirez-Sanchez, S., Rizzi, G., Rol, A., I, G., Roy, Chowdhury, Scribano, S., Shafiei, A., Spagnolo, N., Tenchini, P., Tonelli, R., Turini, G., Venturi, N., Verdini, A., Barria, P. G., Campana, P., Cavallari, M., Del, Re, Marco, Di, Diemoz, E., Longo, M., Meridiani, E., Organtini, P., G. P., Olfi, F., Paramatti, R., Quaranta, C., Rahatlou, S., Rovelli, C., Santanastasio, F., Soffi, L., Tramontano, R., Amapane, N., Arcidiacono, R., Argiro, S., Arneodo, M., Bartosik, N., Bellan, R., Bellora, A., Berenguer, Antequera, Biino, J., Cartiglia, C., Cometti, N., Covarelli, M., Demaria, R., Kiani, N., Legger, B., Mariotti, F., Maselli, C., Migliore, S., Monteil, E., Monteno, E., Obertino, M., Ortona, M. M., Pacher, G., Pastrone, L., Pelliccioni, N., Pinna, Angioni, Ruspa, G. L., Shchelina, M., Siviero, K., Sola, F., Solano, V., Soldi, A., Staiano, D., Tornago, A., Trocino, M., Vagnerini, D., Belforte, A., S. C., Elise, V., Casarsa, M., Cossutti, F., Rold, Da, Della, Ricca, Sorrentino, G., Vazzoler, G., Dogra, F., Huh, S., Kim, C., Kim, B., Kim, D. H., Kim, G. N., Lee, J., Moon, S. W., C. S., Oh, Pak, Y. D., Radburn-Smith, S. I., Sekmen, B. C., Yang, S., Kim, Y. C., Moon, H., Francois, D. H., Park, T. J., Cho, J., Choi, S., Go, S., Hong, Y., Lee, B., Lee, K., Lim, K. S., Park, J., Yoo, S. K., Goh, J., Gurtu, J., Kim, A., Kim, H. S., Almond, Y., Bhyun, J., Choi, J. H., Jeon, J., Kim, S., Kim, J., J. S., Ko, Kwon, S., Lee, H., Oh, S., B. H., Oh, Oh, M., Seo, S. B., Yang, H., Yoon, U. K., Jang, I., Kang, W., Kang, D. Y., Kim, Y., Ko, S., Lee, J. S. H., Merlin, Y., Park, J. A., Roh, I. C., Ryu, Y., Song, M. S., Watson, D., Yang, I. J., Ha, S., Yoo, S., Choi, H. D., Lee, M., Yu, Y., Beyrouthy, I., Maghrbi, T., Dreimanis, Y., Veckalns, K., Ambrozas, V., Carvalho Antunes De Oliveira, Juodagalvis, A., Rinkevicius, A., Tamulaitis, A., Bin, Norjoharuddeen, Wan, Abdullah, Yusli, W. A. T., Zolkapli, M. N., Benitez, Z., J. F., Castaneda, Hern, Ez, A., Leon, Coello, Murillo, Quijada, Sehrawat, J. A., Valencia, Palomo, Ayala, L., Castilla-Valdez, G., De La Cruz-Burelo, Heredia-De La Cruz, Lopez-Fern, I., Ez, R., Mondragon, Herrera, C. A., Perez, Navarro, D. A., Sanchez, Hern, Carrillo, Moreno, Oropeza, Barrera, Vazquez, Valencia, Pedraza, F., Salazar, Ibarguen, H. A., Uribe, Estrada, Mijuskovic, C., Raicevic, J., Krofcheck, N., Butler, D., Ahmad, P. H., Asghar, A., Awais, M. I., Awan, A., Hoorani, M. I. M., Khan, H. R., Shah, W. A., Shoaib, M. A., Waqas, M., Avati, M., Grzanka, V., Malawski, L., Bialkowska, M., Bluj, H., Boimska, M., Gorski, B., Kazana, M., Szleper, M., Zalewski, M., Bunkowski, P., Doroba, K., Kalinowski, K., Konecki, A., Krolikowski, M., Araujo, J., Bargassa, M., Bastos, P., Boletti, D., Faccioli, A., Gallinaro, P., Hollar, M., Leonardo, J., Niknejad, N., Pisano, T., Seixas, M., Toldaiev, J., Varela, O., Afanasiev, J., Budkouski, S., Golutvin, D., Gorbunov, I., Karjavine, I., Korenkov, V., Lanev, V., Malakhov, A., Matveev, A., Palichik, V., Perelygin, V., Savina, V., Seitova, M., Shalaev, D., Shmatov, V., Shulha, S., Smirnov, S., Teryaev, V., Voytishin, O., Yuldashev, N., Zarubin, B. S., Zhizhin, A., Gavrilov, I., Golovtcov, G., Ivanov, V., Kuznetsova, V., Murzin, E., Oreshkin, V., Smirnov, V., Sosnov, I., Sulimov, D., Uvarov, V., Volkov, L., Vorobyev, S., Reev, A., Dermenev, Yu., Gninenko, A., Golubev, S., Karneyeu, N., Kirpichnikov, A., Kirsanov, D., Krasnikov, M., Pashenkov, N., Pivovarov, A., Toropin, G., Epshteyn, A., Gavrilov, V., Lychkovskaya, V., Nikitenko, N., Popov, A., Stepennov, V., Toms, A., Vlasov, M., Zhokin, E., Aushev, A., Chadeeva, T., Oskin, M., Parygin, A., Popova, P., Rusinov, E., Selivanova, V., Reev, D., Azarkin, V., Dremin, M., Kirakosyan, I., Terkulov, M., Belyaev, A., Boos, A., Dubinin, E., Dudko, M., Ershov, L., Klyukhin, A., Kodolova, V., Lokhtin, O., Lukina, I., Obraztsov, O., Petrushanko, S., Savrin, S., Snigirev, V., Blinov, A., Dimova, V., Kardapoltsev, T., Kozyrev, L., Ovtin, A., Radchenko, I., Skovpen, O., Azhgirey, Y., Bayshev, I., Elumakhov, I., Kachanov, D., Konstantinov, V., D. M., Rik, P., Petrov, V., Ryutin, R., Slabospitskii, S., Sobol, A., Troshin, S., Tyurin, N., Uzunian, A., Volkov, A., Babaev, A., Okhotnikov, V., Borshch, V., Ivanchenko, V., Tcherniaev, E., Adzic, P., Dordevic, M., Milenovic, P., Milosevic, J., Aguilar-Benitez, M., Alcaraz, Maestre, Alvarez, Fern, Bachiller, I., Barrio, Luna, Bedoya, M., Cristina, F., Carrillo, Montoya, Cepeda, C. A., Cerrada, M., Colino, M., De La Cruz, Delgado, Peris, Fern, A., Ramos, Ez, Flix, J. P., Fouz, J., M. C., Gonzalez, Lopez, Goy, Lopez, Hern, S., J. M., Ez, Josa, M. I., Leon, Holgado, Moran, J., Navarro, Tobar, Perez, Dengra, Perez-Calero, Yzquierdo, Puerta, Pelayo, Redondo, J., Romero, I., Sanchez, Navas, Urda, Gomez, Willmott, L., Troconiz, De, Reyes-Almanza, J. F., Alvarez, Gonzalez, Cuevas, B., Erice, J., Fern, C., Menendez, Ez, Folgueras, J., Gonzalez, Caballero, Gonzalez, Fern, J. R., Ez, Palencia, Cortezon, Ramon, Alvarez, Rodriguez, Bouza, Soto, Rodriguez, Trapote, A., Trevisani, A., Vico, Villalba, Brochero, Cifuentes, Cabrillo, J. A., Calderon, I. J., Duarte, Campderros, Fern, J., Ez, M., Fern, Madrazo, Ez, Manteca, Ez, P. J., Garcia, Alonso, Gomez, A., Martinez, Rivero, Martinez Ruiz del Arbol, Matorras, P., Matorras, Cuevas, Piedra, Gomez, Prieels, J., Rodrigo, C., Ruiz-Jimeno, T., Scodellaro, A., Vila, L., Vizan, Garcia, Jayan, J. M., M. K., A, Kailasapathy, B., Sonnadara, D. U. J., Wickramarathna, D. D. C., Dharmaratna, W. G. D., Liyanage, K., Perera, N., Wickramage, N., Aarrestad, T. K., Abbaneo, D., Alimena, J., Auffray, E., Auzinger, G., Baechler, J., Baillon, P., Barney, D., Bendavid, J., Bianco, M., Bocci, A., Camporesi, T., Capeans, Garrido, Cerminara, M., Chernyavskaya, G., Chhibra, N., Cipriani, S. S., Cristella, M., D'Enterria, L., Dabrowski, D., David, A., Roeck, De, Defranchis, A., Deile, M. M., Dobson, M., Dunser, M., Dupont, M., Elliott-Peisert, N., Emriskova, A., Fallavollita, N., Fasanella, F., Florent, D., Franzoni, A., Funk, G., Giani, W., Gigi, S., Gill, D., Glege, K., Gouskos, F., Haranko, L., Hegeman, M., Innocente, J., James, V., Janot, T., Kaspar, P., Kieseler, J., Komm, J., Kratochwil, M., Lange, N., Laurila, C., Lecoq, S., Lintuluoto, P., Long, A., Lourenco, K., Maier, C., Malgeri, B., Mallios, L., Mannelli, S., Marini, M., Meijers, A. C., Mersi, F., Meschi, S., Moortgat, E., Mulders, F., Orfanelli, M., Orsini, S., Pantaleo, L., Pape, F., Perez, L., Peruzzi, E., Petrilli, M., Petrucciani, A., Pfeiffer, G., Pierini, A., Piparo, M., Pitt, D., Qu, M., Quast, H., Rabady, T., Racz, D., Reales, Gutierrez, Rieger, G., Rovere, M., Sakulin, M., Salfeld-Nebgen, H., Scarfi, J., Schafer, S., Schwick, C., Selvaggi, C., Sharma, M., Silva, A., Snoeys, P., Sphicas, W., Summers, P., Tatar, S., Tavolaro, K., Treille, V. R., Tropea, D., Tsirou, P., Van, Onsem, Wanczyk, G. P., Wozniak, J., Zeuner, K. A., Caminada, W. D., Ebrahimi, L., Erdmann, A., Horisberger, W., Ingram, R., Kaestli, Q., Kotlinski, H. C., Langenegger, D., Missiroli, U., Noehte, M., Rohe, L., Rosov, T., Backhaus, K., Berger, M., Cal, P., Ri, A., Cosa, De, Dissertori, A., Dittmar, G., Donega, M., Dorfer, M., Eble, C., Gedia, F., Glessgen, K., Gomez, Espinosa, Grab, T. A., Hits, C., Lustermann, D., Lyon, W., A. -M., Manzoni, R. A., Marchese, L., Martin, Perez, Meinhard, C., Nessi-Tedaldi, M. T., Niedziela, F., Pauss, J., Perovic, F., Pigazzini, V., Ratti, S., Reichmann, M. G., Reissel, M., Reitenspiess, C., Ristic, T., Ruini, B., Sanz, Becerra, Stampf, D. A., Steggemann, V., Wallny, J., Zhu, R., Amsler, D. H., Bartschi, C., Botta, P., Brzhechko, C., Canelli, D., Cormier, M. F., Wit, De, Del, Burgo, Heikkila, R., Huwiler, J. K., Jin, M., Jofrehei, W., Kilminster, A., Leontsinis, B., Liechti, S., Macchiolo, S. P., Meiring, A., Mikuni, P., Molinatti, V. M., Neutelings, U., Reimers, I., Robmann, A., Sanchez, Cruz, Schweiger, S., Senger, K., Takahashi, M., Adloff, Y., Kuo, C., Lin, C. M., Roy, W., Sarkar, A., Yu, T., Ceard, S. S., Chao, L., Chen, Y., Chen, K. F., Hou, P. H., W. -S., Y. y., Li, R. -S., Paganis, E., Psallidas, A., Steen, A., H. y., Wu, Yazgan, E., P. r., Yu, Asavapibhop, B., Asawatangtrakuldee, C., Srimanobhas, N., Boran, F., Damarseckin, S., Demiroglu, Z. S., Dolek, F., Dumanoglu, I., Eskut, E., Guler, Y., Gurpinar, Guler, Isik, E., Kara, C., Kayis, Topaksu, Kiminsu, A., Onengut, U., Ozdemir, G., Polatoz, K., Simsek, A., Tali, A. E., Tok, B., Turkcapar, U. G., Zorbakir, S., Isildak, I. S., Karapinar, B., Ocalan, G., Yalvac, K., Akgun, M., Atakisi, B., Gulmez, I. O., Kaya, E., Kaya, M., Ozcelik, O., Tekten, O., Yetkin, S., Cakir, E. A., Cankocak, A., Komurcu, K., Sen, Y., Cerci, S., Hos, S., Kaynak, I., Ozkorucuklu, B., Sunar, Cerci, Zorbilmez, D., Grynyov, C., Levchuk, B., Anthony, L., Bhal, D., Bologna, E., Brooke, S., Bundock, J. J., Clement, A., Cussans, E., Flacher, D., Goldstein, H., Heath, J., Heath, G. P., Kreczko, H. F., Krikler, L., Paramesvaran, B., Seif El Nasr-Storey, Smith, S., Stylianou, V. J., Walkingshaw, Pass, White, K., Bell, R., Belyaev, K. W., Brew, A., Brown, C., Cockerill, R. M., Cooke, D. J. A., Ellis, C., Harder, K. V., Harper, K., Holmberg, S., M. -L., Linacre, J., Manolopoulos, K., Newbold, D. M., Olaiya, E., Petyt, D., Reis, T., Schuh, T., Shepherd-Themistocleous, C. H., Tomalin, I. R., Williams, T., Bainbridge, R., Bloch, P., Bonomally, S., Borg, J., Breeze, S., Buchmuller, O., Cepaitis, V., Chahal, G. S., Colling, D., Dauncey, P., Davies, G., Della, Negra, Fayer, M., Fedi, S., Hall, G., Hassanshahi, G., Iles, M. H., Langford, G., Lyons, J., Magnan, L., Malik, S., Martelli, A., Monk, D. G., Nash, J., Pesaresi, M., Raymond, D. M., Richards, A., Rose, A., Scott, E., Seez, C., Shtipliyski, A., Tapper, A., Uchida, K., Virdee, T., Vojinovic, M., Wardle, N., Webb, S. N., Winterbottom, D., Coldham, K., Cole, J. E., Khan, A., Kyberd, P., Reid, I. D., Teodorescu, L., Zahid, S., Abdullin, S., Brinkerhoff, A., Caraway, B., Dittmann, J., Hatakeyama, K., Kanuganti, A. R., Mcmaster, B., Pastika, N., Saunders, M., Sawant, S., Sutantawibul, C., Wilson, J., Bartek, R., Dominguez, A., Uniyal, R., Vargas, Hern, A. M., Ez, Buccilli, A., Cooper, S. I., Croce, Di, Gleyzer, D., Henderson, S. V., Perez, C., Rumerio, C. U., West, P., Akpinar, C., Albert, A., Arcaro, A., Cosby, D., Demiragli, C., Fontanesi, Z., Gastler, E., May, D., Rohlf, S., Salyer, J., Sperka, K., Spitzbart, D., Suarez, D., Tsatsos, I., Yuan, A., Zou, S., Benelli, D., Burkle, G., Coubez, B., Cutts, X., Hadley, D., Heintz, M., Hogan, U., Kwon, J. M., T. L., Sberg, G., Lau, K. T., Li, D., Lukasik, M., Luo, J., Narain, M., Pervan, N., Sagir, S., Simpson, F., Usai, E., Wong, W. Y., Yan, X., Yu, D., Zhang, W., Bonilla, J., Brainerd, C., Breedon, R., Calderon De La Barca