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1,497 results on '"Moser, L."'

3. ALMA-IRDC: Dense gas mass distribution from cloud to core scales

Author

Barnes, A. T., Henshaw, J. D., Fontani, F., Pineda, J. E., Cosentino, G., Tan, J. C., Caselli, P., Jiménez-Serra, I., Law, C. Y., Avison, A., Bigiel, F., Feng, S., Kong, S., Longmore, S. N., Moser, L., Parker, R. J., Sánchez-Monge, Á., and Wang, K.

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
Abstract

Infrared dark clouds (IRDCs) are potential hosts of the elusive early phases of high-mass star formation (HMSF). Here we conduct an in-depth analysis of the fragmentation properties of a sample of 10 IRDCs, which have been highlighted as some of the best candidates to study HMSF within the Milky Way. To do so, we have obtained a set of large mosaics covering these IRDCs with ALMA at band 3 (or 3mm). These observations have a high angular resolution (~3arcsec or ~0.05pc), and high continuum and spectral line sensitivity (~0.15mJy/beam and ~0.2K per 0.1km/s channel at the N2H+(1-0) transition). From the dust continuum emission, we identify 96 cores ranging from low- to high-mass (M = 3.4 to 50.9Msun) that are gravitationally bound (alpha_vir = 0.3 to 1.3) and which would require magnetic field strengths of B = 0.3 to 1.0mG to be in virial equilibrium. We combine these results with a homogenised catalogue of literature cores to recover the hierarchical structure within these clouds over four orders of magnitude in spatial scale (0.01pc to 10pc). Using supplementary observations at an even higher angular resolution, we find that the smallest fragments (<0.02pc) within this hierarchy do not currently have the mass and/or the density required to form high-mass stars. Nonetheless, the new ALMA observations presented in this paper have facilitated the identification of 19 (6 quiescent and 13 star-forming) cores that retain >16Msun without further fragmentation. These high-mass cores contain trans-sonic non-thermal motions, are kinematically sub-virial, and require moderate magnetic field strengths for support against collapse. The identification of these potential sites of high-mass star formation represents a key step in allowing us to test the predictions from high-mass star and cluster formation theories., Comment: 21(+6 in appendix) pages, 12(+3) figures, 3(+3) tables. Machine-readable versions of Table A1, A2 and A3 are available online. Accepted for publication in MNRAS

Published
2021
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4. Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS): I. Robust ALMA Continuum Photometry Catalogs and Stellar Mass and Star Formation Properties for ~700 Galaxies at z=0.5-6

Author

Liu, Daizhong, Lang, P., Magnelli, B., Schinnerer, E., Leslie, S., Fudamoto, Y., Bondi, M., Groves, B., Jimenez-Andrade, E., Harrington, K., Karim, A., Oesch, P., Sargent, M., Vardoulaki, E., Badescu, T., Moser, L., Bertoldi, F., Battisti, A., da Cunha, E., Zavala, J., Vaccari, M., Davidzon, I., Riechers, D., and Aravena, M.

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

The rich information on (sub)millimeter dust continuum emission from distant galaxies in the public Atacama Large Millimeter/submillimeter Array (ALMA) archive is contained in thousands of inhomogeneous observations from individual PI-led programs. To increase the usability of these data for studies deepening our understanding of galaxy evolution, we have developed automated mining pipelines for the ALMA archive in the COSMOS field (A3COSMOS) that efficiently exploit the available information for large numbers of galaxies across cosmic time and keep the data products in sync with the increasing public ALMA archive: (a) a dedicated ALMA continuum imaging pipeline, (b) two complementary photometry pipelines for both blind source extraction and prior source fitting, (c) a counterpart association pipeline utilizing the multiwavelength data available (including quality assessment based on machine-learning techniques), (d) an assessment of potential (sub)millimeter line contribution to the measured ALMA continuum, and (e) extensive simulations to provide statistical corrections to biases and uncertainties in the ALMA continuum measurements. Application of these tools yields photometry catalogs with ~1000 (sub)millimeter detections (spurious fraction ~8%-12%) from over 1500 individual ALMA continuum images. Combined with ancillary photometric and redshift catalogs and the above quality assessments, we provide robust information on redshift, stellar mass, and star formation rate for ~700 galaxies at redshifts 0.5-6 in the COSMOS field (with undetermined selection function). The ALMA photometric measurements and galaxy properties are released publicly within our blind extraction, prior fitting, and galaxy property catalogs, plus the images. These products will be updated on a regular basis in the future., Comment: 56 pages, 36 figures, 5 tables, published on ApJS. Catalogs are available at journal website in FITS format. Current and future catalogs and continuum images will be released at COSMOS IRSA server https://irsa.ipac.caltech.edu/data/COSMOS/overview.html and A3COSMOS website https://sites.google.com/view/a3cosmos/data

Published
2019
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5. Observations of the 86 GHz SiO maser sources in the Central Parsec of the Galactic Centre

Author

Borkar, A., Eckart, A., Straubmeier, C., Sjouwerman, L. O., Karas, V., Kunneriath, D., Moser, L., Britzen, S., Valencia-S, M., Donea, A., and Zensus, A.

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
Abstract

We present results of 3 mm observations of SiO maser sources in the Galactic Centre (GC) from observations with the Australia Telescope Compact Array between $2010-2014$, along the transitions of the SiO molecule at $v = 1, J = 2-1$ at 86.243 GHz and $v = 2, J = 2-1$ at 85.640 GHz. We also present the results of the 3 mm observations with Atacama Large Millimeter/Submillimeter Array (ALMA). We detected 5 maser sources from the ATCA data, IRS 7, IRS 9, IRS 10EE, IRS 12N, and IRS 28; and 20 sources from the ALMA data including 4 new sources. These sources are predominantly late-type giants or emission line stars with strong circumstellar maser emission. We analyse these sources and calculate their proper motions. We also study the variability of the maser emission. IRS 7, IRS 12N and IRS 28 exhibit long period variability of the order of $1 - 2$ years, while other sources show steady increase or decrease in flux density and irregular variability over observation timescales. This behaviour is consistent with the previous observations., Comment: 22 pages, 5 figures, to be published in the proceedings of the XIII workshop on "Multifrequency Behaviour of High Energy Cosmic Sources - XIII - MULTIF2019", held on 3-8 June, 2019, in Palermo, Italy

Published
2019

7. Imaging pinning and expulsion of individual superconducting vortices in amorphous MoSi thin films

Author

Ceccarelli, L., Vasyukov, D., Wyss, M., Romagnoli, G., Rossi, N., Moser, L., and Poggio, M.

Subjects
Condensed Matter - Superconductivity, Condensed Matter - Mesoscale and Nanoscale Physics
Abstract

We use a scanning nanometer-scale superconducting quantum interference device (SQUID) to image individual vortices in amorphous superconducting MoSi thin films. Spatially resolved measurements of the magnetic field generated by both vortices and Meissner screening satisfy the Pearl model for vortices in thin films and yield values for the Pearl length and bulk penetration depth at 4.2 K. Flux pinning is observed and quantified through measurements of vortex motion driven by both applied currents and thermal activation. The effects of pinning are also observed in metastable vortex configurations, which form as the applied magnetic field is reduced and magnetic flux is expelled from the film. Understanding and controlling vortex dynamics in amorphous thin films is crucial for optimizing devices such as superconducting nanowire single photon detectors (SNSPDs), the most efficient of which are made from MoSi, WSi, and MoGe., Comment: Main text (11 pages, 5 figures) and Supplementary material (10 pages, 9 figures)

Published
2019
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8. Competence of radiologists in cardiac CT and MR imaging in Europe: insights from the ESCR Registry

Author

Catapano, F, Moser, L, Francone, M, Catalano, C, Vliegenthart, R, Budde, R, Salgado, R, Hrabak Paar, M, Pirnat, M, Loewe, C, Nikolaou, K, Williams, M, Muscogiuri, G, Natale, L, Lehmkuhl, L, Sieren, M, Gutberlet, M, Alkadhi, H, Catapano F., Moser L. J., Francone M., Catalano C., Vliegenthart R., Budde R. P. J., Salgado R., Hrabak Paar M., Pirnat M., Loewe C., Nikolaou K., Williams M. C., Muscogiuri G., Natale L., Lehmkuhl L., Sieren M. M., Gutberlet M., Alkadhi H., Catapano, F, Moser, L, Francone, M, Catalano, C, Vliegenthart, R, Budde, R, Salgado, R, Hrabak Paar, M, Pirnat, M, Loewe, C, Nikolaou, K, Williams, M, Muscogiuri, G, Natale, L, Lehmkuhl, L, Sieren, M, Gutberlet, M, Alkadhi, H, Catapano F., Moser L. J., Francone M., Catalano C., Vliegenthart R., Budde R. P. J., Salgado R., Hrabak Paar M., Pirnat M., Loewe C., Nikolaou K., Williams M. C., Muscogiuri G., Natale L., Lehmkuhl L., Sieren M. M., Gutberlet M., and Alkadhi H.