Sanchez, Chertok, M., Conway, M., Cox, J., Erbacher, P. T., Haza, R., Jensen, G., Kukral, F., O. L., Er, R., Mulhearn, M., Pellett, D., Regnery, B., Taylor, D., Yao, Y., Zhang, F., Bachtis, M., Cousins, R., Datta, A., Hamilton, D., Hauser, J., Ignatenko, M., Iqbal, M. A., Lam, T., Nash, W. A., Regnard, S., Saltzberg, D., Stone, B., Valuev, V., Burt, K., Clare, R., Gary, J. W., Gordon, M., Hanson, G., Karapostoli, G., Long, O. R., Manganelli, N., Olmedo, Negrete, Si, M., Wimpenny, W., Zhang, S., Branson, Y., Chang, J. G., Cittolin, P., Cooperstein, S., Deelen, S., Diaz, N., Duarte, D., Gerosa, J., Giannini, R., Guiang, L., Kansal, J., Krutelyov, R., Lee, V., Letts, R., Masciovecchio, J., Mokhtar, M., Pieri, F., Sathia, Narayanan, Sharma, B. V., Tadel, V., Vartak, M., Wurthwein, A., Xiang, F., Yagil, Y., Amin, A., Campagnari, N., Citron, C., Dorsett, M., Dutta, A., Inc, V., Ela, J., Kilpatrick, M., Marsh, B., Mei, H., Oshiro, M., Quinnan, M., Richman, J., Sarica, U., Setti, F., Sheplock, J., Stuart, D., Wang, S., Bornheim, A., Cerri, O., Dutta, I., Lawhorn, J. M., Lu, N., Mao, J., Newman, H. B., Nguyen, T. Q., Spiropulu, M., Vlimant, J. R., Wang, C., Xie, S., Zhang, Z., Zhu, R. Y., Alison, J., Rews, M. B., Bryant, P., Ferguson, T., Harilal, A., Liu, C., Mudholkar, T., Paulini, M., Sanchez, A., Terrill, W., Cumalat, J. P., Ford, W. T., Hassani, A., Macdonald, E., Patel, R., Perloff, A., Savard, C., Stenson, K., Ulmer, K. A., Wagner, S. R., Alex, Er, Bright-Thonney, J., Chen, S., Cheng, X., Cranshaw, Y., Hogan, D. J., Monroy, S., Patterson, J., Quach, J. R., Reichert, D., Reid, J., Ryd, M., Sun, A., Thom, W., Wittich, J., Zou, P., Albrow, R., Alyari, M., Apollinari, M., Apresyan, G., Apyan, A., Banerjee, A., Bauerdick, S., Berry, L. A. T., Berryhill, D., Bhat, J., Burkett, P. C., Butler, K., Canepa, J. N., Cerati, A., Cheung, G. B., Chlebana, H. W. K., Petrillo, Di, Elvira, K. F., Feng, V. D., Freeman, Y., Gecse, J., Gray, Z., Green, L., Grunendahl, D., Gutsche, S., Harris, O., Heller, R. M., Herwig, R., Hirschauer, T. C., Jayatilaka, J., Jindariani, B., Johnson, S., Joshi, M., Klijnsma, U., Klima, T., Kwok, B., Lammel, K. H. M., Lincoln, S., Lipton, D., Liu, R., Madrid, T., Maeshima, C., Mantilla, K., Mason, C., Mcbride, D., Merkel, P., Mrenna, P., Nahn, S., Ngadiuba, S., O'Dell, J., Papadimitriou, V., Pedro, V., Pena, K., Prokofyev, C., Ravera, O., Reinsvold, Hall, Ristori, A., Sexton-Kennedy, L., Smith, E., Soha, N., Spalding, A., Spiegel, W. J., Stoynev, L., Strait, S., Taylor, J., Tkaczyk, L., Tran, S., Uplegger, N. V., Va, L., Ering, E. W., Weber, H. A., Acosta, D., Avery, P., Bourilkov, D., Cadamuro, L., Cherepanov, V., Errico, F., Field, R. D., Guerrero, D., Joshi, B. M., Kim, M., Koenig, E., Konigsberg, J., Korytov, A., K. H., Lo, Matchev, K., Menendez, N., Mitselmakher, G., Muthirakalayil, Madhu, Rawal, A., Rosenzweig, N., Rosenzweig, D., Rotter, S., Shi, J., Sturdy, K., Yigitbasi, J., Zuo, E., Adams, X., Askew, T., Habibullah, A., Hagopian, R., Johnson, V., Khurana, K. F., Kolberg, R., Martinez, T., Prosper, G., Schiber, H., Viazlo, C., Yohay, O., Zhang, R., Baarm, J., Butalla, M. M., Elkafrawy, S., Hohlmann, T., Kumar, Verma, Noonan, R., Rahmani, D., Yumiceva, M., Adams, F., M. R., Becerril, Gonzalez, Cavanaugh, H., Dittmer, R., Evdokimov, S., Gerber, O., Hangal, C. E., Hofman, D. A., Merrit, D. J., Mills, A. H., Oh, C., Roy, G., Rudrabhatla, T., Tonjes, S., Varelas, M. B., Viinikainen, N., Wu, X., Ye, Z., Alhusseini, Z., Dilsiz, M., K. G., Rajula, R. P., Koseyan, O. K., Merlo, J. -P., Mestvirishvili, A., Nachtman, J., Ogul, H., Onel, Y., Penzo, A., Snyder, C., Tiras, E., Amram, O., Blumenfeld, B., Corcodilos, L., Davis, J., Eminizer, M., Gritsan, A. V., Kyriacou, S., Maksimovic, P., Roskes, J., Swartz, M., Vami, T. A., Abreu, A., Anguiano, J., Baldenegro, Barrera, Baringer, C., Bean, P., Bylinkin, A., Flowers, A., Isidori, Z., Khalil, T., King, S., Krintiras, J., Kropivnitskaya, G., Lazarovits, A., Mahieu, Le, Lindsey, C., Marquez, C., Minafra, J., Murray, N., Nickel, M., Rogan, M., Royon, C., Salvatico, C., R. S., Ers, S., Schmitz, E., Smith, C., Tapia, Takaki, Wang, J. D., Warner, Q., Williams, Z., Duric, G., Ivanov, S., Kaadze, A., Kim, K., Maravin, D., Mitchell, Y., Modak, T., Nam, A., Rebassoo, K., Wright, F., Adams, D., Baden, E., Baron, A., Belloni, O., Eno, A., Hadley, S. C., Jabeen, N. J., Kellogg, S., Koeth, R. G., Mignerey, T., Nabili, A. C., Palmer, S., Seidel, C., Skuja, M., Wang, A., Wong, L., Abercrombie, K., Reassi, D., Bi, G., Busza, R., Cali, W., Chen, I. A., D'Alfonso, Y., Eysermans, M., Freer, J., Gomez, Ceballos, Goncharov, G., Harris, M., Hu, P., Klute, M., Kovalskyi, M., Krupa, D., Y. -J., Mironov, C., Paus, C., Rankin, D., Rol, Rol, C., Shi, G., Stephans, Z., Wang, G. S. F., Wyslouch, Z., Chatterjee, B., Evans, R. M., Hiltbr, A., Jain, J., Krohn, Sh., Kubota, M., Mans, Y., Revering, J., Rusack, M., Saradhy, R., Schroeder, R., Strobbe, N., Wadud, N., Bloom, M. A., Bryson, K., Chauhan, M., Claes, S., Fangmeier, D. R., Finco, C., Golf, L., Joo, F., Kravchenko, C., Musich, I., Reed, M., Siado, I., Snow, J. E., Tabb, G. R., Yan, W., Zecchinelli, F., Agarwal, A. G., G. B., Yopadhyay, H., Hay, L., Iashvili, I., Kharchilava, A., Mclean, C., Nguyen, D., Pekkanen, J., Rappoccio, S., Williams, A., Alverson, G., Barberis, E., Haddad, Y., Hortiangtham, A., Li, J., Madigan, G., Marzocchi, B., Morse, D. M., Nguyen, V., Orimoto, T., Parker, A., Skinnari, L., Tishelman-Charny, A., Wamorkar, T., Wang, B., Wisecarver, A., Wood, D., Bueghly, J., Chen, Z., Gilbert, A., Gunter, T., Hahn, K. A., Liu, Y., Odell, N., Schmitt, M. H., Velasco, M., B, R., Bucci, R., Cremonesi, M., Das, A., Dev, N., Goldouzian, R., Hildreth, M., Hurtado, Anampa, Jessop, K., Lannon, C., Lawrence, K., Loukas, J., Lutton, N., Marinelli, D., Mcalister, N., Mccauley, I., Mcgrady, T., Mohrman, C., Moore, K., Musienko, C., Ruchti, Y., Siddireddy, R., Townsend, P., Wayne, A., Wightman, M., Zarucki, A., Zygala, M., Bylsma, L., Cardwell, B., Durkin, B., Francis, L. S., Hill, B., Nunez, Ornelas, Wei, M., Winer, K., Yates, B. L., Addesa, B. R., Bonham, F. M., Das, B., Dezoort, P., Elmer, G., Frankenthal, P., Greenberg, A., Haubrich, B., Higginbotham, N., Kalogeropoulos, S., Kopp, A., Kwan, G., Lange, S., Marlow, D., Mei, D., Ojalvo, K., Olsen, I., Stickl, J., Tully, D., Malik, C., Norberg, S., Bakshi, S., Barnes, A. S., Chawla, V. E., Das, R., Gutay, S., Jones, L., Jung, M., Karmarkar, A. W., Kondratyev, S., Liu, D., Negro, M., Neumeister, G., Paspalaki, N., Piperov, G., Purohit, S., Schulte, A., Stojanovic, J. F., Thieman, M., Xiao, F., Xie, R., Dolen, W., Parashar, J., Baty, N., Carnahan, A., Decaro, T., Dildick, M., Ecklund, S., Freed, K. M., Gardner, S., Geurts, P., Kumar, F. J. M., Li, A., Padley, W., Redjimi, B. P., Shi, R., Stahl, Leiton, Yang, A. G., Zhang, L., Bodek, Y., Barbaro, De, Demina, P., Dulemba, R., Fallon, J. L., Ferbel, C., Galanti, T., Garcia-Bellido, M., Hindrichs, A., Khukhunaishvili, O., Ranken, A., Taus, E., Chiarito, R., Chou, B., J. P. G., Rakota, A., Gershtein, Y., Halkiadakis, E., Hart, A., Heindl, M., Karacheban, O., Laflotte, I., Lath, A., Montalvo, R., Nash, K., Osherson, M., Salur, S., Schnetzer, S., Somalwar, S., Stone, R., Thayil, S. A., Thomas, S., Wang, H., Acharya, H., Delannoy, A. G., Fiorendi, S., Spanier, S., Bouhali, O., Dalchenko, M., Delgado, A., Eusebi, R., Gilmore, J., Huang, T., Kamon, T., Kim, H., Luo, S., Malhotra, S., Mueller, R., Overton, D., Rathjens, D., Safonov, A., Akchurin, N., Damgov, J., Hegde, V., Kunori, S., Lamichhane, K., Lee, S. W., Mengke, T., Muthumuni, S., Peltola, T., Volobouev, I., Wang, Z., Whitbeck, A., Appelt, E., Greene, S., Gurrola, A., Johns, W., Melo, A., Ni, H., Padeken, K., Romeo, F., Sheldon, P., Tuo, S., Velkovska, J., Arenton, M. W., Cox, B., Cummings, G., Hakala, J., Hirosky, R., Joyce, M., Ledovskoy, A., Neu, C., Perez, Lara, Tannenwald, C. E., White, B., Wolfe, S., Poudyal, E., Black, N., Bose, K., Caillol, T., Dasu, C., Bruyn, De, Everaerts, I., Fienga, P., Galloni, F., He, C., Herndon, H., Herve, M., Hussain, A., Lanaro, U., Loeliger, A., Loveless, A., Madhusudanan, Sreekala, Mallampalli, J., Mohammadi, A., Pinna, A., Savin, D., Shang, A., Sharma, V., Smith, V., Teague, W. H., Trembath-Reichert, D., Vetens, S., Cms, Collaboration, Damarseçkin, Serdal, CMS Collaboration, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut Pluridisciplinaire Hubert Curien (IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), CMS, Tumasyan, A, Adam, W, Andrejkovic, JW, Bergauer, T, Chatterjee, S, Damanakis, K, Dragicevic, M, Del Valle, AE, Fruhwirth, R, Jeitler, M, Krammer, N, Lechner, L, Liko, D, Mikulec, I, Paulitsch, P, Pitters, FM, Schieck, J, Schofbeck, R, Schwarz, D, Templ, S, Waltenberger, W, Wulz, CE, Chekhovsky, V, Litomin, A, Makarenko, V, Darwish, MR, De Wolf, EA, Janssen, T, Kello, T, Lelek, A, Sfar, HR, Van Mechelen, P, Van Putte, S, Van Remortel, N, Blekman, F, Bols, ES, D'Hondt, J, Delcourt, M, El Faham, H, Lowette, S, Moortgat, S, Morton, A, Muller, D, Sahasransu, AR, Tavernier, S, Van Doninck, W, Beghin, D, Bilin, B, Clerbaux, B, De Lentdecker, G, Favart, L, Grebenyuk, A, Kalsi, AK, Lee, K, Mahdavikhorrami, M, Makarenko, I, Moureaux, L, Petre, L, Popov, A, Postiau, N, Starling, E, Thomas, L, Vanden Bemden, M, Vander Velde, C, Vanlaer, P, Cornelis, T, Dobur, D, Knolle, J, Lambrecht, L, Mestdach, G, Niedziela, M, Roskas, C, Samalan, A, Skovpen, K, Tytgat, M, Vermassen, B, Wezenbeek, L, Benecke, A, Bethani, A, Bruno, G, Bury, F, Caputo, C, David, P, Delaere, C, Donertas, IS, Giammanco, A, Jaffel, K, Jain, S, Lemaitre, V, Mondal, K, Prisciandaro, J, Taliercio, A, Teklishyn, M, Tran, TT, Vischia, P, Wertz, S, Alves, GA, Hensel, C, Moraes, A, Alda, WL, Pereira, MAG, Ferreira, MB, Malbouisson, HB, Carvalho, W, Chinellato, J, Da Costa, EM, Da Silveira, GG, Damiao, DD, De Souza, SF, Herrera, CM, Amarilo, KM, Mundim, L, Nogima, H, Teles, PR, Santoro, A, Do Amaral, SMS, Sznajder, A, Thiel, M, De Araujo, FTD, Pereira, AV, Bernardes, CA, Calligaris, L, Tomei, TRFP, Gregores, EM, Lemos, DS, Mercadante, PG, Novaes, SF, Padula, SS, Aleksandrov, A, Antchev, G, Hadjiiska, R, Iaydjiev, P, Misheva, M, Rodozov, M, Shopova, M, Sultanov, G, Dimitrov, A, Ivanov, T, Litov, L, Pavlov, B, Petkov, P, Petrov, A, Cheng, T, Javaid, T, Mittal, M, Yuan, L, Ahmad, M, Bauer, G, Dozen, C, Hu, Z, Martins, J, Wang, Y, Yi, K, Chapon, E, Chen, GM, Chen, HS, Chen, M, Iemmi, F, Kapoor, A, Leggat, D, Liao, H, Liu, ZA, Milosevic, V, Monti, F, Sharma, R, Tao, J, Thomas-Wilsker, J, Wang, J, Zhang, H, Zhao, J, Agapitos, A, An, Y, Ban, Y, Chen, C, Levin, A, Li, Q, Lyu, X, Mao, Y, Qian, SJ, Wang, D, Wang, Q, Xiao, J, Lu, M, You, Z, Gao, X, Okawa, H, Zhang, Y, Lin, Z, Xiao, M, Avila, C, Cabrera, A, Florez, C, Fraga, J, Guisao, JM, Ramirez, F, Alvarez, JDR, Gonzalez, CAS, Giljanovic, D, Godinovic, N, Lelas, D, Puljak, I, Antunovic, Z, Kovac, M, Sculac, T, Brigljevic, V, Ferencek, D, Majumder, D, Roguljic, M, Starodumov, A, Susa, T, Attikis, A, Christoforou, K, Erodotou, E, Ioannou, A, Kole, G, Kolosova, M, Konstantinou, S, Mousa, J, Nicolaou, C, Ptochos, F, Razis, PA, Rykaczewski, H, Saka, H, Finger, M, Kveton, A, Ayala, E, Jarrin, EC, Assran, Y, Kamel, AE, Mahmoud, MA, Mohammed, Y, Bhowmik, S, Dewanjee, RK, Ehataht, K, Kadastik, M, Nandan, S, Nielsen, C, Pata, J, Raidal, M, Tani, L, Veelken, C, Eerola, P, Forthomme, L, Kirschenmann, H, Osterberg, K, Voutilainen, M, Bharthuar, S, Brucken, E, Garcia, F, Havukainen, J, Kim, MS, Kinnunen, R, Lampen, T, Lassila-Perini, K, Lehti, S, Linden, T, Lotti, M, Martikainen, L, Myllymaki, M, Ott, J, Siikonen, H, Tuominen, E, Tuominiemi, J, Luukka, P, Petrow, H, Tuuva, T, Amendola, C, Besancon, M, Couderc, F, Dejardin, M, Denegri, D, Faure, JL, Ferri, F, Ganjour, S, Gras, P, de Monchenault, GH, Jarry, P, Lenzi, B, Locci, E, Malcles, J, Rander, J, Rosowsky, A, Sahin, MO, Savoy-Navarro, A, Titov, M, Yu, GB, Ahuja, S, Beaudette, F, Bonanomi, M, Perraguin, AB, Busson, P, Cappati, A, Charlot, C, Davignon, O, Diab, B, Falmagne, G, Ghosh, S, de Cassagnac, RG, Hakimi, A, Kucher, I, Motta, J, Nguyen, M, Ochando, C, Paganini, P, Rembser, J, Salerno, R, Sarkar, U, Sauvan, JB, Sirois, Y, Tarabini, A, Zabi, A, Zghiche, A, Agram, JL, Andrea, J, Apparu, D, Bloch, D, Bourgatte, G, Brom, JM, Chabert, EC, Collard, C, Darej, D, Fontaine, JC, Goerlach, U, Grimault, C, Le