Abstract

Rationale: To provide an overview of the current status of cardiac multimodality imaging practices in Europe and radiologist involvement using data from the European Society of Cardiovascular Radiology (ESCR) MRCT-registry. Materials and methods: Numbers on cardiac CT and MRI examinations were extracted from the MRCT-registry of the ESCR, entered between January 2011 and October 2023 (n = 432,265). Data collection included the total/annual numbers of examinations, indications, complications, and reporting habits. Results: Thirty-two countries contributed to the MRCT-registry, including 29 European countries. Between 2011 and 2022, there was a 4.5-fold increase in annually submitted CT examinations, from 3368 to 15,267, and a 3.8-fold increase in MRI examinations, from 3445 to 13,183. The main indications for cardiac CT were suspected coronary artery disease (CAD) (59%) and transcatheter aortic valve replacement planning (21%). The number of patients with intermediate pretest probability who underwent CT for suspected CAD showed an increase from 61% in 2012 to 82% in 2022. The main MRI indications were suspected myocarditis (26%), CAD (21%), and suspected cardiomyopathy (19%). Adverse event rates were very low for CT (0.3%) and MRI (0.7%) examinations. Reporting of CT and MRI examinations was performed mainly by radiologists (respectively 76% and 71%) and, to a lesser degree, in consensus with non-radiologists (19% and 27%, respectively). The remaining examinations (4.9% CT and 1.7% MRI) were reported by non-radiological specialties or in separate readings of radiologists and non-radiologists. Conclusions: Real-life data on cardiac imaging in Europe using the largest available MRCT-registry demonstrate a considerable increase in examinations over the past years, the vast majority of which are read by radiologists. These findings indicate that radiologists contribute to meeting the increasing demands of competent and effective care in cardiac imaging to a relevant ext

Published
2024

10. Experimental Indicators of Accretion Processes in Active Galactic Nuclei

Author

Eckart, A., Valencia-S., M., Shahzamanian, B., Zajacek, M., Moser, L., Busch, G., Parsa, M., Subroweit, M., Peissker, F., Sabha, N., Hosseini, S. E., Horrobin, M., Straubmeier, C., Fazeli, N., Borkar, A., Kunneriath, D., Karas, V., Rauch, C., Britzen, S., Zensus, A., Garcia-Marin, M., and Rashed, Y. E.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

Bright Active Galactic Nuclei are powered by accretion of mass onto the super massive black holes at the centers of the host galaxies. For fainter objects star formation may significantly contribute to the luminosity. We summarize experimental indicators of the accretion processes in Active Galactic Nuclei (AGN), i.e., observable activity indicators that allow us to conclude on the nature of accretion. The Galactic Center is the closest galactic nucleus that can be studied with unprecedented angular resolution and sensitivity. Therefore, here we also include the presentation of recent observational results on Sagittarius A* and the conditions for star formation in the central stellar cluster. We cover results across the electromagnetic spectrum and find that the Sagittarius A* (SgrA*) system is well ordered with respect to its geometrical orientation and its emission processes of which we assume to reflect the accretion process onto the super massive black hole., Comment: 16 pages, 4 figures, conference proceeding: Accretion Processes in Cosmic Sources - APCS2016 - 5-10 September 2016, Saint Petersburg, Russia

Published
2017
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11. Nuclear Activity and the Conditions of Star-formation at the Galactic Center

Author

Eckart, A., Valencia-S., M., Shahzamanian, B., Zajacek, M., Moser, L., Parsa, M., Subroweit, M., Peissker, F., Sabha, N., Horrobin, M., Straubmeier, C., Borkar, A., Kunneriath, D., Karas, V., Rauch, C., Britzen, S., Zensus, A., and García-Marín, M.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

The Galactic Center is the closest galactic nucleus that can be studied with unprecedented angular resolution and sensitivity. We summarize recent basic observational results on Sagittarius A* and the conditions for star formation in the central stellar cluster. We cover results from the radio, infrared, and X-ray domain and include results from simulation as well. From (sub-)mm and near-infrared variability and near-infrared polarization data we find that the SgrA* system (supermassive black hole spin, a potential temporary accretion disk and/or outflow) is well ordered in its geometrical orientation and in its emission process that we assume to reflect the accretion process onto the supermassive black hole (SMBH)., Comment: 11 pages, 4 figures, 1 table; published in PoS-SISSA Proceedings of the: Frontier Research in Astrophysics - II, 23-28 May 2016, Mondello (Palermo), Italy

Published
2017

12. Polarized near-infrared light of the Dusty S-cluster Object (DSO/G2) at the Galactic Center

Author

Shahzamanian, B., Eckart, A., Zajacek, M., Valencia-S., M., Sabha, N., Moser, L., Parsa, M., Peissker, F., and Straubmeier, C.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

We investigate an infrared-excess source called G2 or Dusty S-cluster Object (DSO) moving on a highly eccentric orbit around the Galaxy's central black hole, Sgr A*. We use, for the first time, near-infrared polarimetric imaging data to determine the nature and the properties of the DSO, and obtain an improved K_s-band identification of this source in median polarimetry images of different observing years. The source starts to deviate from the stellar confusion in 2008, and it does not show any flux density variability over the years we analyzed it. We measure the polarization degree and angle of the DSO between 2008 and 2012 and conclude, based on the significance analysis on polarization parameters, that it is an intrinsically polarized source (>20%) with a varying polarization angle as it approaches Sgr A* position. DSO shows a near-infrared excess of K_s-L' > 3 that remains compact close to the pericenter of its orbit. Its observed parameters and the significant polarization obtained in this work show that the DSO might be a dust-enshrouded young star, forming a bow shock as it approaches the super massive black hole. The significantly high measured polarization degree indicates that it has a non-spherical geometry and it can be modelled as a combination of a bow shock with a bipolar wind of the star. We use a 3D radiative transfer model that can reproduce the observed properties of the source such as the total flux density and the polarization degree. We obtain that the change of the polarization angle can be due to an intrinsic change in the source structure. Accretion disc precession of the young star in the gravitational field of the black hole can lead to the change of the bipolar outflow and therefore the polarization angle variation. It might also be the result of the source interaction with the ambient medium., Comment: 15 pages, 12 figures, Accepted to be published in Astronomy & Astrophysics

Published
2016
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14. Low rate of nonrelapse mortality in under 4-year-olds with ALL given chemo-conditioning for HSCT: Phase III FORUM study

Author

Bader, P, Poetschger, U, Dalle, J, Moser, L, Balduzzi, A, Ansari, M, Buechner, J, Güngör, T, Ifversen, M, Kriván, G, Pichler, H, Renard, M, Staciuk, R, Sedlacek, P, Stein, J, Heusel, J, Truong, T, Wachowiak, J, Yeşilipek, M, Locatelli, F, Peters, C, Bader, Peter, Poetschger, Ulrike, Dalle, Jean-Hugues, Moser, Laura M, Balduzzi, Adriana Cristina, Ansari, Marc, Buechner, Jochen, Güngör, Tayfun, Ifversen, Marianne, Kriván, Gergely, Pichler, Herbert, Renard, Marleen, Staciuk, Raquel, Sedlacek, Petr, Stein, Jerry, Heusel, Jan Robert, Truong, Tony, Wachowiak, Jacek, Yeşilipek, M Akif, Locatelli, Franco, Peters, Christina, Bader, P, Poetschger, U, Dalle, J, Moser, L, Balduzzi, A, Ansari, M, Buechner, J, Güngör, T, Ifversen, M, Kriván, G, Pichler, H, Renard, M, Staciuk, R, Sedlacek, P, Stein, J, Heusel, J, Truong, T, Wachowiak, J, Yeşilipek, M, Locatelli, F, Peters, C, Bader, Peter, Poetschger, Ulrike, Dalle, Jean-Hugues, Moser, Laura M, Balduzzi, Adriana Cristina, Ansari, Marc, Buechner, Jochen, Güngör, Tayfun, Ifversen, Marianne, Kriván, Gergely, Pichler, Herbert, Renard, Marleen, Staciuk, Raquel, Sedlacek, Petr, Stein, Jerry, Heusel, Jan Robert, Truong, Tony, Wachowiak, Jacek, Yeşilipek, M Akif, Locatelli, Franco, and Peters, Christina

Abstract

Allogeneic hematopoietic stem cell transplantation (HSCT) is highly effective for treating pediatric high-risk or relapsed acute lymphoblastic leukemia (ALL). For young children, total body irradiation (TBI) is associated with severe late sequelae. In the FORUMstudy (NCT01949129), we assessed safety, event-free survival (EFS), and overall survival (OS) of 2 TBIfree conditioning regimens in children aged <4 years with ALL. Patients received fludarabine (Flu), thiotepa (Thio), and either busulfan (Bu) or treosulfan (Treo) before HSCT. From 2013 to 2021, 191 children received transplantation and were observed for ≥6 months (median followup: 3 years). The 3-year OS was 0.63 (95% confidence interval [95% CI], 0.52-0.72) and 0.76 (95% CI, 0.64-0.84) for Flu/Thio/Bu and Flu/Thio/Treo (P = .075), respectively. Three-year EFSwas 0.52 (95% CI, 0.41-0.61) and 0.51 (95% CI, 0.39-0.62), respectively (P = .794). Cumulative incidence of nonrelapse mortality (NRM)and relapse at 3 years were 0.06 (95% CI, 0.02-0.12) vs 0.03 (95%CI: [removed]1 acute graft-versus-host disease (GVHD) occurred in 29% of patients receiving Flu/Thio/ Bu and 17% of those receiving Flu/Thio/Treo (P = .049), whereas grade 3/4 occurred in 10% and 9%, respectively (P = .813). The 3-year incidence of chronic GVHD was 0.07 (95% CI, 0.03-0.13) vs 0.05 (95% CI, 0.02-0.11), respectively (P = .518). In conclusion, both chemotherapeutic conditioning regimens were well tolerated and NRM was low. However, relapse was the major cause of treatment failure.

Published
2024

15. The nuclear gas disk of NGC 1566 dissected by SINFONI and ALMA

Author

Smajić, S., Moser, L., Eckart, A., Busch, G., Combes, F., García-Burillo, S., Valencia-S., M., and Horrobin, M.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

We present the results of near-infrared H- and K-band European Southern Observatory SINFONI integral field spectroscopy of the Seyfert galaxy NGC 1566. We investigate the central kpc of this nearby galaxy, concentrating on excitation conditions, morphology, and stellar content. NGC 1566 was selected from our NUGA (-south) sample and is a ringed, spiral galaxy with a stellar bar. We present emission and absorption line measurements in the central kpc of NGC 1566. Broad and narrow Br{\gamma} lines were detected. The detection of a broad Br{\gamma} component is a clear sign of a super-massive black hole in the center. Blackbody emission temperatures of ~1000 K are indicative of a hot dust component, the torus, in the nuclear region. The molecular hydrogen lines, hydrogen recombination lines, and [FeII] indicate that the excitation at the center is coming from an AGN. The central region is predominantly inhabited by molecular gas, dust, and an old K-M type giant stellar population. The molecular gas and stellar velocity maps both show a rotation pattern. The molecular gas velocity field shows a perturbation toward the center that is typical for bars or spiral density waves. The molecular gas species of warm H_2(1-0)S(1) and cold ^{12}CO(3-2) gas trace a nuclear gas disk of about 3" in radius with a nuclear spiral reaching toward the nucleus. From the equivalent width of H_2(1-0)S(1) a molecular ring with r<~3" can be inferred. This spiral seems to be an instrument that allows gas to fall toward the nucleus down to <50 pc scales. The excitation of molecular hydrogen in the nuclear gas disk is not clear but diagnostic diagrams show a distinction between the nuclear region and a <9 Myr old star forming region at the southwestern spiral arm. Possibly shocked gas is detected ~2" from the center, which is visible in dispersion maps of H$_2$(1-0)S(1) and ^{12}CO(3-2) and in the 0.87 mm continuum., Comment: 20 pages, 16 figures, NUGA, Active Galaxies, AGN

Published
2015
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17. Monitoring the Dusty S-Cluster Object (DSO/G2) on its Orbit towards the Galactic Center Black Hole

Author

Valencia-S., M., Eckart, A., Zajacek, M., Peissker, F., Parsa, M., Grosso, N., Mossoux, E., Porquet, D., Jalali, B., Karas, V., Yazici, S., Shahzamanian, B., Sabha, N., Saalfeld, R., Smajic, S., Grellmann, R., Moser, L., Horrobin, M., Borkar, A., Marin, M. Garcia, Dovciak, M., Kunneriath, D., Karssen, G. D., Bursa, M., Straubmeier, C., and Bushouse, H.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

We analyse and report in detail new near-infrared (1.45 - 2.45 microns) observations of the Dusty S-cluster Object (DSO/G2) during its approach to the black hole at the center of the Galaxy that were carried out with ESO VLT/SINFONI between February and September 2014. Before May 2014 we detect spatially compact Br-gamma and Pa-alpha line emission from the DSO at about 40mas east of SgrA*. The velocity of the source, measured from the red-shifted emission, is 2700+-60 km/s. No blue-shifted emission above the noise level is detected at the position of SgrA* or upstream the presumed orbit. After May we find spatially compact Br-gamma blue-shifted line emission from the DSO at about 30mas west of SgrA* at a velocity of -3320+-60 km/s and no indication for significant red-shifted emission. We do not detect any significant extension of velocity gradient across the source. We find a Br-gamma-line full width at half maximum of 50+-10 Angstroem before and 15+-10 Angstroem after the peribothron transit, i.e. no significant line broadening with respect to last year is observed. Br-gamma line maps show that the bulk of the line emission originates from a region of less than 20mas diameter. This is consistent with a very compact source on an elliptical orbit with a peribothron time passage in 2014.39+-0.14. For the moment, the flaring activity of the black hole in the near-infrared regime has not shown any statistically significant increment. Increased accretion activity of SgrA* may still be upcoming. We discuss details of a source model according to which the DSO is rather a young accreting star than a coreless gas and dust cloud., Comment: 32 pages - 3 tables - 17 figure - accepted by ApJ

Published
2014
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18. Star Formation in the vicinity of Nuclear Black Holes: Young Stellar Objects close to Sgr A*

Author

Jalali, B., Pelupessy, F. I., Eckart, A., Zwart, S. Portegies, Sabha, N., Borkar, A., Moultaka, J., Mužić, K., and Moser, L.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

It is often assumed that the strong gravitational field of a super-massive black hole disrupts an adjacent molecular cloud preventing classical star formation in the deep potential well of the black hole. Yet, young stars have been observed across the entire nuclear star cluster of the Milky Way including the region close ($<$0.5~pc) to the central black hole, Sgr A*. Here, we focus particularly on small groups of young stars, such as IRS 13N located 0.1 pc away from Sgr A*, which is suggested to contain about five embedded massive young stellar objects ($<$1 Myr). We perform three dimensional hydrodynamical simulations to follow the evolution of molecular clumps orbiting about a $4\times10^6~M_{\odot}$ black hole, to constrain the formation and the physical conditions of such groups. The molecular clumps in our models assumed to be isothermal containing 100 $M_{\odot}$ in $<$0.2 pc radius. Such molecular clumps exist in the circumnuclear disk of the Galaxy. In our highly eccentrically orbiting clump, the strong orbital compression of the clump along the orbital radius vector and perpendicular to the orbital plane causes the gas densities to increase to values higher than the tidal density of Sgr A*, which are required for star formation. Additionally, we speculate that the infrared excess source G2/DSO approaching Sgr A* on a highly eccentric orbit could be associated with a dust enshrouded star that may have been formed recently through the mechanism supported by our models., Comment: 18 pages, 11 figures, accepted for publication in MNRAS

Published
2014
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19. Young Stellar Objects close to Sgr A*

Author

Jalali, B., Pelupessy, I., Eckart, A., Zwart, S. Portegies, Sabha, N., Borkar, A., Moultaka, J., Muzic, K., and Moser, L.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

We aim at modelling small groups of young stars such as IRS 13N, 0.1 pc away from Sgr A*, which is suggested to contain a few embedded massive young stellar objects. We perform hydrodynamical simulations to follow the evolution of molecular clumps orbiting about a $4\times10^6 ~ M_{\odot}$ black hole, to constrain the formation and the physical conditions of such groups. We find that, the strong compression due to the black hole along the orbital radius vector of clumps evolving on highly eccentric orbits causes the clumps densities to increase to higher than the tidal density of Sgr A*, and required for star formation. This suggests that the tidal compression from the black hole could support star formation. Additionally, we speculate that the infrared excess source G2/DSO approaching Sgr A* on a highly eccentric orbit could be associated with a dust enshrouded star that may have been formed recently through the mechanism supported by our models., Comment: 2 pages, 2 figures, Proc. of a Conf. on IAU Symposium No.303: The GC: Feeding and Feedback in a Normal Galactic Nucleus 2013, Santa Fe New Mexico (USA)

Published
2013
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20. The infrared K-band identification of the DSO/G2 source from VLT and Keck data

Author

Eckart, Andreas, Horrobin, M., Britzen, S., Zamaninasab, M., Muzic, K., Sabha, N., Shahzamanian, B., Yazici, S., Moser, L., Garcia-Mari, M., Valencia-S., M., Borkar, A., Bursa, M., Karssen, G., Karas, V., Zajacek, M., Bronfman, L., Finger, R., Jalali, B., Vitale, M., Rauch, C., Kunneriath, D., Moultaka, J., Straubmeier, C., Rashed, Y. E., Markakis, K., and Zensus, A.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

A fast moving infrared excess source (G2) which is widely interpreted as a core-less gas and dust cloud approaches Sagittarius A* (SgrA*) on a presumably elliptical orbit. VLT K_s-band and Keck K'-band data result in clear continuum identifications and proper motions of this about 19m Dusty S-cluster Object (DSO). In 2002-2007 it is confused with the star S63, but free of confusion again since 2007. Its near-infrared (NIR) colors and a comparison to other sources in the field speak in favor of the DSO being an IR excess star with photospheric continuum emission at 2 microns than a core-less gas and dust cloud. We also find very compact L'-band emission ($<$0.1'') contrasted by the reported extended (0.03'' up to about 0.2'' for the tail) Brgamma emission. The presence of a star will change the expected accretion phenomena, since a stellar Roche lobe may retain a fraction of the material during and after the peri-bothron passage., Comment: 4 pages, 2 figures, Proc. of a Conf. on IAU Symposium No.303: The GC: Feeding and Feedback in a Normal Galactic Nucleus 2013 September 30 - October 4, Santa Fe New Mexico (USA)

Published
2013
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21. The Galactic Center as a Paradigm for Low Luminosity Nuclei? The K-band identification of the DSO/G2 source from VLT and Keck data

Author

Eckart, Andreas, Britzen, S., Horrobin, M., Zamaninasab, M., Muzic, K., Sabha, N., Shahzamanian, B., Yazici, S., Moser, L., Zuther, J., Garcia-Marin, M., Valencia-S., M., Bursa, M., Karssen, G., Karas, V., Jalali, B., Vitale, M., Bremer, M., Fischer, S., Smajic, S., Rauch, C., Kunneriath, D., Moultaka, J., Straubmeier, C., Rashed, Y. E., Iserlohe, C., Busch, G., Markakis, K., Borkar, A., and Zensus, A.

Subjects
Astrophysics - Galaxy Astrophysics
Abstract

The super-massive 4 million solar mass black hole (SMBH) SgrA* shows flare emission from the millimeter to the X-ray domain. The nucleus of the Milky Way has properties (stellar cluster, young stars, molecular gas and an accreting SMBH) that resemble those of currently higher luminous Low Luminosity Active Galactic Nuclei. A detailed analysis of the infrared light curves shows that the flares are probably generated in a single-state process forming a power-law distribution of the flux density. Near-infrared polarimetry shows signatures of strong gravity that are statistically significant against randomly polarized red noise. Details of the emission mechanism are discussed in a synchrotron/self-Compton model. SgrA* also allows to study the interaction of the SMBH with the immediate interstellar and gaseous environment of the central stellar cluster. Through infrared imaging of the central few arcseconds it is possible to study both inflow and outflow phenomena linked to the SgrA* black hole. In this context we also discuss the newly found dusty object that approaches SgrA* and present a comparison between recent Keck and VLT K-band data that clearly supports its detection as a about 19m K'-band continuum source., Comment: 15 pages, 7 figures, 2 tables, Proc. of a conf. on Nuclei of Seyfert galaxies and QSOs - Central engine \& conditions of star formation, November 6-8, 2012 Max-Planck-Insitut f\"ur Radioastronomie (MPIfR), Bonn, Germany

Published
2013

22. Discovery of an Intermediate Mass Black Hole at the center of the starburst/Seyfert composite galaxy IRAS 01072+4954

Author

Valencia-S., M., Eckart, A., Zuther, J., Fischer, S., Smajic, S., Iserlohe, C., Garcia-Marin, M., Moser, L., Bremer, M., and Vitale, M.