Bihan, AC, Nibigira, E, Van Hove, P, Asilar, E, Beauceron, S, Bernet, C, Boudoul, G, Camen, C, Carle, A, Chanon, N, Contardo, D, Depasse, P, El Mamouni, H, Fay, J, Gascon, S, Gouzevitch, M, Ille, B, Laktineh, IB, Lattaud, H, Lesauvage, A, Lethuillier, M, Mirabito, L, Perries, S, Shchablo, K, Sordini, V, Torterotot, L, Touquet, G, Vander Donckt, M, Viret, S, Lomidze, I, Toriashvili, T, Tsamalaidze, Z, Botta, V, Feld, L, Klein, K, Lipinski, M, Meuser, D, Pauls, A, Rowert, N, Schulz, J, Teroerde, M, Dodonova, A, Eliseev, D, Erdmann, M, Fackeldey, P, Fischer, B, Hebbeker, T, Hoepfner, K, Ivone, F, Mastrolorenzo, L, Merschmeyer, M, Meyer, A, Mocellin, G, Mondal, S, Mukherjee, S, Noll, D, Novak, A, Pook, T, Pozdnyakov, A, Rath, Y, Reithler, H, Roemer, J, Schmidt, A, Schuler, SC, Sharma, A, Vigilante, L, Wiedenbeck, S, Zaleski, S, Dziwok, C, Flugge, G, Ahmad, WH, Hlushchenko, O, Kress, T, Nowack, A, Pistone, C, Pooth, O, Roy, D, Sert, H, Stahl, A, Ziemons, T, Zotz, A, Petersen, HA, Martin, MA, Asmuss, P, Baxter, S, Bayatmakou, M, Behnke, O, Martinez, AB, Bhattacharya, S, Bin Anuar, AA, Borras, K, Brunner, D, Campbell, A, Cardini, A, Cheng, C, Colombina, F, Rodriguez, SC, Silva, GC, Danilov, V, De Silva, M, Didukh, L, Eckerlin, G, Eckstein, D, Eren, E, Banos, LIE, Filatov, O, Gallo, E, Gao, J, Geiser, A, Giraldi, A, Grohsjean, A, Guthoff, M, Jafari, A, Jomhari, NZ, Jung, H, Kasem, A, Kasemann, M, Kaveh, H, Kleinwort, C, Krucker, D, Lange, W, Lidrych, J, Lipka, K, Lohmann, W, Makela, T, Mankel, R, Melzer-Pellmann, IA, Morentin, MM, Metwally, J, Meyer, AB, Meyer, M, Mnich, J, Mussgiller, A, Otarid, Y, Adan, DP, Pitzl, D, Raspereza, A, Lopes, BR, Rubenach, J, Saggio, A, Saibel, A, Savitskyi, M, Scham, M, Scheurer, V, Schnake, S, Schutze, P, Schwanenberger, C, Shchedrolosiev, M, Ricardo, RES, Stafford, D, Tonon, N, Van De Klundert, M, Walsh, R, Walter, D, Wen, Y, Wichmann, K, Wiens, L, Wissing, C, Wuchterl, S, Zlebcik, R, Aggleton, R, Albrecht, S, Bein, S, Benato, L, Connor, P, De Leo, K, Eich, M, Feindt, F, Frohlich, A, Garbers, C, Garutti, E, Gunnellini, P, Hajheidari, M, Haller, J, Hinzmann, A, Kasieczka, G, Klanner, R, Kogler, R, Kramer, T, Kutzner, V, Lange, J, Lange, T, Lobanov, A, Malara, A, Nigamova, A, Rodriguez, KJP, Rieger, O, Schleper, P, Schroder, M, Schwandt, J, Sonneveld, J, Stadie, H, Steinbruck, G, Tews, A, Zoi, I, Bechtel, J, Brommer, S, Burkart, M, Butz, E, Caspart, R, Chwalek, T, De Boer, W, Dierlamm, A, Droll, A, El Morabit, K, Faltermann, N, Giffels, M, Gosewisch, JO, Gottmann, A, Hartmann, F, Heidecker, C, Husemann, U, Keicher, P, Koppenhofer, R, Maier, S, Metzler, M, Mitra, S, Muller, T, Neukum, M, Nurnberg, A, Quast, G, Rabbertz, K, Rauser, J, Savoiu, D, Schnepf, M, Seith, D, Shvetsov, I, Simonis, HJ, Ulrich, R, Van Der Linden, J, Von Cube, RF, Wassmer, M, Weber, M, Wieland, S, Wolf, R, Wozniewski, S, Wunsch, S, Anagnostou, G, Daskalakis, G, Geralis, T, Kyriakis, A, Loukas, D, Stakia, A, Diamantopoulou, M, Karasavvas, D, Karathanasis, G, Kontaxakis, P, Koraka, CK, Manousakis-Katsikakis, A, Panagiotou, A, Papavergou, I, Saoulidou, N, Theofilatos, K, Tziaferi, E, Vellidis, K, Vourliotis, E, Bakas, G, Kousouris, K, Papakrivopoulos, I, Tsipolitis, G, Zacharopoulou, A, Adamidis, K, Bestintzanos, I, Evangelou, I, Foudas, C, Gianneios, P, Katsoulis, P, Kokkas, P, Manthos, N, Papadopoulos, I, Strologas, J, Csanad, M, Farkas, K, Gadallah, MMA, Lokos, S, Major, P, Mandal, K, Mehta, A, Pasztor, G, Radl, AJ, Suranyi, O, Veres, GI, Bartok, M, Bencze, G, Hajdu, C, Horvath, D, Sikler, F, Veszpremi, V, Czellar, S, Karancsi, J, Molnar, J, Szillasi, Z, Teyssier, D, Raics, P, Trocsanyi, ZL, Ujvari, B, Csorgo, T, Nemes, F, Novak, T, Choudhury, S, Komaragiri, JR, Kumar, D, Panwar, L, Tiwari, PC, Bahinipati, S, Kar, C, Mal, P, Mishra, T, Bindhu, VKMN, Nayak, A, Saha, P, Sur, N, Swain, SK, Vats, D, Bansal, S, Beri, SB, Bhatnagar, V, Chaudhary, G, Chauhan, S, Dhingra, N, Gupta, R, Kaur, A, Kaur, M, Kaur, S, Kumari, P, Meena, M, Sandeep, K, Singh, JB, Virdi, AK, Ahmed, A, Bhardwaj, A, Choudhary, BC, Gola, M, Keshri, S, Kumar, A, Naimuddin, M, Priyanka, P, Ranjan, K, Shah, A, Bharti, M, Bhattacharya, R, Bhowmik, D, Dutta, S, Gomber, B, Maity, M, Palit, P, Rout, PK, Saha, G, Sahu, B, Sarkar, S, Sharan, M, Singh, B, Thakur, S, Behera, PK, Behera, SC, Kalbhor, P, Muhammad, A, Pradhan, R, Pujahari, PR, Sikdar, AK, Dutta, D, Jha, V, Kumar, V, Mishra, DK, Naskar, K, Netrakanti, PK, Pant, LM, Shukla, P, Aziz, T, Dugad, S, Kumar, M, Banerjee, S, Chudasama, R, Guchait, M, Karmakar, S, Kumar, S, Majumder, G, Mazumdar, K, Alpana, K, Dube, S, Kansal, B, Laha, A, Pandey, S, Rane, A, Rastogi, A, Sharma, S, Bakhshiansohi, H, Khazaie, E, Zeinali, M, Chenarani, S, Etesami, SM, Khakzad, M, Najafabadi, MM, Grunewald, M, Abbrescia, M, Aly, R, Aruta, C, Colaleo, A, Creanza, D, De Filippis, N, De Palma, M, Di Florio, A, Di Pilato, A, Elmetenawee, W, Fiore, L, Gelmi, A, Gul, M, Iaselli, G, Ince, M, Lezki, S, Maggi, G, Maggi, M, Margjeka, I, Mastrapasqua, V, My, S, Nuzzo, S, Pellecchia, A, Pompili, A, Pugliese, G, Ramos, D, Ranieri, A, Selvaggi, G, Silvestris, L, Simone, FM, Venditti, R, Verwilligen, P, Abbiendi, G, Battilana, C, Bonacorsi, D, Borgonovi, L, Brigliadori, L, Campanini, R, Capiluppi, P, Castro, A, Cavallo, FR, Cuffiani, M, Dallavalle, GM, Diotalevi, T, Fabbri, F, Fanfani, A, Giacomelli, P, Giommi, L, Grandi, C, Guiducci, L, Lo Meo, S, Lunerti, L, Marcellini, S, Masetti, G, Navarria, FL, Perrotta, A, Primavera, F, Rossi, AM, Rovelli, T, Siroli, GP, Albergo, S, Costa, S, Di Mattia, A, Potenza, R, Tricomi, A, Tuve, C, Barbagli, G, Cassese, A, Ceccarelli, R, Ciulli, V, Civinini, C, D'Alessandro, R, Focardi, E, Latino, G, Lenzi, P, Lizzo, M, Meschini, M, Paoletti, S, Seidita, R, Sguazzoni, G, Viliani, L, Benussi, L, Bianco, S, Piccolo, D, Bozzo, M, Ferro, F, Mulargia, R, Robutti, E, Tosi, S, Benaglia, A, Boldrini, G, Brivio, F, Cetorelli, F, De Guio, F, Dinardo, ME, Dini, P, Gennai, S, Ghezzi, A, Govoni, P, Guzzi, L, Lucchini, MT, Malberti, M, Malvezzi, S, Massironi, A, Menasce, D, Moroni, L, Paganoni, M, Pedrini, D, Pinolini, BS, Ragazzi, S, Redaelli, N, de Fatis, TT, Valsecchi, D, Zuolo, D, Buontempo, S, Carnevali, F, Cavallo, N, De Iorio, A, Fabozzi, F, Iorio, AOM, Lista, L, Meola, S, Paolucci, P, Rossi, B, Sciacca, C, Azzi, P, Bacchetta, N, Bisello, D, Bortignon, P, Bragagnolo, A, Carlin, R, Checchia, P, Dorigo, T, Dosselli, U, Gasparini, F, Gasparini, U, Grosso, G, Hoh, SY, Layer, L, Lusiani, E, Margoni, M, Meneguzzo, AT, Pazzini, J, Ronchese, P, Rossin, R, Simonetto, F, Strong, G, Tosi, M, Yarar, H, Zanetti, M, Zotto, P, Zucchetta, A, Zumerle, G, Aime, C, Braghieri, A, Calzaferri, S, Fiorina, D, Montagna, P, Ratti, SP, Re, V, Riccardi, C, Salvini, P, Vai, I, Vitulo, P, Asenov, P, Bilei, GM, Ciangottini, D, Fano, L, Lariccia, P, Magherini, M, Mantovani, G, Mariani, V, Menichelli, M, Moscatelli, F, Piccinelli, A, Presilla, M, Rossi, A, Santocchia, A, Spiga, D, Tedeschi, T, Azzurri, P, Bagliesi, G, Bertacchi, V, Bianchini, L, Boccali, T, Bossini, E, Castaldi, R, Ciocci, MA, D'Amante, V, Dell'Orso, R, Di Domenico, MR, Donato, S, Giassi, A, Ligabue, F, Manca, E, Mandorli, G, Figueiredo, DM, Messineo, A, Palla, F, Parolia, S, Ramirez-Sanchez, G, Rizzi, A, Rolandi, G, Chowdhury, SR, Scribano, A, Shafiei, N, Spagnolo, P, Tenchini, R, Tonelli, G, Turini, N, Venturi, A, Verdini, PG, Barria, P, Campana, M, Cavallari, F, Del Re, D, Di Marco, E, Diemoz, M, Longo, E, Meridiani, P, Organtini, G, Pandolfi, F, Paramatti, R, Quaranta, C, Rahatlou, S, Rovelli, C, Santanastasio, F, Soffi, L, Tramontano, R, Amapane, N, Arcidiacono, R, Argiro, S, Arneodo, M, Bartosik, N, Bellan, R, Bellora, A, Antequera, JB, Biino, C, Cartiglia, N, Cometti, S, Costa, M, Covarelli, R, Demaria, N, Kiani, B, Legger, F, Mariotti, C, Maselli, S, Migliore, E, Monteil, E, Monteno, M, Obertino, MM, Ortona, G, Pacher, L, Pastrone, N, Pelliccioni, M, Angioni, GLP, Ruspa, M, Shchelina, K, Siviero, F, Sola, V, Solano, A, Soldi, D, Staiano, A, Tornago, M, Trocino, D, Vagnerini, A, Belforte, S, Candelise, V, Casarsa, M, Cossutti, F, Da Rold, A, Della Ricca, G, Sorrentino, G, Vazzoler, F, Dogra, S, Huh, C, Kim, B, Kim, DH, Kim, GN, Kim, J, Lee, J, Lee, SW, Moon, CS, Oh, YD, Pak, SI, Radburn-Smith, BC, Sekmen, S, Yang, YC, Kim, H, Moon, DH, Francois, B, Kim, TJ, Park, J, Cho, S, Choi, S, Go, Y, Hong, B, Lee, KS, Lim, J, Park, SK, Yoo, J, Goh, J, Gurtu, A, Kim, HS, Kim, Y, Almond, J, Bhyun, JH, Choi, J, Jeon, S, Kim, JS, Ko, S, Kwon, H, Lee, H, Lee, S, Oh, BH, Oh, M, Oh, SB, Seo, H, Yang, UK, Yoon, I, Jang, W, Kang, DY, Kang, Y, Kim, S, Ko, B, Lee, JSH, Lee, Y, Merlin, JA, Park, IC, Roh, Y, Ryu, MS, Song, D, Watson, IJ, Yang, S, Ha, S, Yoo, HD, Choi, M, Yu, I, Beyrouthy, T, Maghrbi, Y, Dreimanis, K, Veckalns, V, Ambrozas, M, De Oliveira, ACA, Juodagalvis, A, Rinkevicius, A, Tamulaitis, G, Bin Norjoharuddeen, N, Abdullah, WATW, Yusli, MN, Zolkapli, Z, Benitez, JF, Hernandez, AC, Coello, ML, Quijada, JAM, Sehrawat, A, Palomo, LV, Ayala, G, Castilla-Valdez, H, De La Cruz-Burelo, E, Heredia-De La Cruz, I, Lopez-Fernandez, R, Herrera, CAM, Navarro, DAP, Hernandez, AS, Moreno, SC, Barrera, CO, Valencia, FV, Pedraza, I, Ibarguen, HAS, Estrada, CU, Mijuskovic, J, Raicevic, N, Krofcheck, D, Butler, PH, Ahmad, A, Asghar, MI, Awais, A, Awan, MIM, Hoorani, HR, Khan, WA, Shah, MA, Shoaib, M, Waqas, M, Avati, V, Grzanka, L, Malawski, M, Bialkowska, H, Bluj, M, Boimska, B, Gorski, M, Kazana, M, Szleper, M, Zalewski, P, Bunkowski, K, Doroba, K, Kalinowski, A, Konecki, M, Krolikowski, J, Araujo, M, Bargassa, P, Bastos, D, Boletti, A, Faccioli, P, Gallinaro, M, Hollar, J, Leonardo, N, Niknejad, T, Pisano, M, Seixas, J, Toldaiev, O, Varela, J, Afanasiev, S, Budkouski, D, Golutvin, I, Gorbunov, I, Karjavine, V, Korenkov, V, Lanev, A, Malakhov, A, Matveev, V, Palichik, V, Perelygin, V, Savina, M, Seitova, D, Shalaev, V, Shmatov, S, Shulha, S, Smirnov, V, Teryaev, O, Voytishin, N, Yuldashev, BS, Zarubin, A, Zhizhin, I, Gavrilov, G, Golovtcov, V, Ivanov, Y, Kim, V, Kuznetsova, E, Murzin, V, Oreshkin, V, Smirnov, I, Sosnov, D, Sulimov, V, Uvarov, L, Volkov, S, Vorobyev, A, Andreev, Y, Dermenev, A, Gninenko, S, Golubev, N, Karneyeu, A, Kirpichnikov, D, Kirsanov, M, Krasnikov, N, Pashenkov, A, Pivovarov, G, Toropin, A, Epshteyn, V, Gavrilov, V, Lychkovskaya, N, Nikitenko, A, Popov, V, Stepennov, A, Toms, M, Vlasov, E, Zhokin, A, Aushev, T, Chadeeva, M, Oskin, A, Parygin, P, Popova, E, Rusinov, V, Selivanova, D, Andreev, V, Azarkin, M, Dremin, I, Kirakosyan, M, Terkulov, A, Belyaev, A, Boos, E, Dubinin, M, Dudko, L, Ershov, A, Klyukhin, V, Kodolova, O, Lokhtin, I, Lukina, O, Obraztsov, S, Petrushanko, S, Savrin, V, Snigirev, A, Blinov, V, Dimova, T, Kardapoltsev, L, Kozyrev, A, Ovtin, I, Radchenko, O, Skovpen, Y, Azhgirey, I, Bayshev, I, Elumakhov, D, Kachanov, V, Konstantinov, D, Mandrik, P, Petrov, V, Ryutin, R, Slabospitskii, S, Sobol, A, Troshin, S, Tyurin, N, Uzunian, A, Volkov, A, Babaev, A, Okhotnikov, V, Borshch, V, Ivanchenko, V, Tcherniaev, E, Adzic, P, Dordevic, M, Milenovic, P, Milosevic, J, Aguilar-Benitez, M, Maestre, JA, Fernandez, AA, Bachiller, I, Luna, MB, Bedoya, CF, Montoya, CAC, Cepeda, M, Cerrada, M, Colino, N, De La Cruz, B, Peris, AD, Ramos, JPF, Flix, J, Fouz, MC, Lopez, OG, Lopez, SG, Hernandez, JM, Josa, MI, Holgado, JL, Moran, D, Tobar, AN, Dengra, CP, Yzquierdo, APC, Pelayo, JP, Redondo, I, Romero, L, Navas, SS, Gomez, LU, Willmott, C, de