Subjects
Astrophysics - Cosmology and Extragalactic Astrophysics
Abstract

The starburst/Seyfert composite galaxy IRAS 01072+4954 (z=0.0236) is an enigmatic source that combines a Seyfert~1-like X-ray emission with a starburst optical spectrum that lacks broad line emission. We performed high angular resolution observations of the central kiloparsec of this galaxy in the near-infrared. Combining our data with 2MASS images of the whole galaxy, we obtain and model the surface brightness profile. We find indications for the presence of an elongated bar-like structure in both data sets. We also model the line of sight velocity distribution of the stars in the bulge. The derived photometrical and kinematical parameters of the bulge are used to evaluate the black hole mass through scaling relations. We find that all reliable estimations of the black hole mass are consistent with the presence of an intermediate mass black hole with a mass of ~10^5 solar masses (or less)., Comment: 9 pages, 5 figures. Proceedings of the Conference "The Central Kiloparsec in Galactic Nuclei. Astronomy at High Angular Resolution" (Bad Honnef, Germany, 29.8-2.9.2011)

Published
2013
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23. Are Narrow Line Seyfert 1s a special class of Active Galactic Nuclei?

Author

Valencia-S., M., Zuther, J., Eckart, A., Smajic, S., Iserlohe, C., Garcia-Marin, M., Busch, G., Vitale, M., Bremer, M., Fischer, S., Horrobin, M., Moser, L., Rashed, Y. E., and Straubmeier, C.

Subjects
Astrophysics - Cosmology and Extragalactic Astrophysics
Abstract

No. Due to their apparently extreme optical to X-ray properties, Narrow Line Seyfert 1s (NLSy1s) have been considered a special class of active galactic nuclei (AGN). Here, we summarize observational results from different groups to conclude that none of the characteristics that are typically used to define the NLSy1s as a distinct group - from the, nowadays called, Broad Line Seyfert 1s (BLSy1s) - is unique, nor ubiquitous of these particular sources, but shared by the whole Type 1 AGN. Historically, the NLSy1s have been distinguished from the BLSy1s by the narrow width of the broad Hbeta emission line. The upper limit on the full width at half maximum of this line is 2000 km/s for NLSy1s, while in BLSy1s it can be of several thousands of km/s. However, this border has been arbitrarily set and does not correspond to the change of any physical property. All observed parameters in Type 1 AGN cover continues ranges of values, which does not allow to infer the existence of two different kind of populations with FWHM(Hbeta,broad) = 2000 km/s as dividing point. We argue that the usage of this velocity limit to define samples of NLSy1s galaxies - as it is usually done in comparative studies -, together with the well known observational biases, naturally favors the selection of sources with low black hole masses and high Eddington ratios that are hosted by blue spiral galaxies. Therefore selection biases might be responsible for the reported differences between NLSy1 and BLSy1 sources., Comment: New version includes a Figure and extra references. Proceedings of the Conference "Nuclei of Seyfert galaxies and QSOs - Central engine & conditions of star formation" (Bonn, Germany, 6-8 November 2012)

Published
2013

24. Near-infrared proper motions and spectroscopy of infrared excess sources at the Galactic Center

Author

Eckart, A., Muzic, K., Yazici, S., Shahzamanian, B., Witzel, G., Sabha, N., Moser, L., Garcia-Marin, M., Valencia-S., M., Jalali, B., Bremer, M., Straubmeier, C., Kunneriath, D., and Moultaka, J.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

There are a number of faint compact infrared excess sources in the central stellar cluster of the Milky Way. Their nature and origin is unclear. In addition to several isolated objects of this kind we find a small but dense cluster of co-moving sources (IRS13N) about 3" west of SgrA* just 0.5" north of the bright IRS13E cluster of WR and O-type stars. Based on their color and brightness, there are two main possibilities: (1) they may be dust embedded stars older than few Myr, or (2) extremely young, dusty stars with ages less than 1Myr. We present fist H- and Ks-band identifications or proper motions of the IRS13N members, the high velocity dusty S-cluster object (DSO), and other infrared excess sources in the central field. We also present results of NIR H- and Ks-band ESO-SINFONI integral field spectroscopy of ISR13N. We show that within the uncertainties, the proper motions of the IRS13N sources in Ks- and L'-band are identical. This indicates that the bright L'-band IRS13N sources are indeed dust enshrouded stars rather than core-less dust clouds. The proper motions show that the IRS13N sources are not strongly gravitationally bound to each other implying that they have been formed recently. We also present a first H- and Ks-band identification as well as proper motions and HKsL'-colors of a fast moving DSO which was recently found in the cluster of high speed S-stars that surround the super-massive black hole Sagittarius A* (SgrA*). Most of the compact L'-band excess emission sources have a compact H- or Ks-band counterpart and therefore are likely stars with dust shells or disks. Our new results and orbital analysis from our previous work favor the hypothesis that the infrared excess IRS13N members and other dusty sources close to SgrA* are very young dusty stars and that star formation at the GC is a continuously ongoing process., Comment: 20 pages, 18 figures, 4 tables plus appendix with 16 figures and 3 tables accepted by A&A

Published
2012
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25. Flare emission from Sagittarius A*

Author

Eckart, A., Garcia-Marin, M., Vogel, S. N., Teuben, P., Morris, M. R., Baganoff, F., Dexter, J., Schoedel, R., Witzel, G., Valencia-S., M., Karas, V., Kunneriath, D., Bremer, M., Straubmeier, C., Moser, L., Sabha, N., Buchholz, R., Zamaninasab, M., Muzic, K., Moultaka, J., and Zensus, J. A.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

Based on Bremer et al. (2011) and Eckart et al. (2012) we report on simultaneous observations and modeling of the millimeter, near-infrared, and X-ray flare emission of the source Sagittarius A* (SgrA*) associated with the super-massive black hole at the Galactic Center. We study physical processes giving rise to the variable emission of SgrA* from the radio to the X-ray domain. To explain the statistics of the observed variability of the (sub-)mm spectrum of SgrA*, we use a sample of simultaneous NIR/X-ray flare peaks and model the flares using a synchrotron and SSC mechanism. The observations reveal flaring activity in all wavelength bands that can be modeled as the signal from adiabatically expanding synchrotron self-Compton (SSC) components. The model parameters suggest that either the adiabatically expanding source components have a bulk motion larger than v_exp or the expanding material contributes to a corona or disk, confined to the immediate surroundings of SgrA*. For the bulk of the synchrotron and SSC models, we find synchrotron turnover frequencies in the range 300-400 GHz. For the pure synchrotron models this results in densities of relativistic particles of the order of 10^6.5 cm^-3 and for the SSC models, the median densities are about one order of magnitude higher. However, to obtain a realistic description of the frequency-dependent variability amplitude of SgrA*, models with higher turnover frequencies and even higher densities are required. We discuss the results in the framework of possible deviations from equilibrium between particle and magnetic field energy. We also summarize alternative models to explain the broad-band variability of SgrA*., Comment: 14 pages, 3 figures, Conf. Proc. The Central Kiloparsec in Galactic Nuclei; Astronomy at High Angular Resolution 2011 (AHAR2011), held 29.8.2011-2.9.2011 at the DPG Physikzentrum Bad Honnef (Cologne/Bonn) Germany

Published
2012
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26. Beating the confusion limit: The necessity of high angular resolution for probing the physics of Sagittarius A* and its environment: Opportunities for LINC-NIRVANA (LBT), GRAVITY (VLTI) and and METIS (E-ELT)

Author

Eckart, A., Sabha, N., Witzel, G., Straubmeier, C., Shahzamanian, B., Valencia-S., M., Garcia-Marin, M., Horrobin, M., Moser, L., Zuther, J., Fischer, S., Rauch, C., Rost, S., Iserlohe, C., Yazici, S., Smajic, S., Wiest, M., Araujo-Hauck, C., and Wank, I.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

The super-massive 4 million solar mass black hole (SMBH) SgrA* shows variable emission from the millimeter to the X-ray domain. A detailed analysis of the infrared light curves allows us to address the accretion phenomenon in a statistical way. The analysis shows that the near-infrared flux density excursions are dominated by a single state power law, with the low states of SgrA* limited by confusion through the unresolved stellar background. We show that for 8-10m class telescopes blending effects along the line of sight will result in artificial compact star-like objects of 0.5-1 mJy that last for about 3-4 years. We discuss how the imaging capabilities of GRAVITY at the VLTI, LINC-NIRVANA at the LBT and METIS at the E-ELT will contribute to the investigation of the low variability states of SgrA*., Comment: 19 pages, 5 figure, Conf. Proc. SPIE Astronomical Telescopes + Instrumentation 1 - 6 July 2012. Amsterdam No. 8445-4

Published
2012
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27. The Low Latency Fault Tolerance System

Author

Zhao, Wenbing, Melliar-Smith, P. M., and Moser, L. E.

Subjects
Computer Science - Distributed, Parallel, and Cluster Computing
Abstract

The Low Latency Fault Tolerance (LLFT) system provides fault tolerance for distributed applications, using the leader-follower replication technique. The LLFT system provides application-transparent replication, with strong replica consistency, for applications that involve multiple interacting processes or threads. The LLFT system comprises a Low Latency Messaging Protocol, a Leader-Determined Membership Protocol, and a Virtual Determinizer Framework. The Low Latency Messaging Protocol provides reliable, totally ordered message delivery by employing a direct group-to-group multicast, where the message ordering is determined by the primary replica in the group. The Leader-Determined Membership Protocol provides reconfiguration and recovery when a replica becomes faulty and when a replica joins or leaves a group, where the membership of the group is determined by the primary replica. The Virtual Determinizer Framework captures the ordering information at the primary replica and enforces the same ordering at the backup replicas for major sources of non-determinism, including multi-threading, time-related operations and socket communication. The LLFT system achieves low latency message delivery during normal operation and low latency reconfiguration and recovery when a fault occurs.

Published
2010

32. Enhanced performance in fusion plasmas through turbulence suppression by megaelectronvolt ions

Author

Mazzi, S., Garcia, J., Zarzoso, D., Kazakov, Y., Ongena, J., Dreval, M., Nocente, M., Stancar, Z., Szepesi, G., Eriksson, J., Sahlberg, A., Benkadda, S., Abid, N., Abraham, K., Abreu, P., Adabonyan, O., Adrich, P., Afanasev, V., Afzal, M., Ahlgren, T., Aho-Mantila, L., Aiba, N., Airila, M., Akhtar, M., Albanese, R., Alderson-Martin, M., Alegre, D., Aleiferis, S., Aleksa, A., Alekseev, A., Alessi, E., Aleynikov, P., Algualcil, J., Ali, M., Allinson, M., Alper, B., Alves, E., Ambrosino, G., Ambrosino, R., Amosov, V., Andersson Sunden, E., Andrew, P., Angelini, B., Angioni, C., Antoniou, I., Appel, L., Appelbee, C., Aria, S., Ariola, M., Artaserse, G., Arter, W., Artigues, V., Asakura, N., Ash, A., Ashikawa, N., Aslanyan, V., Astrain, M., Asztalos, O., Auld, D., Auriemma, F., Austin, Y., Avotina, L., Aymerich, E., Baciero, A., Bairaktaris, F., Balbin, J., Balbinot, L., Balboa, I., Balden, M., Balshaw, C., Balshaw, N., Bandaru, V., Banks, J., Baranov, Y., Barcellona, C., Barnard, A., Barnard, M., Barnsley, R., Barth, A., Baruzzo, M., Barwell, S., Bassan, M., Batista, A., Batistoni, P., Baumane, L., Bauvir, B., Baylor, L., Beaumont, P., Beckett, D., Begolli, A., Beidler, M., Bekris, N., Beldishevski, M., Belli, E., Belli, F., Belonohy, E., Ben Yaala, M., Benayas, J., Bentley, J., Bergsaker, H., Bernardo, J., Bernert, M., Berry, M., Bertalot, L., Betar, H., Beurskens, M., Bickerton, S., Bieg, B., Bielecki, J., Bierwage, A., Biewer, T., Bilato, R., Bílkova, P., Birkenmeier, G., Bishop, H., Bizarro, J., Blackburn, J., Blanchard, P., Blatchford, P., Bobkov, V., Boboc, A., Bohm, P., Bohm, T., Bolshakova, I., Bolzonella, T., Bonanomi, N., Bonfiglio, D., Bonnin, X., Bonofiglo, P., Boocock, S., Booth, A., Booth, J., Borba, D., Borodin, D., Borodkina, I., Boulbe, C., Bourdelle, C., Bowden, M., Boyd, K., Bozicevic Mihalic, I., Bradnam, S., Braic, V., Brandt, L., Bravanec, R., Breizman, B., Brett, A., Brezinsek, S., Brix, M., Bromley, K., Brown, B., Brunetti, D., Buckingham, R., Buckley, M., Budny, R., Buermans, J., Bufferand, H., Buratti, P., Burgess, A., Buscarino, A., Busse, A., Butcher, D., Cal, E., Calabro, G., Calacci, L., Calado, R., Camenen, Y., Canal, G., Cannas, B., Cappelli, M., Carcangiu, S., Card, P., Cardinali, A., Carman, P., Carnevale, D., Carr, M., Carralero, D., Carraro, L., Carvalho, I., Carvalho, P., Casiraghi, I., Casson, F., Castaldo, C., Catalan, J., Catarino, N., Causa, F., Cavedon, M., Cecconello, M., Challis, C., Chamberlain, B., Chang, C., Chankin, A., Chapman, B., Chernyshova, M., Chiariello, A., Chmielewski, P., Chomiczewska, A., Chone, L., Ciraolo, G., Ciric, D., Citrin, J., Ciupinski, t., Clark, M., Clarkson, R., Clements, C., Cleverly, M., Coad, J., Coates, P., Cobalt, A., Coccorese, V., Coelho, R., Coenen, J., Coffey, I., Colangeli, A., Colas, L., Collins, C., Collins, J., Collins, S., Conka, D., Conroy, S., Conway, B., Conway, N., Coombs, D., Cooper, P., Cooper, S., Corradino, C., Corrigan, G., Coster, D., Cox, P., Craciunescu, T., Cramp, S., Crapper, C., Craven, D., Craven, R., Crialesi Esposito, M., Croci, G., Croft, D., Croitoru, A., Crombe, K., Cronin, T., Cruz, N., Crystal, C., Cseh, G., Cufar, A., Cullen, A., Curuia, M., Czarski, T., Dabirikhah, H., Dal Molin, A., Dale, E., Dalgliesh, P., Dalley, S., Dankowski, J., David, P., Davies, A., Davies, S., Davis, G., Dawson, K., Dawson, S., Day, I., De Bock, M., De Temmerman, G., De Tommasi, G., Deakin, K., Deane, J., Dejarnac, R., Del Sarto, D., Delabie, E., Del-Castillo-Negrete, D., Dempsey, A., Dendy, R., Devynck, P., Di Siena, A., Di Troia, C., Dickson, T., Dinca, P., Dittmar, T., Dobrashian, J., Doerner, R., Donne, A., Dorling, S., Dormido-Canto, S., Douai, D., Dowson, S., Doyle, R., Drewelow, P., Drews, P., Drummond, G., Duckworth, P., Dudding, H., Dumont, R., Dumortier, P., Dunai, D., Dunatov, T., Dunne, M., Duran, I., Durodie, F., Dux, R., Dvornova, A., Eastham, R., Edwards, J., Eich, T., Eichorn, A., Eidietis, N., Eksaeva, A., Haroun, H., Ellwood, G., Elsmore, C., Embreus, O., Emery, S., Ericsson, G., Eriksson, B., Eriksson, F., Eriksson, L., Ertmer, S., Esquembri, S., Esquisabel, A., Estrada, T., Evans, G., Evans, S., Fable, E., Fagan, D., Faitsch, M., Falessi, M., Fanni, A., Farahani, A., Farquhar, I., Fasoli, A., Faugeras, B., Fazinie, S., Felici, F., Felton, R., Fernandes, A., Fernandes, H., Ferrand, J., Ferreira, D., Ferreira, J., Ferro, G., Fessey, J., Ficker, O., Field, A., Figueiredo, A., Figueiredo, J., Fil, A., Fil, N., Finburg, P., Fiorucci, D., Fischer, U., Fishpool, G., Fittill, L., Fitzgerald, M., Flammini, D., Flanagan, J., Flinders, K., Foley, S., Fonnesu, N., Fontana, M., Fontdecaba, J., Forbes, S., Formisano, A., Fornal, T., Fortuna, L., Fortuna-Zalesna, E., Fortune, M., Fowler, C., Fransson, E., Frassinetti, L., Freisinger, M., Fresa, R., Fridstrom, R., Frigione, D., Fülop, T., Furseman, M., Fusco, V., Futatani, S., Gadariya, D., Gal, K., Galassi, D., Gafezka, K., Galeani, S., Gallart, D., Galvao, R., Gao, Y., Garcia-Munoz, M., Gardener, M., Garzotti, L., Gaspar, J., Gatto, R., Gaudio, P., Gear, D., Gebhart, T., Gee, S., Gelfusa, M., George, R., Gerasimov, S., Gervasini, G., Gethins, M., Ghani, Z., Gherendi, M., Ghezzi, F., Giacalone, J., Giacomelli, L., Giacometti, G., Gibson, C., Gibson, K., Gil, L., Gillgren, A., Gin, D., Giovannozzi, E., Giroud, C., Glen, R., Gloggler, S., Goff, J., Gohil, P., Goloborodko, V., Gomes, R., Goncalves, B., Goniche, M., Goodyear, A., Gore, S., Gorini, G., Görler, T., Gotts, N., Goulding, R., Gow, E., Graham, B., Graves, J., Greuner, H., Grierson, B., Griffiths, J., Griph, S., Grist, D., Gromelski, W., Groth, M., Grove, R., Gruca, M., Guard, D., Gupta, N., Gurl, C., Gusarov, A., Hackett, L., Hacquin, S., Hager, R., Hagg, L., Hakola, A., Halitovs, M., Hall, S., Hallworth-Cook, S., Ham, C., Hamaguchi, D., Hamed, M., Hamlyn-Harris, C., Hammond, K., Harford, E., Harrison, J., Harting, D., Hatano, Y., Hatch, D., Haupt, T., Hawes, J., Hawkes, N., Hawkins, J., Hayashi, T., Hazael, S., Hazel, S., Heesterman, P., Heidbrink, B., Helou, W., Hemming, O., Henderson, S., Henriques, R., Hepple, D., Herfindal, J., Hermon, G., Hill, J., Hillesheim, J., Hizanidis, K., Hjalmarsson, A., Ho, A., Hobirk, J., Hoenen, O., Hogben, C., Hollingsworth, A., Hollis, S., Hollmann, E., Hoelzl, M., Homan, B., Hook, M., Hopley, D., Horacek, J., Horsley, D., Horsten, N., Horton, A., Horton, L., Horvath, L., Hotchin, S., Howell, R., Hu, Z., Huber, A., Huber, V., Huddleston, T., Huijsmans, G., Huynh, P., Hynes, A., Iliasova, M., lmrie, D., lmrísek, M., lngleby, J., Innocente, P., Insulander Björk, K., Isernia, N., lvanova-Stanik, I., lvings, E., Jablonski, S., Jachmich, S., Jackson, T., Jacquet, P., Järleblad, H., Jaulmes, F., Jenaro Rodriguez, J., Jepu, I., Joffrin, E., Johnson, R., Johnson, T., Johnston, J., Jones, C., Jones, G., Jones, L., Jones, N., Jones, T., Joyce, A., Juarez, R., Juvonen, M., Kalnina, P., Kaltiaisenaho, T., Kaniewski, J., Kantor, A., Kappatou, A., Karhunen, J., Karkinsky, D., Kashchuk, Y., Kaufman, M., Kaveney, G., Kazantzidis, V., Keeling, D., Kelly, R., Kempenaars, M., Kennedy, C., Kennedy, D., Kent, J., Khan, K., Khilkevich, E., Kiefer, C., Kilpeläinen, J., Kim, C., Kim, H., Kim, S., King, D., King, R., Kinna, D., Kiptily, V., Kirjasuo, A., Kirov, K., Kirschner, A., kiviniemi, T., Kizane, G., Klas, M., Klepper, C., Klix, A., Kneale, G., Knight, M., Knight, P., Knights, R., Knipe, S., Knolker, M., Knott, S., Kocan, M., Kochl, F., Kodeli, I., Kolesnichenko, Y., Kominis, Y., Kong, M., Korovin, V., Kos, B., Kos, D., Koslowski, H., Kotschenreuther, M., Koubiti, M., Kowalska-Strzeciwilk, E., Koziol, K., Krasilnikov, A., Krasilnikov, V., Kresina, M., Krieger, K., Krishnan, N., Krivska, A., Kruezi, U., Ksiezek, I., Kukushkin, A., Kumpulainen, H., Kurki-Suonio, T., Kurotaki, H., Kwak, S., Kwon, O., Laguardia, L., Lagzdina, E., Lahtinen, A., Laing, A., Lam, N., Lambertz, H., Lane, B., Lane, C., Lascas Neto, E., Laszyriska, E., Lawson, K., Lazaros, A., Lazzaro, E., Learoyd, G., Lee, C., Lee, S., Leerink, S., Leeson, T., Lefebvre, X., Leggate, H., Lehmann, J., Lehnen, M., Leichtle, D., Leipold, F., Lengar, I., Lennholm, M., Leon Gutierrez, E., Lepiavko, B., Leppanen, J., Lerche, E., Lescinskis, A., Lewis, J., Leysen, W., Li, L., Li, Y., Likonen, J., Linsmeier, C., Lipschultz, B., Litaudon, X., Litherland-Smith, E., Liu, F., Loarer, T., Loarte, A., Lobel, R., Lomanowski, B., Lomas, P., Lopez, J., Lorenzini, R., Loreti, S., Losada, U., Loschiavo, V., Loughlin, M., Louka, Z., Lovell, J., Lowe, T., Lowry, C., Lubbad, S., Luce, T., Lucock, R., Lukin, A., Luna, C., Luna, E., Lungaroni, M., Lungu, C., Lunt, T., Lutsenko, V., Lyons, B., Lyssoivan, A., Machielsen, M., Macusova, E., Mäenpää, R., Maggi, C., Maggiora, R., Magness, M., Mahesan, S., Maier, H., Maingi, R., Malinowski, K., Manas, P., Mantica, P., Mantsinen, M., Manyer, J., Manzanares, A., Maquet, P., Marceca, G., Marcenko, N., Marchetto, C., Marchuk, O., 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moléculaires (PIIM), Aix Marseille Université (AMU)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherche sur la Fusion par confinement Magnétique (IRFM), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Swiss Plasma Center (SPC), Ecole Polytechnique Fédérale de Lausanne (EPFL), Laboratory for Plasma Physics (LPP), Ecole Royale Militaire / Koninklijke Militaire School (ERM KMS), Kharkiv Institute of Physics and Technology (Ukraine), V.N. Karazin Kharkiv National University (KhNU), Dipartimento di Fisica (Milano), Università degli Studi di Milano = University of Milan (UNIMI), Consiglio Nazionale delle Ricerche [Milano] (CNR), Jozef Stefan Institute [Ljubljana] (IJS), Culham Centre for Fusion Energy (CCFE), Department of Physics and Astronomy [Uppsala], Uppsala University, This work has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom research and training programme 2014–2018 and 2019–2020 under Grant agreement No 633053., Mazzi, S, Garcia, J, Zarzoso, D, Kazakov, Y, Ongena, J, Dreval, M, Nocente, M, Stancar, Z, Szepesi, G, Eriksson, J, Sahlberg, A, Benkadda, S, Abid, N, Abraham, K, Abreu, P, Adabonyan, O, Adrich, P, Afzal, M, Ahlgren, T, Aho-Mantila, L, Aiba, N, Airila, M, Akhtar, M, Albanese, R, Alderson-Martin, M, Alegre, D, Aleiferis, S, Aleksa, A, Alessi, E, Aleynikov, P, Algualcil, J, Ali, M, Allinson, M, Alper, B, Alves, E, Ambrosino, G, Ambrosino, R, 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K., Zoulias, I., Zwingmann, W., Zychor, I., JET Contributors, Science and Technology of Nuclear Fusion, EIRES Eng. for Sustainable Energy Systems, Magneto-Hydro-Dynamic Stability of Fusion Plasmas, Applied Physics and Science Education, Kazakov, Yo, VTT Technical Research Centre of Finland, Culham Science Centre, Princeton Plasma Physics Laboratory, Department of Applied Physics, European Commission, Forschungszentrum Jülich, Universidade Lisboa, Fusion and Plasma Physics, University of Milan - Bicocca, Aalto University, General Atomics, ITER, University of Toyama, CEA, Oak Ridge National Laboratory, Technical University of Madrid, Swiss Federal Institute of Technology Lausanne, Dutch Institute for Fundamental Energy Research, Royal Military Academy, Seoul National University, Chalmers University of Technology, Max Planck Institute for Plasma Physics, KTH Royal Institute of Technology, and Aalto-yliopisto