Troconiz, JF, Reyes-Almanza, R, Gonzalez, BA, Cuevas, J, Erice, C, Menendez, JF, Folgueras, S, Caballero, IG, Fernandez, JRG, Cortezon, EP, Alvarez, CR, Bouza, VR, Rodriguez, AS, Trapote, A, Trevisani, N, Villalba, CV, Cifuentes, JAB, Cabrillo, IJ, Calderon, A, Campderros, JD, Fernandez, M, Madrazo, CF, Manteca, PJF, Alonso, AG, Gomez, G, Rivero, CM, del Arbol, PMR, Matorras, F, Cuevas, PM, Gomez, JP, Prieels, C, Rodrigo, T, Ruiz-Jimeno, A, Scodellaro, L, Vila, I, Garcia, JMV, Jayananda, MK, Kailasapathy, B, Sonnadara, DUJ, Wickramarathna, DDC, Dharmaratna, WGD, Liyanage, K, Perera, N, Wickramage, N, Aarrestad, TK, Abbaneo, D, Alimena, J, Auffray, E, Auzinger, G, Baechler, J, Baillon, P, Barney, D, Bendavid, J, Bianco, M, Bocci, A, Camporesi, T, Garrido, MC, Cerminara, G, Chernyavskaya, N, Chhibra, SS, Cipriani, M, Cristella, L, d'Enterria, D, Dabrowski, A, David, A, De Roeck, A, Defranchis, MM, Deile, M, Dobson, M, Dunser, M, Dupont, N, Elliott-Peisert, A, Emriskova, N, Fallavollita, F, Fasanella, D, Florent, A, Franzoni, G, Funk, W, Giani, S, Gigi, D, Gill, K, Glege, F, Gouskos, L, Haranko, M, Hegeman, J, Innocente, V, James, T, Janot, P, Kaspar, J, Kieseler, J, Komm, M, Kratochwil, N, Lange, C, Laurila, S, Lecoq, P, Lintuluoto, A, Long, K, Lourenco, C, Maier, B, Malgeri, L, Mallios, S, Mannelli, M, Marini, AC, Meijers, F, Mersi, S, Meschi, E, Moortgat, F, Mulders, M, Orfanelli, S, Orsini, L, Pantaleo, F, Pape, L, Perez, E, Peruzzi, M, Petrilli, A, Petrucciani, G, Pfeiffer, A, Pierini, M, Piparo, D, Pitt, M, Qu, H, Quast, T, Rabady, D, Racz, A, Gutierrez, GR, Rieger, M, Rovere, M, Sakulin, H, Salfeld-Nebgen, J, Scarfi, S, Schafer, C, Schwick, C, Selvaggi, M, Silva, P, Snoeys, W, Sphicas, P, Summers, S, Tatar, K, Tavolaro, VR, Treille, D, Tropea, P, Tsirou, A, Van Onsem, GP, Wanczyk, J, Wozniak, KA, Zeuner, WD, Caminada, L, Ebrahimi, A, Erdmann, W, Horisberger, R, Ingram, Q, Kaestli, HC, Kotlinski, D, Langenegger, U, Missiroli, M, Noehte, L, Rohe, T, Androsov, K, Backhaus, M, Berger, P, Calandri, A, De Cosa, A, Dissertori, G, Dittmar, M, Donega, M, Dorfer, C, Eble, F, Gedia, K, Glessgen, F, Espinosa, TAG, Grab, C, Hits, D, Lustermann, W, Lyon, AM, Manzoni, RA, Marchese, L, Perez, CM, Meinhard, MT, Nessi-Tedaldi, F, Niedziela, J, Pauss, F, Perovic, V, Pigazzini, S, Ratti, MG, Reichmann, M, Reissel, C, Reitenspiess, T, Ristic, B, Ruini, D, Becerra, DAS, Stampf, V, Steggemann, J, Wallny, R, Zhu, DH, Amsler, C, Bartschi, P, Botta, C, Brzhechko, D, Canelli, MF, Cormier, K, De Wit, A, Del Burgo, R, Heikkila, JK, Huwiler, M, Jin, W, Jofrehei, A, Kilminster, B, Leontsinis, S, Liechti, SP, Macchiolo, A, Meiring, P, Mikuni, VM, Molinatti, U, Neutelings, I, Reimers, A, Robmann, P, Cruz, SS, Schweiger, K, Senger, M, Takahashi, Y, Adloff, C, Kuo, CM, Lin, W, Roy, A, Sarkar, T, Yu, SS, Ceard, L, Chao, Y, Chen, KF, Chen, PH, Hou, WS, Li, YY, Lu, RS, Paganis, E, Psallidas, A, Steen, A, Wu, HY, Yazgan, E, Yu, PR, Asavapibhop, B, Asawatangtrakuldee, C, Srimanobhas, N, Boran, F, Damarseckin, S, Demiroglu, ZS, Dolek, F, Dumanoglu, I, Eskut, E, Guler, Y, Guler, EG, Isik, C, Kara, O, Topaksu, AK, Kiminsu, U, Onengut, G, Ozdemir, K, Polatoz, A, Simsek, AE, Tali, B, Tok, UG, Turkcapar, S, Zorbakir, IS, Isildak, B, Karapinar, G, Ocalan, K, Yalvac, M, Akgun, B, Atakisi, IO, Gulmez, E, Kaya, M, Kaya, O, Ozcelik, O, Tekten, S, Yetkin, EA, Cakir, A, Cankocak, K, Komurcu, Y, Sen, S, Cerci, S, Hos, I, Kaynak, B, Ozkorucuklu, S, Cerci, DS, Zorbilmez, C, Grynyov, B, Levchuk, L, Anthony, D, Bhal, E, Bologna, S, Brooke, JJ, Bundock, A, Clement, E, Cussans, D, Flacher, H, Goldstein, J, Heath, GP, Heath, HF, Kreczko, L, Krikler, B, Paramesvaran, S, El Nasr-Storey, SS, Smith, VJ, Stylianou, N, Pass, KW, White, R, Bell, KW, Brew, C, Brown, RM, Cockerill, DJA, Cooke, C, Ellis, KV, Harder, K, Harper, S, Holmberg, ML, Linacre, J, Manolopoulos, K, Newbold, DM, Olaiya, E, Petyt, D, Reis, T, Schuh, T, Shepherd-Themistocleous, CH, Tomalin, IR, Williams, T, Bainbridge, R, Bloch, P, Bonomally, S, Borg, J, Breeze, S, Buchmuller, O, Cepaitis, V, Chahal, GS, Colling, D, Dauncey, P, Davies, G, Della Negra, M, Fayer, S, Fedi, G, Hall, G, Hassanshahi, MH, Iles, G, Langford, J, Lyons, L, Magnan, AM, Malik, S, Martelli, A, Monk, DG, Nash, J, Pesaresi, M, Raymond, DM, Richards, A, Rose, A, Scott, E, Seez, C, Shtipliyski, A, Tapper, A, Uchida, K, Virdee, T, Vojinovic, M, Wardle, N, Webb, SN, Winterbottom, D, Coldham, K, Cole, JE, Khan, A, Kyberd, P, Reid, ID, Teodorescu, L, Zahid, S, Abdullin, S, Brinkerhoff, A, Caraway, B, Dittmann, J, Hatakeyama, K, Kanuganti, AR, McMaster, B, Pastika, N, Saunders, M, Sawant, S, Sutantawibul, C, Wilson, J, Bartek, R, Dominguez, A, Uniyal, R, Hernandez, AMV, Buccilli, A, Cooper, SI, Di Croce, D, Gleyzer, SV, Henderson, C, Perez, CU, Rumerio, P, West, C, Akpinar, A, Albert, A, Arcaro, D, Cosby, C, Demiragli, Z, Fontanesi, E, Gastler, D, May, S, Rohlf, J, Salyer, K, Sperka, D, Spitzbart, D, Suarez, I, Tsatsos, A, Yuan, S, Zou, D, Benelli, G, Burkle, B, Coubez, X, Cutts, D, Hadley, M, Heintz, U, Hogan, JM, Kwon, T, Landsberg, G, Lau, KT, Li, D, Lukasik, M, Luo, J, Narain, M, Pervan, N, Sagir, S, Simpson, F, Usai, E, Wong, WY, Yan, X, Yu, D, Zhang, W, Bonilla, J, Brainerd, C, Breedon, R, Sanchez, MCD, Chertok, M, Conway, J, Cox, PT, Erbacher, R, Haza, G, Jensen, F, Kukral, O, Lander, R, Mulhearn, M, Pellett, D, Regnery, B, Taylor, D, Yao, Y, Zhang, F, Bachtis, M, Cousins, R, Datta, A, Hamilton, D, Hauser, J, Ignatenko, M, Iqbal, MA, Lam, T, Nash, WA, Regnard, S, Saltzberg, D, Stone, B, Valuev, V, Burt, K, Chen, Y, Clare, R, Gary, JW, Gordon, M, Hanson, G, Karapostoli, G, Long, OR, Manganelli, N, Negrete, MO, Si, W, Wimpenny, S, Branson, JG, Chang, P, Cittolin, S, Cooperstein, S, Deelen, N, Diaz, D, Duarte, J, Gerosa, R, Giannini, L, Guiang, J, Kansal, R, Krutelyov, V, Lee, R, Letts, J, Masciovecchio, M, Mokhtar, F, Pieri, M, Narayanan, BVS, Sharma, V, Tadel, M, Vartak, A, Wurthwein, F, Xiang, Y, Yagil, A, Amin, N, Campagnari, C, Citron, M, Dorsett, A, Dutta, V, Incandela, J, Kilpatrick, M, Marsh, B, Mei, H, Oshiro, M, Quinnan, M, Richman, J, Sarica, U, Setti, F, Sheplock, J, Stuart, D, Wang, S, Bornheim, A, Cerri, O, Dutta, I, Lawhorn, JM, Lu, N, Mao, J, Newman, HB, Nguyen, TQ, Spiropulu, M, Vlimant, JR, Wang, C, Xie, S, Zhang, Z, Zhu, RY, Alison, J, An, S, Andrews, MB, Bryant, P, Ferguson, T, Harilal, A, Liu, C, Mudholkar, T, Paulini, M, Sanchez, A, Terrill, W, Cumalat, JP, Ford, WT, Hassani, A, MacDonald, E, Patel, R, Perloff, A, Savard, C, Stenson, K, Ulmer, KA, Wagner, SR, Alexander, J, Bright-Thonney, S, Chen, X, Cheng, Y, Cranshaw, DJ, Hogan, S, Monroy, J, Patterson, JR, Quach, D, Reichert, J, Reid, M, Ryd, A, Sun, W, Thom, J, Wittich, P, Zou, R, Albrow, M, Alyari, M, Apollinari, G, Apresyan, A, Apyan, A, Bauerdick, LAT, Berry, D, Berryhill, J, Bhat, PC, Burkett, K, Butler, JN, Canepa, A, Cerati, GB, Cheung, HWK, Chlebana, F, Di Petrillo, KF, Elvira, VD, Feng, Y, Freeman, J, Gecse, Z, Gray, L, Green, D, Grunendahl, S, Gutsche, O, Harris, RM, Heller, R, Herwig, TC, Hirschauer, J, Jayatilaka, B, Jindariani, S, Johnson, M, Joshi, U, Klijnsma, T, Klima, B, Kwok, KHM, Lammel, S, Lincoln, D, Lipton, R, Liu, T, Madrid, C, Maeshima, K, Mantilla, C, Mason, D, McBride, P, Merkel, P, Mrenna, S, Nahn, S, Ngadiuba, J, O'Dell, V, Papadimitriou, V, Pedro, K, Pena, C, Prokofyev, O, Ravera, F, Hall, AR, Ristori, L, Sexton-Kennedy, E, Smith, N, Soha, A, Spalding, WJ, Spiegel, L, Stoynev, S, Strait, J, Taylor, L, Tkaczyk, S, Tran, NV, Uplegger, L, Vaandering, EW, Weber, HA, Acosta, D, Avery, P, Bourilkov, D, Cadamuro, L, Cherepanov, V, Errico, F, Field, RD, Guerrero, D, Joshi, BM, Kim, M, Koenig, E, Konigsberg, J, Korytov, A, Lo, KH, Matchev, K, Menendez, N, Mitselmakher, G, Madhu, AM, Rawal, N, Rosenzweig, D, Rosenzweig, S, Rotter, J, Shi, K, Sturdy, J, Yigitbasi, E, Zuo, X, Adams, T, Askew, A, Habibullah, R, Hagopian, V, Johnson, KF, Khurana, R, Kolberg, T, Martinez, G, Prosper, H, Schiber, C, Viazlo, O, Yohay, R, Zhang, J, Baarmand, MM, Butalla, S, Elkafrawy, T, Hohlmann, M, Verma, RK, Noonan, D, Rahmani, M, Yumiceva, F, Adams, MR, Gonzalez, HB, Cavanaugh, R, Dittmer, S, Evdokimov, O, Gerber, CE, Hangal, DA, Hofman, DJ, Merrit, AH, Mills, C, Oh, G, Roy, T, Rudrabhatla, S, Tonjes, MB, Varelas, N, Viinikainen, J, Wang, X, Wu, Z, Ye, Z, Alhusseini, M, Dilsiz, K, Gandrajula, RP, Koseyan, OK, Merlo, JP, Mestvirishvili, A, Nachtman, J, Ogul, H, Onel, Y, Penzo, A, Snyder, C, Tiras, E, Amram, O, Blumenfeld, B, Corcodilos, L, Davis, J, Eminizer, M, Gritsan, AV, Kyriacou, S, Maksimovic, P, Roskes, J, Swartz, M, Vami, TA, Abreu, A, Anguiano, J, Barrera, CB, Baringer, P, Bean, A, Bylinkin, A, Flowers, Z, Isidori, T, Khalil, S, King, J, Krintiras, G, Kropivnitskaya, A, Lazarovits, M, Le Mahieu, C, Lindsey, C, Marquez, J, Minafra, N, Murray, M, Nickel, M, Rogan, C, Royon, C, Salvatico, R, Sanders, S, Schmitz, E, Smith, C, Takaki, JDT, Warner, Z, Williams, J, Wilson, G, Duric, S, Ivanov, A, Kaadze, K, Kim, D, Maravin, Y, Mitchell, T, Modak, A, Nam, K, Rebassoo, F, Wright, D, Adams, E, Baden, A, Baron, O, Belloni, A, Eno, SC, Hadley, NJ, Jabeen, S, Kellogg, RG, Koeth, T, Mignerey, AC, Nabili, S, Palmer, C, Seidel, M, Skuja, A, Wang, L, Wong, K, Abercrombie, D, Andreassi, G, Bi, R, Busza, W, Cali, IA, D'Alfonso, M, Eysermans, J, Freer, C, Ceballos, GG, Goncharov, M, Harris, P, Hu, M, Klute, M, Kovalskyi, D, Krupa, J, Lee, YJ, Mironov, C, Paus, C, Rankin, D, Roland, C, Roland, G, Shi, Z, Stephans, GSF, Wang, Z, Wyslouch, B, Chatterjee, RM, Evans, A, Hiltbrand, J, Krohn, M, Kubota, Y, Mans, J, Revering, M, Rusack, R, Saradhy, R, Schroeder, N, Strobbe, N, Wadud, MA, Bloom, K, Bryson, M, Claes, DR, Fangmeier, C, Finco, L, Golf, F, Joo, C, Kravchenko, I, Musich, M, Reed, I, Siado, JE, Snow, GR, Tabb, W, Yan, F, Zecchinelli, AG, Agarwal, G, Bandyopadhyay, H, Hay, L, Iashvili, I, Kharchilava, A, McLean, C, Nguyen, D, Pekkanen, J, Rappoccio, S, Williams, A, Alverson, G, Barberis, E, Haddad, Y, Hortiangtham, A, Li, J, Madigan, G, Marzocchi, B, Morse, DM, Nguyen, V, Orimoto, T, Parker, A, Skinnari, L, Tishelman-Charny, A, Wamorkar, T, Wang, B, Wisecarver, A, Wood, D, Bueghly, J, Chen, Z, Gilbert, A, Gunter, T, Hahn, KA, Liu, Y, Odell, N, Schmitt, MH, Velasco, M, Band, R, Bucci, R, Cremonesi, M, Das, A, Dev, N, Goldouzian, R, Hildreth, M, Anampa, KH, Jessop, C, Lannon, K, Lawrence, J, Loukas, N, Lutton, D, Marinelli, N, Mcalister, I, McCauley, T, Mcgrady, C, Mohrman, K, Moore, C, Musienko, Y, Ruchti, R, Siddireddy, P, Townsend, A, Wayne, M, Wightman, A, Zarucki, M, Zygala, L, Bylsma, B, Cardwell, B, Durkin, LS, Francis, B, Hill, C, Ornelas, MN, Wei, K, Winer, BL, Yates, BR, Addesa, FM, Bonham, B, Das, P, Dezoort, G, Elmer, P, Frankenthal, A, Greenberg, B, Haubrich, N, Higginbotham, S, Kalogeropoulos, A, Kopp, G, Kwan, S, Lange, D, Marlow, D, Mei, K, Ojalvo, I, Olsen, J, Stickland, D, Tully, C, Norberg, S, Bakshi, AS, Barnes, VE, Chawla, R, Das, S, Gutay, L, Jones, M, Jung, AW, Karmarkar, S, Kondratyev, D, Liu, M, Negro, G, Neumeister, N, Paspalaki, G, Piperov, S, Purohit, A, Schulte, JF, Stojanovic, M, Thieman, J, Wang, F, Xiao, R, Xie, W, Dolen, J, Parashar, N, Baty, A, Carnahan, T, Decaro, M, Dildick, S, Ecklund, KM, Freed, S, Gardner, P, Geurts, FJM, Li, W, Padley, BP, Redjimi, R, Shi, W, Leiton, AGS, Zhang, L, Bodek, A, de