Subjects
[PHYS]Physics [physics], Settore FIS/01, Settore ING-IND/18 - Fisica dei Reattori Nucleari, General Physics and Astronomy, simulation, magnetically confined plasma, nuclear fusion, tokamaks, turbulence suppression, Plasma, [PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph], confinement, transport, Alpha particles, Fusion reactors, Turbulence, physics
Abstract

openaire: EC/H2020/633053/EU//EUROfusion Funding Information: We thank M. Baruzzo and F. Nave for the preparation and execution of JET experiments discussed in this paper; E. de la Luna for support in detailing the experimental diagnostics of JET; A. Ho for assistance in processing the experimental data; T. Görler for providing essential advice to ensure the correct numerical setup for the GENE modelling reported in this paper; Y. Camenen, X. Garbet and A. Bierwage for fruitful discussions about the gyrokinetic analyses; G. Giruzzi for valuable suggestions on the article strategy. The simulations were performed on the IRENE Joliot-Curie HPC system, in the framework of the PRACE projects IONFAST and AFIETC, led by J. Garcia, and on the CINECA Marconi HPC within the project GENE4EP, led by D. Zarzoso. This work has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom research and training programme 2014-2018 and 2019-2020 under grant agreement no. 633053. The views and opinions express herein do not necessarily reflect those of the European Commission. Part of the work by Ye. O. Kazakov and J.Ongena was also carried out in the framework of projects done for the ITER Scientist Fellow Network (ISFN). Funding Information: We thank M. Baruzzo and F. Nave for the preparation and execution of JET experiments discussed in this paper; E. de la Luna for support in detailing the experimental diagnostics of JET; A. Ho for assistance in processing the experimental data; T. Görler for providing essential advice to ensure the correct numerical setup for the GENE modelling reported in this paper; Y. Camenen, X. Garbet and A. Bierwage for fruitful discussions about the gyrokinetic analyses; G. Giruzzi for valuable suggestions on the article strategy. The simulations were performed on the IRENE Joliot-Curie HPC system, in the framework of the PRACE projects IONFAST and AFIETC, led by J. Garcia, and on the CINECA Marconi HPC within the project GENE4EP, led by D. Zarzoso. This work has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom research and training programme 2014-2018 and 2019-2020 under grant agreement no. 633053. The views and opinions express herein do not necessarily reflect those of the European Commission. Part of the work by Ye. O. Kazakov and J.Ongena was also carried out in the framework of projects done for the ITER Scientist Fellow Network (ISFN). Publisher Copyright: © 2022, The Author(s), under exclusive licence to Springer Nature Limited. Alpha particles with energies on the order of megaelectronvolts will be the main source of plasma heating in future magnetic confinement fusion reactors. Instead of heating fuel ions, most of the energy of alpha particles is transferred to electrons in the plasma. Furthermore, alpha particles can also excite Alfvénic instabilities, which were previously considered to be detrimental to the performance of the fusion device. Here we report improved thermal ion confinement in the presence of megaelectronvolts ions and strong fast ion-driven Alfvénic instabilities in recent experiments on the Joint European Torus. Detailed transport analysis of these experiments reveals turbulence suppression through a complex multi-scale mechanism that generates large-scale zonal flows. This holds promise for more economical operation of fusion reactors with dominant alpha particle heating and ultimately cheaper fusion electricity.

Published
2022

33. Disruption prediction with artificial intelligence techniques in tokamak plasmas

Author

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J., Ratynskaia S., Rebai M., Refy D., Reichle R., Reinke M., Reiser D., Reux C., Reynolds S., Richiusa M. L., Richyal S., Rigamonti D., Rimini F. G., Risner J., Riva M., Rivero-Rodriguez J., Roach C. M., Robins R., Robinson S., Robson D., Rodionov R., Rodrigues P., Ramos M. R., Rodriguez-Fernandez P., Romanelli F., Romanelli M., Romanelli S., Romazanov J., Rossi R., Rowe S., Rowlands D., Rubel M., Rubinacci G., Rubino G., Ruchko L., Ruiz M., Ruiz J. R., Ruset C., Rzadkiewicz J., Saarelma S., Safi E., Sahlberg A., Salewski M., Salmi A., Salmon R., Salzedas F., Sanders I., Sandiford D., Santos B., Santucci A., Sarkimaki K., Sarwar R., Sarychev I., Sauter O., Sauwan P., Scapin N., Schluck F., Schmid K., Schmuck S., Schneider M., Schneider P. A., Schworer D., Scott G., Scott M., Scraggs D., Scully S., Segato M., Seo J., Sergienko G., Sertoli M., Sharapov S. E., Shaw A., Sheikh H., Sheikh U., Shepherd A., Shevelev A., Shigin P., Shinohara K., Shiraiwa S., Shiraki D., Short M., Sias G., Silburn S. A., Silva A., Silva C., Silva J., Silvagni D., Simfukwe D., Simpson J., Sinclair D., Sipila S. K., Sips A. C. C., Siren P., Sirinelli A., Sjostrand H., Skinner N., Slater J., Smith N., Smith P., Snell J., Snoep G., Snoj L., Snyder P., Soare S., Solano E. R., Solokha V., Somers A., Sommariva C., Soni K., Sorokovoy E., Sos M., Sousa J., Sozzi C., Spagnolo S., Spelzini T., Spineanu F., Spong D., Sprada D., Sridhar S., Srinivasan C., Stables G., Staebler G., Stamatelatos I., Stancar Z., Staniec P., Stankunas G., Stead M., Stefanikova E., Stephen A., Stephens J., Stevenson P., Stojanov M., Strand P., Strauss H. R., Strikwerda S., Strom P., Stuart C. I., Studholme W., Subramani M., Suchkov E., Sumida S., Sun H. J., Susts T. E., Svensson J., Svoboda J., Sweeney R., Sytnykov D., Szabolics T., Szepesi G., Tabia B., Tadic T., Tal B., Tala T., Tallargio A., Tamain P., Tan H., Tanaka K., Tang W., Tardocchi M., Taylor D., Teimane A. S., Telesca G., Teplova N., Teplukhina A., Terentyev D., Terra A., Terranova D., Terranova N., Testa D., Tholerus E., Thomas J., Thoren E., Thorman A., Tierens W., Tinguely R. A., Tipton A., Todd H., Tokitani M., Tolias P., Tomes M., Tookey A., Torikai Y., von Toussaint U., Tsavalas P., Tskhakaya D., Turner I., Turner M., Turner M. M., Turnyanskiy M., Tvalashvili G., Tyrrell S., Tyshchenko M., Uccello A., Udintsev V., Urbanczyk G., Vadgama A., Valcarcel D., Valisa M., Olivares P. V., Vallhagen O., Valovic M., Eester D. V., Varje J., Vartanian S., Vasilopoulou T., Vayakis G., Vecsei M., Ventre S., Verdoolaege G., Verona C., Rinati G. V., Veshchev E., Vianello N., Viezzer E., Vignitchouk L., Vila R., Villari R., Villone F., Vincenzi P., Vinyar I., Viola B., Virtanen A. J., Vitins A., Vizvary Z., Vlad G., Vlad M., Vondracek P., de Vries P., Wakeling B., Walkden N. R., Walker M., Walker R., Walsh M., Wang E., Wang N., Warder S., Warren R., Waterhouse J., Watts C., Wauters T., Weckmann A., Maxwell H. W., Weiland M., Weisen H., Weiszflog M., Welch P., Wendler N., West A., Wheatley M., Wheeler S., Whitehead A., Whittaker D., Widdowson A., Wiesen S., Wilkinson J., Williams J. C., Willoughby D., Wilson I., Wilson J., Wilson T., Wischmeier M., Wise P., Withenshaw G., Withycombe A., Witts D., Wojcik-Gargula A., Wolfrum E., Wood R., Woodley C., Woodley R., Woods B., Wright J., Wright J. C., Xu T., Yadikin D., Yajima M., Yakovenko Y., Yang Y., Yanling W., Yanovskiy V., Young I., Young R., Zabolockis R. J., Zacks J., Zagorski R., Zaitsev F. S., Zakharov L., Zarins A., Fernandez D. Z., Zastrow K. -D., Zayachuk Y., Zerbini M., Zhang W., Zhou Y., Zlobinski M., Zocco A., Zohar A., Zoita V., Zoletnik S., Zotta V. 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Abstract

In nuclear fusion reactors, plasmas are heated to very high temperatures of more than 100 million kelvin and, in so-called tokamaks, they are confined by magnetic fields in the shape of a torus. Light nuclei, such as deuterium and tritium, undergo a fusion reaction that releases energy, making fusion a promising option for a sustainable and clean energy source. Tokamak plasmas, however, are prone to disruptions as a result of a sudden collapse of the system terminating the fusion reactions. As disruptions lead to an abrupt loss of confinement, they can cause irreversible damage to present-day fusion devices and are expected to have a more devastating effect in future devices. Disruptions expected in the next-generation tokamak, ITER, for example, could cause electromagnetic forces larger than the weight of an Airbus A380. Furthermore, the thermal loads in such an event could exceed the melting threshold of the most resistant state-of-the-art materials by more than an order of magnitude. To prevent disruptions or at least mitigate their detrimental effects, empirical models obtained with artificial intelligence methods, of which an overview is given here, are commonly employed to predict their occurrence—and ideally give enough time to introduce counteracting measures.