Barbaro, P, Demina, R, Dulemba, JL, Fallon, C, Ferbel, T, Galanti, M, Garcia-Bellido, A, Hindrichs, O, Khukhunaishvili, A, Ranken, E, Taus, R, Chiarito, B, Chou, JP, Gandrakota, A, Gershtein, Y, Halkiadakis, E, Hart, A, Heindl, M, Karacheban, O, Laflotte, I, Lath, A, Montalvo, R, Nash, K, Osherson, M, Salur, S, Schnetzer, S, Somalwar, S, Stone, R, Thayil, SA, Thomas, S, Wang, H, Acharya, H, Delannoy, AG, Fiorendi, S, Spanier, S, Bouhali, O, Dalchenko, M, Delgado, A, Eusebi, R, Gilmore, J, Huang, T, Kamon, T, Luo, S, Malhotra, S, Mueller, R, Overton, D, Rathjens, D, Safonov, A, Akchurin, N, Damgov, J, Hegde, V, Kunori, S, Lamichhane, K, Mengke, T, Muthumuni, S, Peltola, T, Volobouev, I, Whitbeck, A, Appelt, E, Greene, S, Gurrola, A, Johns, W, Melo, A, Ni, H, Padeken, K, Romeo, F, Sheldon, P, Tuo, S, Velkovska, J, Arenton, MW, Cox, B, Cummings, G, Hakala, J, Hirosky, R, Joyce, M, Ledovskoy, A, Li, A, Neu, C, Lara, CEP, Tannenwald, B, White, S, Wolfe, E, Poudyal, N, Black, K, Bose, T, Caillol, C, Dasu, S, De Bruyn, I, Everaerts, P, Fienga, F, Galloni, C, He, H, Herndon, M, Herve, A, Hussain, U, Lanaro, A, Loeliger, A, Loveless, R, Sreekala, JM, Mallampalli, A, Mohammadi, A, Pinna, D, Savin, A, Shang, V, Smith, WH, Teague, D, Trembath-Reichert, S, Vetens, W, Department of Physics, Helsinki Institute of Physics, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Physics, Elementary Particle Physics, Faculty of Sciences and Bioengineering Sciences, Vriendenkring VUB, Universidad de Cantabria, Tumasyan A., Adam W., Andrejkovic J., Bergauer T., Chatterjee S., Damanakis K., Dragicevic M., Escalante Del Valle A., Frühwirth R., Jeitler M., et al., SCOAP, European Commission, European Research Council, Principado de Asturias, Ministerio de Economía y Competitividad (España), Yerevan Physics Institute, Institut für Hochenergiephysik, Institute for Nuclear Problems, Universiteit Antwerpen, Vrije Universiteit Brussel, Université Libre de Bruxelles, Ghent University, Université Catholique de Louvain, Centro Brasileiro de Pesquisas Fisicas, Universidade do Estado do Rio de Janeiro (UERJ), Universidade Estadual Paulista (UNESP), Bulgarian Academy of Sciences, University of Sofia, Beihang University, Tsinghua University, Institute of High Energy Physics, Peking University, Sun Yat-Sen University, Institute of Modern Physics and Key Laboratory of Nuclear Physics and Ion-beam Application (MOE) — Fudan University, China, Universidad de Los Andes, Universidad de Antioquia, Mechanical Engineering and Naval Architecture, Faculty of Science, Institute Rudjer Boskovic, University of Cyprus, Charles University, Escuela Politecnica Nacional, Universidad San Francisco de Quito, Egyptian Network of High Energy Physics, Fayoum University, National Institute of Chemical Physics and Biophysics, University of Helsinki, Lappeenranta University of Technology, Université Paris-Saclay, Institut Polytechnique de Paris, IPHC UMR 7178, Institut de Physique des 2 Infinis de Lyon (IP2I), Georgian Technical University, I. Physikalisches Institut, III. Physikalisches Institut A, III. Physikalisches Institut B, Deutsches Elektronen-Synchrotron, University of Hamburg, Karlsruher Institut fuer Technologie, NCSR Demokritos, National and Kapodistrian University of Athens, National Technical University of Athens, University of Ioánnina, Eötvös Loránd University, Wigner Research Centre for Physics, Institute of Nuclear Research ATOMKI, University of Debrecen, MATE Institute of Technology, Indian Institute of Science (IISc), HBNI, Panjab University, University of Delhi, Indian Institute of Technology Madras, Bhabha Atomic Research Centre, Tata Institute of Fundamental Research-A, Tata Institute of Fundamental Research-B, Indian Institute of Science Education and Research (IISER), Isfahan University of Technology, Institute for Research in Fundamental Sciences (IPM), University College Dublin, INFN Sezione di Bari, Università di Bari, Politecnico di Bari, INFN Sezione di Bologna, Università di Bologna, INFN Sezione di Catania, Università di Catania, INFN Sezione di Firenze, Università di Firenze, INFN Laboratori Nazionali di Frascati, INFN Sezione di Genova, Università di Genova, INFN Sezione di Milano-Bicocca, Università di Milano-Bicocca, INFN Sezione di Napoli, Università di Napoli ’Federico II’, Università della Basilicata, Università G. Marconi, INFN Sezione di Padova, Università di Padova, INFN Sezione di Pavia, Università di Pavia, INFN Sezione di Perugia, Università di Perugia, INFN Sezione di Pisa, Università di Pisa, Scuola Normale Superiore di Pisa, Università di Siena, INFN Sezione di Roma, Sapienza Università di Roma, INFN Sezione di Torino, Università di Torino, Università del Piemonte Orientale, INFN Sezione di Trieste, Università di Trieste, Kyungpook National University, Institute for Universe and Elementary Particles, Hanyang University, Korea University, Kyung Hee University, Sejong University, Seoul National University, University of Seoul, Yonsei University, Sungkyunkwan University, Kuwait, Riga Technical University, Vilnius University, Universiti Malaya, Universidad de Sonora (UNISON), Centro de Investigacion y de Estudios Avanzados del IPN, Universidad Iberoamericana, Benemerita Universidad Autonoma de Puebla, University of Montenegro, University of Auckland, University of Canterbury, Quaid-I-Azam University, Electronics and Telecommunications, National Centre for Nuclear Research, University of Warsaw, Laboratório de Instrumentação e Física Experimental de Partículas, Joint Institute for Nuclear Research, Petersburg Nuclear Physics Institute, Institute for Nuclear Research, Institute for Theoretical and Experimental Physics named by A.I. Alikhanov of NRC ‘Kurchatov Institute’, Moscow Institute of Physics and Technology, National Research Nuclear University ’Moscow Engineering Physics Institute’ (MEPhI), P.N. Lebedev Physical Institute, Lomonosov Moscow State University, Novosibirsk State University (NSU), Institute for High Energy Physics of National Research Centre ‘Kurchatov Institute’, National Research Tomsk Polytechnic University, Tomsk State University, University of Belgrade: Faculty of Physics and VINCA Institute of Nuclear Sciences, Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Universidad Autónoma de Madrid, Instituto Universitario de Ciencias y Tecnologías Espaciales de Asturias (ICTEA), CSIC-Universidad de Cantabria, University of Colombo, University of Ruhuna, European Organization for Nuclear Research, Paul Scherrer Institut, ETH Zurich — Institute for Particle Physics and Astrophysics (IPA), Universität Zürich, National Central University, National Taiwan University (NTU), Science and Art Faculty, Physics Department, Bogazici University, Istanbul Technical University, Istanbul University, Institute for Scintillation Materials of National Academy of Science of Ukraine, Kharkov Institute of Physics and Technology, University of Bristol, Rutherford Appleton Laboratory, Imperial College, Brunel University, Baylor University, Catholic University of America, The University of Alabama, Boston University, Brown University, Davis, University of California, Riverside, San Diego, Santa Barbara — Department of Physics, California Institute of Technology, Carnegie Mellon University, University of Colorado Boulder, Cornell University, Fermi National Accelerator Laboratory, University of Florida, Florida State University, Florida Institute of Technology, University of Illinois at Chicago (UIC), The University of Iowa, Johns Hopkins University, The University of Kansas, Kansas State University, Lawrence Livermore National Laboratory, University of Maryland, Massachusetts Institute of Technology, University of Minnesota, University of Nebraska-Lincoln, State University of New York at Buffalo, Northeastern University, Northwestern University, University of Notre Dame, The Ohio State University, Princeton University, University of Puerto Rico, Purdue University, Purdue University Northwest, Rice University, University of Rochester, The State University of New Jersey, University of Tennessee, Texas A&M University, Texas Tech University, Vanderbilt University, University of Virginia, Wayne State University, University of Wisconsin — Madison, TU Wien, Technology and Maritime Transport, Universidade Estadual de Campinas (UNICAMP), Federal University of Rio Grande do Sul, The University of the State of Amazonas, University of Chinese Academy of Sciences, Universidade Federal de Mato Grosso do Sul (UFMS), Nanjing Normal University Department of Physics, Suez University, British University in Egypt, Cairo University, Université de Haute Alsace, Tbilisi State University, Erzincan Binali Yildirim University, Brandenburg University of Technology, Forschungszentrum Jülich, Assiut University, IIT Bhubaneswar, Institute of Physics, Punjab Agricultural University, Shoolini University, University of Hyderabad, University of Visva-Bharati, Indian Institute of Technology (IIT), Sharif University of Technology, University of Science and Technology of Mazandaran, Energy and Sustainable Economic Development, Centro Siciliano di Fisica Nucleare e di Struttura Della Materia, Consiglio Nazionale delle Ricerche — Istituto Officina dei Materiali, Consejo Nacional de Ciencia y Tecnología, Institute of Nuclear Physics of the Uzbekistan Academy of Sciences, St. Petersburg Polytechnic University, Budker Institute of Nuclear Physics, University of Belgrade, Sri Lanka, Ecole Polytechnique Fédérale Lausanne, Stefan Meyer Institute for Subatomic Physics, IN2P3-CNRS, Şırnak University, Research Center of Experimental Health Science, Konya Technical University, Piri Reis University, Adiyaman University, Ozyegin University, Necmettin Erbakan University, Bozok Universitetesi Rektörlügü, Marmara University, Milli Savunma University, Kafkas University, Istanbul Bilgi University, Hacettepe University, Faculty of Engineering, University of Southampton, IPPP Durham University, Bethel University, Karamanoğlu Mehmetbey University, Ain Shams University, Bingol University, Sinop University, Erciyes University, Texas A&M University at Qatar, Università di Trento, CERN, Andrejkovic, J, Escalante Del Valle, A, Pitters, F, Wulz, C, Darwish, M, De Wolf, E, Rejeb Sfar, H, Bols, E, Sahasransu, A, Kalsi, A, Donertas, I, Tran, T, Alves, G, Alda Junior, W, Alves Gallo Pereira, M, Barroso Ferreira Filho, M, Brandao Malbouisson, H, Da Costa, E, Da Silveira, G, De Jesus Damiao, D, Fonseca De Souza, S, Mora Herrera, C, Mota Amarilo, K, Rebello Teles, P, Silva Do Amaral, S, Torres Da Silva De Araujo, F, Vilela Pereira, A, Bernardes, C, Fernandez Perez Tomei, T, Gregores, E, Lemos, D, Mercadante, P, Novaes, S, Padula, S, Chen, G, Chen, H, Liu, Z, Qian, S, Mejia Guisao, J, Ruiz Alvarez, J, Salazar Gonzalez, C, Razis, P, Carrera Jarrin, E, Ellithi Kamel, A, Mahmoud, M, Dewanjee, R, Faure, J, Hamel de Monchenault, G, Sahin, M, Yu, G, Buchot Perraguin, A, Granier de Cassagnac, R, Sauvan, J, Agram, J, Brom, J, Chabert, E, Fontaine, J, Le Bihan, A, Laktineh, I, Schuler, S, Haj Ahmad, W, Aarup Petersen, H, Aldaya Martin, M, Bermudez Martinez, A, Bin Anuar, A, Consuegra Rodriguez, S, Correia Silva, G, Estevez Banos, L, Jomhari, N, Melzer-Pellmann, I, Mendizabal Morentin, M, Perez Adan, D, Ribeiro Lopes, B, Sosa Ricardo, R, Pena Rodriguez, K, Gosewisch, J, Simonis, H, Von Cube, R, Koraka, C, Gadallah, M, Radl, A, Veres, G, Trocsanyi, Z, Komaragiri, J, Tiwari, P, Muraleedharan Nair Bindhu, V, Swain, S, Beri, S, Singh, J, Virdi, A, Choudhary, B, Rout, P, Behera, P, Behera, S, Pujahari, P, Sikdar, A, Mishra, D, Netrakanti, P, Pant, L, Etesami, S, Mohammadi Najafabadi, M, Simone, F, Cavallo, F, Dallavalle, G, Navarria, F, Siroli, G, Dinardo, M, Lucchini, M, Pinolini, B, Tabarelli de Fatis, T, Iorio, A, Hoh, S, Meneguzzo, A, Aime', C, Ratti, S, Bilei, G, Ciocci, M, Di Domenico, M, Matos Figueiredo, D, Roy Chowdhury, S, Verdini, P, Berenguer Antequera, J, Obertino, M, Pinna Angioni, G, Kim, G, Moon, C, Oh, Y, Pak, S, Radburn-Smith, B, Yang, Y, Moon, D, Kim, T, Park, S, Bhyun, J, Oh, B, Oh, S, Yang, U, Kang, D, Merlin, J, Park, I, Ryu, M, Watson, I, Yoo, H, Carvalho Antunes De Oliveira, A, Norjoharuddeen, N, Wan Abdullah, W, Yusli, M, Benitez, J, Castaneda Hernandez, A, Leon Coello, M, Murillo Quijada, J, Valencia Palomo, L, Mondragon Herrera, C, Perez Navarro, D, Sanchez Hernandez, A, Carrillo Moreno, S, Oropeza Barrera, C, Vazquez Valencia, F, Salazar Ibarguen, H, Uribe Estrada, C, Butler, P, Asghar, M, Awan, M, Hoorani, H, Khan, W, Shah, M, Yuldashev, B, Alcaraz Maestre, J, Alvarez Fernandez, A, Barrio Luna, M, Bedoya, C, Carrillo Montoya, C, Delgado Peris, A, Fernandez Ramos, J, Fouz, M, Gonzalez Lopez, O, Goy Lopez, S, Hernandez, J, Josa, M, Leon Holgado, J, Navarro Tobar, A, Perez Dengra, C, Perez-Calero Yzquierdo, A, Puerta Pelayo, J, Sanchez Navas, S, Urda Gomez, L, de Troconiz, J, Alvarez Gonzalez, B, Fernandez Menendez, J, Gonzalez Caballero, I, Gonzalez Fernandez, J, Palencia Cortezon, E, Ramon Alvarez, C, Rodriguez Bouza, V, Soto Rodriguez, A, Vico Villalba, C, Brochero Cifuentes, J, Cabrillo, I, Duarte Campderros, J, Fernandez Madrazo, C, Fernandez Manteca, P, Garcia Alonso, A, Martinez Rivero, C, Martinez Ruiz del Arbol, P, Matorras Cuevas, P, Piedra Gomez, J, Vizan Garcia, J, Jayananda, M, Sonnadara, D, Wickramarathna, D, Dharmaratna, W, Aarrestad, T, Capeans Garrido, M, Chhibra, S, D'Enterria, D, Defranchis, M, Marini, A, Reales Gutierrez, G, Tavolaro, V, Van Onsem, G, Wozniak, K, Zeuner, W, Kaestli, H, Gomez Espinosa, T, Lyon, A, Manzoni, R, Martin Perez, C, Meinhard, M, Ratti, M, Sanz Becerra, D, Zhu, D, Canelli, M, Heikkila, J, Liechti, S, Mikuni, V, Sanchez Cruz, S, Kuo, C, Yu, S, Chen, K, Chen, P, Hou, W, Li, Y, Lu, R, Wu, H, Yu, P, Demiroglu, Z, Gurpinar Guler, E, Kayis Topaksu, A, Simsek, A, Tok, U, Zorbakir, I, Atakisi, I, Yetkin, E, Sunar Cerci, D, Brooke, J, Heath, G, Heath, H, Seif El Nasr-Storey, S, Smith, V, Walkingshaw Pass, K, Bell, K, Brown, R, Cockerill, D, Ellis, K, Holmberg, M, Newbold, D, Shepherd-Themistocleous, C, Tomalin, I, Chahal, G, Hassanshahi, M, Magnan, A, Monk, D, Raymond, D, Webb, S, Cole, J, Reid, I, Kanuganti, A, Mcmaster, B, Vargas Hernandez, A, Cooper, S, Gleyzer, S, Perez, C, Hogan, J, Lau, K, Wong, W, Calderon De La Barca Sanchez, M, Cox, P, Iqbal, M, Nash, W, Gary, J, Long, O, Olmedo Negrete, M, Branson, J, Sathia Narayanan, B, Lawhorn, J, Newman, H, Nguyen, T, Vlimant, J, Zhu, R, Andrews, M, Cumalat, J, Ford, W, Macdonald, E, Ulmer, K, Wagner, S, Cranshaw, D, Patterson, J, Bauerdick, L, Bhat, P, Butler, J, Cerati, G, Cheung, H, Di Petrillo, K, Elvira, V, Harris, R, Herwig, T, Kwok, K, Mcbride, P, Reinsvold Hall, A, Spalding, W, Tran, N, Vaandering, E, Weber, H, Field, R, Joshi, B, Lo, K, Muthirakalayil Madhu, A, Johnson, K, Baarmand, M, Kumar Verma, R, Adams, M, Becerril Gonzalez, H, Gerber, C, Hangal, D, Hofman, D, Merrit, A, Tonjes, M, Gandrajula, R, Koseyan, O, Merlo, J, Gritsan, A, Vami, T, Baldenegro Barrera, C, Tapia Takaki, J, Eno, S, Hadley, N, Kellogg, R, Mignerey, A, Cali, I, Gomez Ceballos, G, Stephans, G, Chatterjee, R, Wadud, M, Claes, D, Siado, J, Snow, G, Zecchinelli, A, Mclean, C, Morse, D, Hahn, K, Schmitt, M, Hurtado Anampa, K, Mccauley, T, Zygala, B, Durkin, L, Nunez Ornelas, M, Winer, B, Yates, B, Addesa, F, Bakshi, A, Barnes, V, Jung, A, Schulte, J, Ecklund, K, Geurts, F, Padley, B, Stahl Leiton, A, Dulemba, J, Chou, J, Thayil, S, Delannoy, A, Arenton, M, Perez Lara, C, Madhusudanan Sreekala, J, Smith, W, Sağır, Sinan, Belforte, S., Candelise, V., Casarsa, M., Cossutti, F., DA ROLD, A., DELLA RICCA, G., Sorrentino, G., Vazzoler, F., and ET AL (the CMS, Collaboration)
- Subjects
13000 GeV-cms ,Temel Bilimler (SCI) ,parton: distribution function ,transverse momentum [jet] ,PARTICLE PHYSICS ,LARGE HADRON COLLIDER ,CMS ,Physics, Particles & Fields ,rapidity dependence ,Hadron-Hadron Scattering ,Jet Physics ,effective field theory ,strong interaction: coupling constant ,scattering [p p] ,PROGRAM ,jet, production ,High energy physics ,Experimental particle physics ,LHC ,p p: scattering ,p p: colliding beams ,B: decay ,tau: hadronic decay ,interaction: gauge ,interaction: model ,transverse momentum: missing-energy ,new physics: search for ,mass spectrum: transverse ,black hole: quantum ,vector boson: mass ,W': leptonic decay ,sensitivity ,leptoquark: coupling ,CERN LHC Coll ,leptoquark: mass: lower limit ,anomaly ,channel cross section: upper limit ,Higgs ,Nuclear Experiment ,протон-протонные столкновения ,parton, distribution function ,двойные дифференциальные инклюзивные струи ,Physics ,QUARK ,perturbation theory: higher-order ,contact interaction ,PHYSICS, NUCLEAR ,2 [higher-order] ,higher-order, 2 ,higher-order, 1 ,track data analysis: jet ,Physical Sciences ,hadroproduction [jet] ,colliding beams [p p] ,distribution function [parton] ,coupling constant [strong interaction] ,1 [higher-order] ,p p, scattering ,strong interaction, coupling constant ,114 Physical sciences ,quark ,phase space ,FİZİK, NÜKLEER ,Z0, mass ,quantum chromodynamics ,strong coupling ,TeV ,ddc:530 ,0206 Quantum Physics ,Science & Technology ,higher-order [perturbation theory] ,jet: rapidity ,ATLAS, детектор ,Большой адронный коллайдер ,GeV ,jet: transverse momentum ,transverse momentum dependence ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,SINGLET ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,jet [track data analysis] ,0105 Mathematical Physics ,Temel Bilimler ,Wilson ,higher-order: 2 ,higher-order: 1 ,jet, rapidity ,Nuclear & Particles Physics ,Nükleer ve Yüksek Enerji Fiziği ,Natural Sciences (SCI) ,rapidity [jet] ,0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics ,Natural Sciences ,Particle Physics - Experiment ,perturbation theory [quantum chromodynamics] ,Nuclear and High Energy Physics ,data analysis method ,jet, transverse momentum ,FOS: Physical sciences ,Fizik ,PARTON DENSITIES ,COMPUTATION ,differential cross section: measured ,PHYSICS ,measured [differential cross section] ,quantum chromodynamics: perturbation theory ,hep-ex ,High Energy Physics::Phenomenology ,3-LOOP SPLITTING FUNCTIONS ,jet: hadroproduction ,EVOLUTION ,Physics and Astronomy ,Fizik Bilimleri ,High Energy Physics::Experiment ,experimental results - Abstract
A measurement of the inclusive jet production in proton-proton collisions at the LHC at √s = 13 TeV is presented. The double-differential cross sections are measured as a function of the jet transverse momentum pT and the absolute jet rapidity |y|. The anti-kT clustering algorithm is used with distance parameter of 0.4 (0.7) in a phase space region with jet pT from 97 GeV up to 3.1 TeV and |y| < 2.0. Data collected with the CMS detector are used, corresponding to an integrated luminosity of 36.3 fb−1 (33.5 fb−1). The measurement is used in a comprehensive QCD analysis at next-to-next-to-leading order, which results in significant improvement in the accuracy of the parton distributions in the proton. Simultaneously, the value of the strong coupling constant at the Z boson mass is extracted as αS(mZ) = 0.1170±0.0019. For the first time, these data are used in a standard model effective field theory analysis at next-to-leading order, where parton distributions and the QCD parameters are extracted simultaneously with imposed constraints on the Wilson coefficient c1 of 4-quark contact interactions., Individuals have received support from the Marie-Curie programme and the European Research Council and Horizon 2020 Grant, contract Nos. 675440, 724704, 752730, 758316, 765710, 824093, 884104, and COST Action CA16108 (European Union); the Leventis Foundation; the Alfred P. Sloan Foundation; the Alexander von Humboldt Foundation;the Belgian Federal Science Policy Office; the Fonds pour la Formation à la Recherche dans l’Industrie et dans l’Agriculture (FRIA-Belgium); the Agentschap voor Innovatie door Wetenschap en Technologie (IWT-Belgium); the F.R.S.-FNRS and FWO (Belgium) under the “Excellence of Science — EOS” — be.h project n. 30820817; the Beijing Municipal Science & Technology Commission, No. Z191100007219010; the Ministry of Education, Youth and Sports (MEYS) of the Czech Republic; the Deutsche Forschungsgemeinschaft (DFG), under Germany’s Excellence Strategy — EXC 2121 “Quantum Universe” — 390833306, and under project number 400140256 - GRK2497; the Lendület (“Momentum”) Programme and the János Bolyai Research Scholarship of the Hungarian Academy of Sciences, the New National Excellence Program ÚNKP, the NKFIA research grants 123842, 123959, 124845, 124850, 125105, 128713, 128786, and 129058 (Hungary); the Council of Science and Industrial Research, India; the Latvian Council of Science; the Ministry of Science and Higher Education and the National Science Center, contracts Opus 2014/15/B/ST2/03998 and 2015/19/B/ST2/02861 (Poland); the Fundação para a Ciência e a Tecnologia, grant CEECIND/01334/2018 (Portugal); the National Priorities Research Program by Qatar National Research Fund; the Ministry of Science and Higher Education, projects no. 14.W03.31.0026 and no. FSWW-2020-0008, and the Russian Foundation for Basic Research, project No.19-42-703014 (Russia); the Programa Estatal de Fomento de la Investigación Científica y Técnica de Excelencia María de Maeztu, grant MDM-2015-0509 and the Programa Severo Ochoa del Principado de Asturias; the Stavros Niarchos Foundation (Greece); the Rachadapisek Sompot Fund for Postdoctoral Fellowship, Chulalongkorn University and the Chulalongkorn Academic into Its 2nd Century Project Advancement Project (Thailand); the Kavli Foundation; the Nvidia Corporation; the SuperMicro Corporation; the Welch Foundation, contract C-1845; and the Weston Havens Foundation (U.S.A.)., Article funded by SCOAP3.
- Published
- 2022
- Full Text
- View/download PDF
17. The Dust Halo of Saturn's Largest Icy Moon, Rhea
- Author
-
Jones, G. H., Roussos, E., Krupp, N., Beckmann, U., Coates, A. J., Crary, F., Dandouras, I., Dikarev, V., Dougherty, M. K., Garnier, P., Hansen, C. J., Hendrix, A. R., Hospodarsky, G. B., Johnson, R. E., Kempf, S., Khurana, K. K., Krimigis, S. M., Krüger, H., Kurth, W. S., Lagg, A., McAndrews, H. J., Mitchell, D. G., Paranicas, C., Postberg, F., Russell, C. T., Saur, J., Seiß, M., Spahn, F., Srama, R., Strobel, D. F., Tokar, R., Wahlund, J.-E., Wilson, R. J., Woch, J., and Young, D.
- Published
- 2008
- Full Text
- View/download PDF
18. Timing and Duration of Traffic-related Air Pollution Exposure and the Risk for Childhood Wheeze and Asthma
- Author
-
Brunst, Kelly J., Ryan, Patrick H., Brokamp, Cole, Bernstein, David, Reponen, Tiina, Lockey, James, Hershey, Gurjit Khurana K., Levin, Linda, Grinshpun, Sergey A., and LeMasters, Grace
- Published
- 2015
- Full Text
- View/download PDF
19. Magnetic Field Studies of the Solar Wind Interaction with Venus from the Galileo Flyby
- Author
-
Kivelson, M. G., Kennel, C. F., McPherron, R. L., Russell, C. T., Southwood, D. J., Walker, R. J., Hammond, C. M., Khurana, K. K., Strangeway, R. J., and Coleman, P. J.
- Published
- 1991
20. Magnetic Field Signatures Near Galileo's Closest Approach to Gaspra
- Author
-
Kivelson, M. G., Bargatze, L. F., Khurana, K. K., Southwood, D. J., Walker, R. J., and Coleman,, P. J.
- Published
- 1993
21. Radial and Local Time Variations in the Thickness of Jupiter's Magnetospheric Current Sheet.
- Author
-
Khurana, K. K., Leinweber, H. K., Hospodarsky, G. B., and Paranicas, C. P.
- Subjects
CURRENT sheets ,INTERPLANETARY magnetic fields ,MAGNETIC reconnection ,MAGNETIC flux ,MAGNETIC fields ,SOLAR wind - Abstract
The magnetic field observations from the Galileo, Ulysses, Voyager 1 and 2, and Pioneer 10 and 11 spacecraft are analyzed to understand the structures and thickness of the Jovian magnetospheric current sheet. Using a new technique that can determine the motion of the spacecraft relative to the current sheet, we have built the first global map of the thickness of the Jovian magnetospheric current sheet. We show that the current sheet thickness in Jupiter's magnetosphere is not equal everywhere but changes systematically with both radial distance and local time. The extremely thin dawnside current sheet appears to be linked to the stresses imposed by the solar wind on the open magnetic flux housed in the lobes of the magnetosphere in that sector. We also show evidence of a mostly closed magnetosphere in the dusk sector. We show that the current sheet thickness asymmetries likely arise from a field and plasma convection system set up by the reconnection of the interplanetary magnetic field with that of Jupiter. [ABSTRACT FROM AUTHOR]
- Published
- 2022
- Full Text
- View/download PDF
22. Lunar Hydrospheric Explorer (HYDROX)
- Author
-
Cooper, J. F, Paschalidis, N, Sittler, E. C., Jr, Jones, S. L, Stubbs, T. J, Sarantos, M, Khurana, K. K, Angelopoulos, V, Jordan, A. P, and Schwadron, N. A
- Subjects
Lunar And Planetary Science And Exploration - Abstract
The Lunar Hydrospheric Explorer (HYDROX) is a 6U CubeSat designed to further confirm the existence of lunar exospheric water, and to determine source processes and surface sites, through ion mass spectrometer measurements of water group (O+, OH+, H2O+) and related ions at energy charge up to 2 keV/e. and mass/charge 1-40amu/e. HYDROX would follow up on the now-concluded exospheric compositional measurements by the Neutral Mass Spectrometer on the NASA LADEE mission and on other remote sensing surface and exospheric measurements (LADEE,LRO, etc.).
- Published
- 2015
23. ARTEMIS Science Objectives
- Author
-
Sibeck, D. G., Angelopoulos, V., Brain, D. A., Delory, G. T., Eastwood, J. P., Farrell, W. M., Grimm, R. E., Halekas, J. S., Hasegawa, H., Hellinger, P., Khurana, K. K., Lillis, R. J., Øieroset, M., Phan, T.-D., Raeder, J., Russell, C. T., Schriver, D., Slavin, J. A., Travnicek, P. M., and Weygand, J. M.
- Published
- 2011
- Full Text
- View/download PDF
24. Mapping Magnetospheric Equatorial Regions at Saturn from Cassini Prime Mission Observations
- Author
-
Arridge, C. S., André, N., McAndrews, H. J., Bunce, E. J., Burger, M. H., Hansen, K. C., Hsu, H.-W., Johnson, R. E., Jones, G. H., Kempf, S., Khurana, K. K., Krupp, N., Kurth, W. S., Leisner, J. S., Paranicas, C., Roussos, E., Russell, C. T., Schippers, P., Sittler, E. C., Smith, H. T., Thomsen, M. F., and Dougherty, M. K.
- Published
- 2011
- Full Text
- View/download PDF
25. First Results from ARTEMIS, a New Two-Spacecraft Lunar Mission: Counter-Streaming Plasma Populations in the Lunar Wake
- Author
-
Halekas, J. S., Angelopoulos, V., Sibeck, D. G., Khurana, K. K., Russell, C. T., Delory, G. T., Farrell, W. M., McFadden, J. P., Bonnell, J. W., Larson, D., Ergun, R. E., Plaschke, F., and Glassmeier, K. H.
- Published
- 2011
- Full Text
- View/download PDF
26. Energetic electron signatures of Saturn's smaller moons: Evidence of an arc of material at Methone
- Author
-
Roussos, E., Jones, G.H., Krupp, N., Paranicas, C., Mitchell, D.G., Krimigis, S.M., Woch, J., Lagg, A., and Khurana, K.
- Published
- 2008
- Full Text
- View/download PDF
27. Environments in the Outer Solar System
- Author
-
Krupp, N., Khurana, K. K., Iess, L., Lainey, V., Cassidy, T. A., Burger, M., Sotin, C., and Neubauer, F.
- Published
- 2010
- Full Text
- View/download PDF
28. First Results from ARTEMIS, A New Two-Spacecraft Lunar Mission: Counter-Streaming Plasma Populations in the Lunar Wake
- Author
-
Halekas, J. S, Angelopoulos, V, Sibeck, D. G, Khurana, K. K, Russell, C. T, Delory, G. T, Farrell, W. M, McFadden, J. P, Bonnell, J. W, Larson, D, Ergun, R. E, Plaschke, F, and Glassmeier, K. H
- Subjects
Plasma Physics ,Astrophysics ,Lunar And Planetary Science And Exploration - Abstract
We present observations from the first passage through the lunar plasma wake by one of two spacecraft comprising ARTEMIS (Acceleration, Reconnection, Turbulence, and Electrodynamics of the Moon's Interaction with the Sun), a new lunar mission that re-tasks two of five probes from the THEMIS magnetospheric mission. On Feb 13, 2010, ARTEMIS probe P1 passed through the wake at approximately 3.5 lunar radii downstream from the Moon, in a region between those explored by Wind and the Lunar Prospector, Kaguya, Chandrayaan, and Chang'E missions. ARTEMIS observed interpenetrating proton, alpha particle, and electron populations refilling the wake along magnetic field lines from both flanks. The characteristics of these distributions match expectations from self-similar models of plasma expansion into vacuum, with an asymmetric character likely driven by a combination of a tilted interplanetary magnetic field and an anisotropic incident solar wind electron population. On this flyby, ARTEMIS provided unprecedented measurements of the interpenetrating beams of both electrons and ions naturally produced by the filtration and acceleration effects of electric fields set up during the refilling process. ARTEMIS also measured electrostatic oscillations closely correlated with counter-streaming electron beams in the wake, as previously hypothesized but never before directly measured. These observations demonstrate the capability of the comprehensively instrumented ARTEMIS spacecraft and the potential for new lunar science from this unique two spacecraft constellation.
- Published
- 2014
- Full Text
- View/download PDF
29. Anti-planetward auroral electron beams at Saturn
- Author
-
Saur, J., Mauk, B. H., Mitchell, D. G., Krupp, N., Khurana, K. K., Livi, S., Krimigis, S. M., Newell, P. T., Williams, D. J., Brandt, P. C., Lagg, A., Roussos, E., and Dougherty, M. K.
- Subjects
Environmental issues ,Science and technology ,Zoology and wildlife conservation - Abstract
Author(s): J. Saur (corresponding author) [1, 5]; B. H. Mauk [1]; D. G. Mitchell [1]; N. Krupp [2]; K. K. Khurana [3]; S. Livi [1]; S. M. Krimigis [1]; P. [...]
- Published
- 2006
- Full Text
- View/download PDF
30. Some studies of magnetohydrodynamic oscillations of a rotating fluid
- Author
-
Khurana, K. K.
- Subjects
532 ,Fluid mechanics - Abstract
Some theoretical studies on the propagation of Rossby-MHD waves in homogeneous media and the reflection of Rossby-MHD and inertial-MHD waves at rigid boundaries are presented. The evolution of an initial Rossby-MHD disturbance on a beta-plane is studied by the method of stationary phase in two dimensions. For positive β, long wavelength magnetic modes of this wave travel eastwards and propagate in a triangular region of the beta-plane. To an observer moving with the group velocity of a particular wave, its amplitude appears to diminish with time t as a function of t(^-1).The reflection of a Rossby-MHD wave by a conducting or insulating rigid boundary generates two reflected modes, one of which may be a non-propagating wave. The wavenumbers, group velocities, magnetic/kinetic energy ratios and energy densities of the incident and reflected waves are, in general, different. For waves of planetary dimensions, an eastwards travelling magnetic mode, on reflection from a N-S boundary, is transformed entirely into a long wavelength inertial mode and a large conversion of magnetic energy into kinetic energy is observed. An inertial-MHD wave on reflection from a conducting or an insulating rigid boundary splits up into three reflected modes one of which is always a travelling magnetic mode. The wavenumbers, group velocities, magnetic to kinetic energy ratios and energy densities of the incident and reflected waves are not equal. Although, the reflection of any of these modes always generates a reflected magnetic mode, no travelling inertial modes may be generated for certain orientations of the boundary. In the long term this phenomenon will increase the share of the energy of the magnetic modes at the expense of the inertial modes.
- Published
- 1984
31. Jovian plasma sheet morphology: particle and field observations by the Galileo spacecraft
- Author
-
Waldrop, L.S., Fritz, T.A., Kivelson, M.G., Khurana, K., Krupp, N., and Lagg, A.
- Published
- 2005
- Full Text
- View/download PDF
32. Tidal Heating: Lessons from Io and the Jovian System (Report from the KISS Workshop)
- Author
-
Park, R. S., de Kleer, K., McEwen, A., Bierson, C. J., Davies, A. G., DellaGiustina, D., Ermakov, A. I., Fuller, J., Hamilton, C., Harris, C., Hay, H., Jacobson, R. A., Keane, J., Kestay, L., Khurana, K., Kirby, K., Stevenson, D., Tsai, V. C., and Turtle, E.
- Abstract
Summary of the Keck Institute for Space Studies workshop entitled "Tidal Heating: Lessons from Io and the Jovian System," held on October 15-19, 2018.
- Published
- 2019
33. The IO Volcano Observer (IVO): Follow the Heat
- Author
-
McEwen, A., Turtle, E., Kestay, Lazlo, Khurana, K., Westlake, J.H., Wurz, P, Helbert, Jörn, Park, R., Kirby, K., Haapala-Chalk, A, Breuer, Doris, Davies, A., Paranicas, C, Nimmo, F., and Perry, J.
- Subjects
Planetenphysik ,Leitungsbereich PF ,Io ,Volcano ,Observer ,IVO - Published
- 2019
34. Cassini Observations of Saturn's Magnetotail Region: Preliminary Results
- Author
-
Sittler, E. C, Arridge, C, Rymer, A, Coates, A, Krupp, N, Blanc, M, Richardson, J, Andre, N, Thomsen, M, Tokar, R. L, McAndrews, H. J, Henderson, Mike, Cooper, J. F, Burger, M, Simpson, D, Khurana, K. K, Russell, C, Dougherty, M, and Young, D. T
- Subjects
Lunar And Planetary Science And Exploration - Abstract
Using Cassini thermal plasma, hot plasma and magnetic field observations for several intervals between the dawn meridian of Saturn's outer magnetosphere and Saturn's magnetotail region, we investigate the structure of the magnetotail, plasma and magnetic field properties within tail-like current sheet regions and ion flows within the magnetotail regions. We use Cassini Plasma Spectrometer (CAPS) Ion Mass Spectrometer (IMS), Electron Plasma Spectrometer (ELS) observations, MIMI LEMMS ion and electron observations and Cassini magnetometer data (MAG) to characterize the plasma environment. IMS observations are used to measure plasma flow velocities from which one can infer rotation versus convective flows. IMS composition measurements are used to trace the source of plasma from the inner magnetosphere (protons, H2+ and water group ions) versus an external solar wind source (protons and ~ e +i+on s). A critical parameter for both models is the strength of the convection electric field with respect to the rotational electric field for the large scale magnetosphere. For example, are there significant return flows (i.e., negative radial velocities, VR < 0) and/or plasmoids (V(sub R) > 0) within the magnetotail region? Initial preliminary evidence of such out flows and return flows was presented by Sittler et al. This talk complements the more global analysis by McAndrews et al.
- Published
- 2007
35. The Galileo magnetic field investigation
- Author
-
Kivelson, M. G., Khurana, K. K., Means, J. D., Russell, C. T., and Snare, R. C.
- Published
- 1992
- Full Text
- View/download PDF
36. Cassini Observations of Saturn's Dawn-Magnetotail Region and their Relation to Models of Saturn's Aurora: Preliminary Results
- Author
-
Sittler, E. C, Blanc, M. F, Richardson, J. D, Rymer, A, Thomsen, M, Cooper, J. F, Simpson, D, Khurana, K. K, and Dougherty, M
- Subjects
Astrophysics - Abstract
Using Cassini plasma and magnetic field observations from the dawn meridian of Saturn s outer magnetosphere to Saturn s magnetotail region, we investigate the applicability of the centrifugal instability model by Sittler et al. [2006] for Saturn s auroral response to the solar wind, versus the reconnection model of Saturn s aurora by Cowley et al. [2005]. We use Cassini Plasma Spectrometer (CAPS) Ion Mass Spectrometer (IMS) and Electron Plasma Spectrometer (ELS) observations to characterize the plasma environment. ELS and magnetometer observations are used to map out the morphology of the outer magnetosphere from dawn to midnight local time. IMS observations are used to measure plasma flow velocities from which one can infer rotation versus convective flows. IMS composition measurements are used to trace the source of plasma from the inner magnetosphere (protons, H2 and water group ions) versus an external solar wind source (protons and Heff ions). A critical parameter for both models is the strength of the convection electric field with respect to the rotational electric field for the large scale magnetosphere. Is there a significant return flow from the magnetotail? Pitch angle distributions also play an important role as a discriminator. If the magnetosphere tends to conserve angular momentum as suggested by Sittler et al. [2006], then we expect to see an anti-correlation between rotational flow component and radial flow velocities. All will be investigated.
- Published
- 2006
37. Dynamic Harris current sheet thickness from Cluster current density and plasma measurements
- Author
-
Thompson, S. M, Kivelson, M. G, Khurana, K. K, McPherron, R. L, Weygand, J. M, Balogh, A, Reme, H, and Kistler, L. M
- Subjects
Geophysics - Abstract
We use the first accurate measurements of current densities in the plasma sheet to calculate the half-thickness and position of the current sheet as a function of time. Our technique assumes a Harris current sheet model, which is parameterized by lobe magnetic field B(o), current sheet half-thickness h, and current sheet position z(sub o). Cluster measurements of magnetic field, current density, and plasma pressure are used to infer the three parameters as a function of time. We find that most long timescale (6-12 hours) current sheet crossings observed by Cluster cannot be described by a static Harris current sheet with a single set of parameters B(sub o), h, and z(sub o). Noting the presence of high-frequency fluctuations that appear to be superimposed on lower frequency variations, we average over running 6-min intervals and use the smoothed data to infer the parameters h(t) and z(sub o)(t), constrained by the pressure balance lobe magnetic field B(sub o)(t). Whereas this approach has been used in previous studies, the spatial gnuhen& now provided by the Cluster magnetometers were unavailable or not well constrained in earlier studies. We place the calculated hdf&cknessa in a magnetospheric context by examining the change in thickness with substorm phase for three case study events and 21 events in a superposed epoch analysis. We find that the inferred half-thickness in many cases reflects the nominal changes experienced by the plasma sheet during substorms (i.e., thinning during growth phase, thickening following substorm onset). We conclude with an analysis of the relative contribution of (Delta)B(sub z)/(Delta)X to the cross-tail current density during substorms. We find that (Delta)B(sub z)/(Delta)X can contribute a significant portion of the cross-tail c m n t around substorm onset.
- Published
- 2005
38. Plasma sheet turbulence observed by Cluster II
- Author
-
Weygand, James M, Kivelson, M. G, Khurana, K. K, Schwarzl, H. K, Thompson, S. M, McPherron, R. L, Balogh, A, Kistler, L. M, Goldstein, M. L, and Borovsky, J
- Subjects
Geophysics - Abstract
Cluster fluxgate magnetometer (FGM) and ion spectrometer (CIS) data are employed to analyze magnetic field fluctuations within the plasma sheet during passages through the magnetotail region in the summers of 2001 and 2002 and, in particular, to look for characteristics of magnetohydrodynamic (MHD) turbulence. Power spectral indices determined from power spectral density functions are on average larger than Kolmogorov's theoretical value for fluid turbulence as well as Kraichnan's theoretical value for MHD plasma turbulence. Probability distribution functions of the magnetic fluctuations show a scaling law over a large range of temporal scales with non-Gaussian distributions at small dissipative scales and inertial scales and more Gaussian distribution at large driving scales. Furthermore, a multifractal analysis of the magnetic field components shows scaling behavior in the inertial range of the fluctuations from about 20 s to 13 min for moments through the fifth order. Both the scaling behavior of the probability distribution functions and the multifractal structure function suggest that intermittent turbulence is present within the plasma sheet. The unique multispacecraft aspect and fortuitous spacecraft spacing allow us to examine the turbulent eddy scale sizes. Dynamic autocorrelation and cross correlation analysis of the magnetic field components allow us to determine that eddy scale sizes fit within the plasma sheet. These results suggest that magnetic field turbulence is occurring within the plasma sheet resulting in turbulent energy dissipation.
- Published
- 2005
39. The response of the near earth magnetotail to substorm activity
- Author
-
Kivelson, M. G, McPherron, R. L, Thompson, S, Khurana, K. K, Weygand, J. M, and Balogh, Andrew
- Subjects
Geophysics - Abstract
The large scale structure of the current sheet in the terrestrial magnetotail is often represented as the superposition of a constant northward-oriented magnetic field component (B(sub z)) and a component along the Earth-Sun direction (B(sub x)) that varies with distance from the center of the sheet (z(sub o) in GSM) as in a Hams neutral sheet. The latter implies that B(sub x) = B(sub Lx) tanh((z - z(sub o))/h) where B(sub Lx) is the magnitude of the B(sub x) component in the northern lobe. Correspondingly, the cross-tail current should be approximated by J(sub y) = (B(sub Lx)/h) sech(sup 2)((z - z(sub o))/h). Using data from the fluxgate magnetometer (FGM) on the Cluster I1 spacecraft tetrad, we have used measured fields and currents to ask if this model represents the large-scale properties of the system. During very quiet crossings of the plasmasheet, we find that the model gives a reasonable estimate of the trend of the average current and field distributions, but during disturbed intervals, the best fit fails to represent the data. If, however, the parameters z(sub o) and h of the model are taken as variable functions of time, the fits can be reasonably good. The temporal variation of the fit parameter h that characterizes the thickness of the current sheet can be interpreted in terms of thinning during the growth phase of a substorm and thickening following the expansion phase. Ground signatures that give insight into the local time of substorm onset can be used to interpret the response of the plasmasheet to substorm related changes of the global system. During a substorm, the field magnitude in the central plasmasheet fluctuates at the period of Pi2 pulsations.
- Published
- 2005
40. Cluster observations of quasi-periodic impulsive signatures in the dayside northern lobe: High-latitude flux transfer events?
- Author
-
Thompson, S. M, Kivelson, M. G, Khurana, K. K, Balogh, A, Reme, H, Fazakerley, A. N, and Kistler, L. M
- Subjects
Geophysics - Abstract
We report on a series of quasi-periodic reversals in GSM B(sub Z) observed by the four Cluster spacecraft in the northern dayside lobe poleward of the cusp on 23 February 2001. During an interval of about 35 min, multiple reversals (negative to positive) in B(sub Z) of approximately 1-min duration with an approximate 8-min recurrence time were observed. The individual structures do not resemble low-latitude flux transfer events (FTE) [Russell and Elphic, 1979] but the 8-min recurrence frequency suggests that intermittent reconnection may be occurring .Measurements (appropriately lagged) of the solar wind at ACE show that the IMF was southward-oriented with a strong B(sub X) and that a modest dynamic pressure increased as the events started. The multi-point observations afforded by the Cluster spacecraft were used to infer the motion (direction and speed) of the observed magnetic field reversals. The associated currents were also calculated and they are consistent with the spatial confinement of the observed magnetic field reversals. We propose that the observed reversals are due to flux tubes reconnecting with closed field lines on the dayside. Ancillary data from the Cluster Ion Spectrometry (CIS) and Plasma Electron And Current Experiment (PEACE) instruments were used to develop a physical picture of the reversals.
- Published
- 2004
41. Cluster electric current density measurements within a magnetic flux rope in the plasma sheet
- Author
-
Slavin, J. A, Lepping, R. P, Gjerloev, J, Goldstein, M. L, Fairfield, D. H, Acuna, M. H, Balogh, A, Dunlop, M, Kivelson, M. G, and Khurana, K
- Subjects
Geophysics - Abstract
On August 22, 2001 all 4 Cluster spacecraft nearly simultaneously penetrated a magnetic flux rope in the tail. The flux rope encounter took place in the central plasma sheet, Beta(sub i) approx. 1-2, near the leading edge of a bursty bulk flow. The "time-of-flight" of the flux rope across the 4 spacecraft yielded V(sub x) approx. 700 km/s and a diameter of approx.1 R(sub e). The speed at which the flux rope moved over the spacecraft is in close agreement with the Cluster plasma measurements. The magnetic field profiles measured at each spacecraft were first modeled separately using the Lepping-Burlaga force-free flux rope model. The results indicated that the center of the flux rope passed northward (above) s/c 3, but southward (below) of s/c 1, 2 and 4. The peak electric currents along the central axis of the flux rope predicted by these single-s/c models were approx.15-19 nA/sq m. The 4-spacecraft Cluster magnetic field measurements provide a second means to determine the electric current density without any assumption regarding flux rope structure. The current profile determined using the curlometer technique was qualitatively similar to those determined by modeling the individual spacecraft magnetic field observations and yielded a peak current density of 17 nA/m2 near the central axis of the rope. However, the curlometer results also showed that the flux rope was not force-free with the component of the current density perpendicular to the magnetic field exceeding the parallel component over the forward half of the rope, perhaps due to the pressure gradients generated by the collision of the BBF with the inner magnetosphere. Hence, while the single-spacecraft models are very successful in fitting flux rope magnetic field and current variations, they do not provide a stringent test of the force-free condition.
- Published
- 2003
42. The Permanent and Inductive Magnetic Moments of Ganymede
- Author
-
Kivelson, M. G, Khurana, K. K, and Volwerk, M
- Subjects
Lunar And Planetary Science And Exploration - Abstract
Data acquired by the Galileo magnetometer on five passes by Ganymede have been used to characterize Ganymede's internal magnetic moments. Three of the five passes were useful for determination of the internal moments through quadrupole order. Models representing the internal field as the sum of dipole and quadrupole terms or as the sum of a permanent dipole field upon which is superimposed an induced magnetic dipole driven by the time varying component of the externally imposed magnetic field of Jupiter's magnetosphere give equally satisfactory fits to the data. The permanent dipole moment has an equatorial field magnitude 719 nT and is tilted by 176 degrees from the spin axis with the pole in the southern hemisphere rotated by 24 degrees from the Jupiter-facing meridian plane towards the trailing hemisphere. The data are consistent with an inductive response of a good electrical conductor of radius approximately 1 Ganymede radius. Although the data do not enable us to establish the presence of an inductive response beyond doubt, we favor the inductive response model because it gives a good fit to the data using only 4 parameters to describe the internal sources of fields, whereas the equally good dipole plus quadrupole fit requires 8 parameters. An inductive response is consistent with a buried conducting shell, probably liquid water with dissolved electrolytes, somewhere in the first few hundred km below Ganymede's surface. The depth at which the ocean is buried beneath the surface is somewhat uncertain, but our favored model suggests a depth of order 150 kilometers. As both temperature and pressure increase with depth and the melting temperature of pure ice decreases to a minimum at approximately 170 kilometer depth, it seems possible that near this location, a layer of water would be sandwiched between layers of ice.
- Published
- 2002
43. Wave Activity in Europa's Wake: Implications for Ion Pickup
- Author
-
Volwerk, M, Kivelson, M. G, and Khurana, K. K
- Subjects
Lunar And Planetary Science And Exploration - Abstract
Intense wave power at frequencies near and below the cyclotron frequencies of heavy ions was detected in Europa's wake during the E11 and E15 flybys. The fluctuations are mainly transverse to the background magnetic field. Wave characteristics indicate that they are ion cyclotron waves driven by positively charged pickup ions. In both flybys there is evidence, derived from the wave polarization, for pickup of negatively charged chlorine ions. When the moon is near the center of the Jovian current sheet, the pickup rate inferred for the E15 flyby is larger than that for the E11 flyby, when the moon is outside the Jovian current sheet. The wave power does not provide exact pickup density values because the waves are observed in regions where their growth has not yet fully developed. At the edges of the wake region, low-frequency (< K+ gyrofrequency) magnetohydrodynamic waves are also present. We identify magnetic field signatures that are reminiscent of interchange/ballooning of mass-loaded flux tubes from the wake/pickup region expanding into ambient medium that is less dense.
- Published
- 2001
- Full Text
- View/download PDF
44. Structure of the Jovian Magnetodisk Current Sheet: Initial Galileo Observations
- Author
-
Russell, C. T, Huddleston, D. E, Khurana, K. K, and Kivelson, M. G
- Subjects
Lunar And Planetary Science And Exploration - Abstract
The ten-degree tilt of the Jovian magnetic dipole causes the magnetic equator to move back and forth across Jupiter's rotational equator and tile Galileo orbit that lies therein. Beyond about 24 Jovian radii, the equatorial current sheet thins and tile magnetic structure changes from quasi-dipolar into magnetodisk-like with two regions of nearly radial but antiparallel magnetic field separated by a strong current layer. The magnetic field at the center of the current sheet is very weak in this region. Herein we examine tile current sheet at radial distances from 24 55 Jovian radii. We find that the magnetic structure very much resembles tile structure seen at planetary magnetopause and tail current sheet crossings. Tile magnetic field variation is mainly linear with little rotation of the field direction, At times there is almost no small-scale structure present and the normal component of the magnetic field is almost constant through the current sheet. At other times there are strong small-scale structures present in both the southward and northward directions. This small-scale structure appears to grow with radial distance and may provide the seeds for tile explosive reconnection observed at even greater radial distances oil tile nightside. Beyond about 40 Jovian radii, the thin current sheet also appears to be almost constantly in oscillatory motion with periods of about 10 min. The amplitude of these oscillations also appears to grow with radial distance. The source of these fluctuations may be dynamical events in tile more distant magnetodisk.
- Published
- 2001
- Full Text
- View/download PDF
45. Sounding of Icy Galilean Satellites by Surface Observatories
- Author
-
Khurana, K. K, Banerdt, W. B, Johnson, T. V, Russell, C. T, Kivelson, M. G, Davis, P. M, and Vidale, J. E
- Subjects
Lunar And Planetary Science And Exploration - Abstract
Several independent geological and geophysical investigations suggest that Europa and Ganymede contain subsurface oceans. Using Jupiter's rotating magnetic field as a primary signal, the magnetometer experiment onboard Galileo has measured secondary induction signals emanating from Europa, Ganymede, and surprisingly Callisto. The strong electromagnetic induction from these moons suggests that large global electrical conductors are located just below their icy crusts. A detailed analysis reveals that global salty oceans with salinity similar to the Earth's ocean and thicknesses in the range of approx. 6-100 kms can explain the induction observed by the Galileo magnetometer. Additional information is contained in the original extended abstract.
- Published
- 2001
46. Substorms At Jupiter: Galileo Observations of Transient Reconnection in The Near Tail
- Author
-
Russell, C. T, Khurana, K. K, Kivelson, M. G, and Huddleston, D. E
- Subjects
Astronomy - Abstract
The magnetic flux content of the Jovian magnetosphere is set by the internal dynamo, but those magnetic field lines are constantly being loaded by heavy ions at the orbit of lo and dragged inexorably outward by the centrifugal force. Vasyliunas has proposed a steady state reconnecting magnetospheric model that sheds plasma islands of zero net magnetic flux and returns nearly empty flux tubes to the inner magnetosphere. The Galileo observations indicate that beyond 40 Rj the current sheet begins to tear and beyond 50 Rj on the nightside explosively reconnects as the tearing site reaches the low density lobe region above and below the current sheet. Small events occur irregularly but on average about every 4 hours and large events about once a day. The magnetic flux reconnected in such events amounts up to about 70,000 Webers/sec and is sufficient to return the outwardly convected magnetic flux to the inner magnetosphere. Since this process releases plasmoids into the jovian tail, as do terrestrial substorms; since this process involves explosive reconnection across the current sheet on the nightside of the planet, as do terrestrial substorms; and since the process is a key in closing the circulation pattern of the magnetic and plasma flux, as it is in terrestrial substorms; we refer to these events as jovian substorms.
- Published
- 2000
- Full Text
- View/download PDF
47. Probing Ganymede's Magnetosphere with Field Line Resonances
- Author
-
Volwerk, M, Kivelson, M. G, Khurana, K. K, and McPherron, R. L
- Subjects
Lunar And Planetary Science And Exploration - Abstract
We report on the spectrum of field line resonances identified in data acquired by the Galileo spacecraft within Ganymede's magnetosphere on a relatively low latitude pass. We infer properties of the plasma distribution and its transport from the observed spectrum. The harmonic structure in the spectrum of the magnetometer data agrees very well with the frequencies predicted for resonances of a dipole field. The spectrum implies a density of 2 amu per cubic centimeter near the equator on closed field lines of Ganymede's magnetic field inside of 2 RG (Ganymede radii). This density is significantly reduced relative to the local density of the Jovian plasma sheet near Ganymede (less than or equal to 8 electrons per cubic centimeter, or approximately equal to 100 amu per cubic centimeter for an average ion mass per charge of 20 amu and average charge of 1.5 electron charges). A shadowing effect of Ganymede for the flow of particles injected at a reconnection layer on the side of the moon downstream relative to the direction of torus plasma flow accounts for the marked density depletion. Implications for conducting paths near Ganymede's surface are considered.
- Published
- 1999
- Full Text
- View/download PDF
48. Induced magnetic fields as evidence for subsurface oceans in Europa and Callisto
- Author
-
Khurana, K. K., Kivelson, M. G., Stevenson, D. J., Schubert, G., Russell, C. T., Walker, R. J., and Polanskey, C.
- Published
- 1998
49. Absence of an internal magnetic field at Callisto
- Author
-
Khurana, K. K., Kivelson, M. G., Russell, C. T., Walker, R. J., and Southwood, D. J.
- Published
- 1997
50. Embedded Regions 1 and 2 Field-Aligned Currents: Newly Recognized From Low-Altitude Spacecraft Observations.
- Author
-
Jiang Liu, Lyons, L. R., Chih-Ping Wang, Yuzhang Ma, Strangeway, R. J., Yongliang Zhang, Kivelson, M., Ying Zou, and Khurana, K.
- Subjects
MAGNETOSPHERE ,IONOSPHERE ,CONVECTION (Meteorology) ,ELECTRON precipitation ,GEOMAGNETISM - Abstract
Regions 1 and 2 (R1 and R2) field-aligned currents (FACs), manifestations of large-scale convection in Earth's magnetosphere-ionosphere (M-I) system, often contain intense FAC layers of mesoscale latitudinal width near the R1/R2 interface. We refer to such layers as "embedded" R1 and R2 FACs. Likely resulting from enhanced magnetosphere-ionosphere (M-I) convection, these FACs may indicate M-I configuration change and contribute significantly to substorm current wedges. We present several events in which embedded FACs were observed by low-altitude spacecraft in the ionosphere. All the events occurred during active geomagnetic conditions or a substorm growth phase, and most map to an equatorial location on the nightside. When an embedded FAC is upward, it coincides with inverted-V electron precipitation and a discrete auroral arc. If an upward embedded FAC is in the postmidnight-to-dawn sector, a dawnside auroral polarization stream appears immediately poleward of it, so it may be important for ionospheric heating, M-I convection, and instabilities. Our results establish embedded FACs as a frequently appearing, fundamental phenomenon for understanding and modeling the magnetosphere-ionosphere system. [ABSTRACT FROM AUTHOR]
- Published
- 2021
- Full Text
- View/download PDF
Catalog
Discovery Service for Jio Institute Digital Library
For full access to our library's resources, please sign in.