Published
2022

34. Enhanced performance in fusion plasmas through turbulence suppression by megaelectronvolt ions

Author

Mazzi, S, Garcia, J, Zarzoso, D, Kazakov, Y, Ongena, J, Dreval, M, Nocente, M, Stancar, Z, Szepesi, G, Eriksson, J, Sahlberg, A, Benkadda, S, Abid, N, Abraham, K, Abreu, P, Adabonyan, O, Adrich, P, Afzal, M, Ahlgren, T, Aho-Mantila, L, Aiba, N, Airila, M, Akhtar, M, Albanese, R, Alderson-Martin, M, Alegre, D, Aleiferis, S, Aleksa, A, Alessi, E, Aleynikov, P, Algualcil, J, Ali, M, Allinson, M, Alper, B, Alves, E, Ambrosino, G, Ambrosino, R, Andersson Sunden, E, Andrew, P, Angelini, B, Angioni, C, Antoniou, I, Appel, L, Appelbee, C, Aria, S, Ariola, M, Artaserse, G, Arter, W, Artigues, V, Asakura, N, Ash, A, Ashikawa, N, Aslanyan, V, Astrain, M, Asztalos, O, Auld, D, Auriemma, F, Austin, Y, Avotina, L, Aymerich, E, Baciero, A, Bairaktaris, F, Balbin, J, Balbinot, L, Balboa, I, Balden, M, Balshaw, C, Balshaw, N, Bandaru, V, Banks, J, Baranov, Y, Barcellona, C, Barnard, A, Barnard, M, Barnsley, R, Barth, A, Baruzzo, M, Barwell, S, Bassan, M, Batista, A, Batistoni, P, Baumane, L, Bauvir, B, Baylor, L, Beaumont, P, Beckett, D, Begolli, A, Beidler, M, Bekris, N, Beldishevski, M, Belli, E, Belli, F, Belonohy, E, Ben Yaala, M, Benayas, J, Bentley, J, Bergsaker, H, Bernardo, J, Bernert, M, Berry, M, Bertalot, L, Betar, H, Beurskens, M, Bickerton, S, Bieg, B, Bielecki, J, Bierwage, A, Biewer, T, Bilato, R, Bilkova, P, Birkenmeier, G, Bishop, H, Bizarro, J, Blackburn, J, Blanchard, P, Blatchford, P, Bobkov, V, Boboc, A, Bohm, P, Bohm, T, Bolshakova, I, Bolzonella, T, Bonanomi, N, Bonfiglio, D, Bonnin, X, Bonofiglo, P, Boocock, S, Booth, A, Booth, J, Borba, D, Borodin, D, Borodkina, I, Boulbe, C, Bourdelle, C, Bowden, M, Boyd, K, Bozicevic Mihalic, I, Bradnam, S, Braic, V, Brandt, L, Bravanec, R, Breizman, B, Brett, A, Brezinsek, S, Brix, M, Bromley, K, Brown, B, Brunetti, D, Buckingham, R, Buckley, M, Budny, R, Buermans, J, Bufferand, H, Buratti, P, Burgess, A, Buscarino, A, Busse, A, Butcher, D, de la Cal, E, Calabro, G, Calacci, L, Calado, R, Camenen, Y, Canal, G, Cannas, B, Cappelli, M, Carcangiu, S, Card, P, Cardinali, A, Carman, P, Carnevale, D, Carr, M, Carralero, D, Carraro, L, Carvalho, I, Carvalho, P, Casiraghi, I, Casson, F, Castaldo, C, Catalan, J, Catarino, N, Causa, F, Cavedon, M, Cecconello, M, Challis, C, Chamberlain, B, Chang, C, Chankin, A, Chapman, B, Chernyshova, M, Chiariello, A, Chmielewski, P, Chomiczewska, A, Chone, L, Ciraolo, G, Ciric, D, Citrin, J, Ciupinski, L, Clark, M, Clarkson, R, Clements, C, Cleverly, M, Coad, J, Coates, P, Cobalt, A, Coccorese, V, Coelho, R, Coenen, J, Coffey, I, Colangeli, A, Colas, L, Collins, C, Collins, J, Collins, S, Conka, D, Conroy, S, Conway, B, Conway, N, Coombs, D, Cooper, P, Cooper, S, Corradino, C, Corrigan, G, Coster, D, Cox, P, Craciunescu, T, Cramp, S, Crapper, C, Craven, D, Craven, R, Crialesi Esposito, M, Croci, G, Croft, D, Croitoru, A, Crombe, K, Cronin, T, Cruz, N, Crystal, C, Cseh, G, Cufar, A, Cullen, A, Curuia, M, Czarski, T, Dabirikhah, H, Molin, A, Dale, E, Dalgliesh, P, Dalley, S, Dankowski, J, David, P, Davies, A, Davies, S, Davis, G, Dawson, K, Dawson, S, Day, I, De Bock, M, De Temmerman, G, De Tommasi, G, Deakin, K, Deane, J, Dejarnac, R, Del Sarto, D, Delabie, E, Del-Castillo-Negrete, D, Dempsey, A, Dendy, R, Devynck, P, Di Siena, A, Di Troia, C, Dickson, T, Dinca, P, Dittmar, T, Dobrashian, J, Doerner, R, Donne, A, Dorling, S, Dormido-Canto, S, Douai, D, Dowson, S, Doyle, R, Drewelow, P, Drews, P, Drummond, G, Duckworth, P, Dudding, H, Dumont, R, Dumortier, P, Dunai, D, Dunatov, T, Dunne, M, Duran, I, Durodie, F, Dux, R, Dvornova, A, Eastham, R, Edwards, J, Eich, T, Eichorn, A, Eidietis, N, Eksaeva, A, El Haroun, H, Ellwood, G, Elsmore, C, Embreus, O, Emery, S, Ericsson, G, Eriksson, B, Eriksson, F, Eriksson, L, Ertmer, S, Esquembri, S, Esquisabel, A, Estrada, T, Evans, G, Evans, S, Fable, E, Fagan, D, Faitsch, M, Falessi, M, Fanni, A, Farahani, A, Farquhar, I, Fasoli, A, Faugeras, B, Fazinic, S, Felici, F, Felton, R, Fernandes, A, Fernandes, H, Ferrand, J, Ferreira, D, Ferreira, J, Ferro, G, Fessey, J, Ficker, O, Field, A, Figueiredo, A, Figueiredo, J, Fil, A, Fil, N, Finburg, P, Fiorucci, D, Fischer, U, Fishpool, G, Fittill, L, Fitzgerald, M, Flammini, D, Flanagan, J, Flinders, K, Foley, S, Fonnesu, N, Fontana, M, Fontdecaba, J, Forbes, S, Formisano, A, Fornal, T, Fortuna, L, Fortuna-Zalesna, E, Fortune, M, Fowler, C, Fransson, E, Frassinetti, L, Freisinger, M, Fresa, R, Fridstrom, R, Frigione, D, Fulop, T, Furseman, M, Fusco, V, Futatani, S, Gadariya, D, Gal, K, Galassi, D, Galazka, K, Galeani, S, Gallart, D, Galvao, R, Gao, Y, Garcia-Munoz, M, Gardener, M, Garzotti, L, Gaspar, J, Gatto, R, Gaudio, P, Gear, D, Gebhart, T, Gee, S, Gelfusa, M, George, R, Gerasimov, S, Gervasini, G, Gethins, M, Ghani, Z, Gherendi, M, Ghezzi, F, Giacalone, J, Giacomelli, L, Giacometti, G, Gibson, C, Gibson, K, Gil, L, Gillgren, A, Giovannozzi, E, Giroud, C, Glen, R, Gloggler, S, Goff, J, Gohil, P, Goloborodko, V, Gomes, R, Goncalves, B, Goniche, M, Goodyear, A, Gore, S, Gorini, G, Gorler, T, Gotts, N, Goulding, R, Gow, E, Graham, B, Graves, J, Greuner, H, Grierson, B, Griffiths, J, Griph, S, Grist, D, Gromelski, W, Groth, M, Grove, R, Gruca, M, Guard, D, Gupta, N, Gurl, C, Gusarov, A, Hackett, L, Hacquin, S, Hager, R, Hagg, L, Hakola, A, Halitovs, M, Hall, S, Hallworth-Cook, S, Ham, C, Hamaguchi, D, Hamed, M, Hamlyn-Harris, C, Hammond, K, Harford, E, Harrison, J, Harting, D, Hatano, Y, Hatch, D, Haupt, T, Hawes, J, Hawkes, N, Hawkins, J, Hayashi, T, Hazael, S, Hazel, S, Heesterman, P, Heidbrink, B, Helou, W, Hemming, O, Henderson, S, Henriques, R, Hepple, D, Herfindal, J, Hermon, G, Hill, J, Hillesheim, J, Hizanidis, K, Hjalmarsson, A, Ho, A, Hobirk, J, Hoenen, O, Hogben, C, Hollingsworth, A, Hollis, S, Hollmann, E, Holzl, M, Homan, B, Hook, M, Hopley, D, Horacek, J, Horsley, D, Horsten, N, Horton, A, Horton, L, Horvath, L, Hotchin, S, Howell, R, Hu, Z, Huber, A, Huber, V, Huddleston, T, Huijsmans, G, Huynh, P, Hynes, A, Imrie, D, Imrisek, M, Ingleby, J, Innocente, P, Insulander Bjork, K, Isernia, N, Ivanova-Stanik, I, Ivings, E, Jablonski, S, Jachmich, S, Jackson, T, Jacquet, P, Jarleblad, H, Jaulmes, F, Rodriguez, J, Jepu, I, Joffrin, E, Johnson, R, Johnson, T, Johnston, J, Jones, C, Jones, G, Jones, L, Jones, N, Jones, T, Joyce, A, Juarez, R, Juvonen, M, Kalnina, P, Kaltiaisenaho, T, Kaniewski, J, Kantor, A, Kappatou, A, Karhunen, J, Karkinsky, D, Kaufman, M, Kaveney, G, Kazantzidis, V, Keeling, D, Kelly, R, Kempenaars, M, Kennedy, C, Kennedy, D, Kent, J, Khan, K, Kiefer, C, Kilpelainen, J, Kim, C, Kim, H, Kim, S, King, D, King, R, Kinna, D, Kiptily, V, Kirjasuo, A, Kirov, K, Kirschner, A, Kiviniemi, T, Kizane, G, Klas, M, Klepper, C, Klix, A, Kneale, G, Knight, M, Knight, P, Knights, R, Knipe, S, Knolker, M, Knott, S, Kocan, M, Kochl, F, Kodeli, I, Kolesnichenko, Y, Kominis, Y, Kong, M, Korovin, V, Kos, B, Kos, D, Koslowski, H, Kotschenreuther, M, Koubiti, M, Kowalska-Strzeciwilk, E, Koziol, K, Krasilnikov, V, Kresina, M, Krieger, K, Krishnan, N, Krivska, A, Kruezi, U, Ksiazek, I, Kukushkin, A, Kumpulainen, H, Kurki-Suonio, T, Kurotaki, H, Kwak, S, Kwon, O, Laguardia, L, Lagzdina, E, Lahtinen, A, Laing, A, Lam, N, Lambertz, H, Lane, B, Lane, C, Lascas Neto, E, Laszynska, E, Lawson, K, Lazaros, A, Lazzaro, E, Learoyd, G, Lee, C, Lee, S, Leerink, S, Leeson, T, Lefebvre, X, Leggate, H, Lehmann, J, Lehnen, M, Leichtle, D, Leipold, F, Lengar, I, Lennholm, M, Leon Gutierrez, E, Lepiavko, B, Leppanen, J, Lerche, E, Lescinskis, A, Lewis, J, Leysen, W, Li, L, Li, Y, Likonen, J, Linsmeier, C, Lipschultz, B, Litaudon, X, Litherland-Smith, E, Liu, F, Loarer, T, Loarte, A, Lobel, R, Lomanowski, B, Lomas, P, Lopez, J, Lorenzini, R, Loreti, S, Losada, U, Loschiavo, V, Loughlin, M, Louka, Z, Lovell, J, Lowe, T, Lowry, C, Lubbad, S, Luce, T, Lucock, R, Luna, C, de la Luna, E, Lungaroni, M, Lungu, C, Lunt, T, Lutsenko, V, Lyons, B, Lyssoivan, A, Machielsen, M, Macusova, E, Maenpaa, R, Maggi, C, Maggiora, R, Magness, M, Mahesan, S, Maier, H, Mailloux, J, Maingi, R, Malinowski, K, Manas, P, Mantica, P, Mantsinen, M, Manyer, J, Manzanares, A, Maquet, P, Marceca, G, Marchetto, C, Marchuk, O, Mariani, A, Mariano, G, Marin, M, Marinelli, M, Markovic, T, Marocco, D, Marot, L, Marsden, S, Marsh, J, Marshall, R, Martellucci, L, Martin, A, Martone, R, Maruyama, S, Maslov, M, Masuzaki, S, Matejcik, S, Mattei, M, Matthews, G, Matveev, D, Matveeva, E, Mauriya, A, Maviglia, F, Mayer, M, Mayoral, M, Mazzotta, C, Mcadams, R, Mccarthy, P, Mcclements, K, Mcclenaghan, J, Mccullen, P, Mcdonald, D, Mcguckin, D, Mchugh, D, Mcintyre, G, Mckean, R, Mckehon, J, Mcmillan, B, Mcnamee, L, Mcshee, A, Meakins, A, Medley, S, Meekes, C, Meghani, K, Meigs, A, Meisl, G, Meitner, S, Menmuir, S, Mergia, K, Merriman, S, Mertens, P, Messiaen, A, Michling, R, Middleton, P, Middleton-Gear, D, Mietelski, J, Milanesio, D, Milani, E, Militello, F, Militello Asp, A, Milnes, J, Milocco, A, Miloshevsky, G, Minghao, C, Minucci, S, Miron, I, Miyamoto, M, Mlynar, J, Moiseenko, V, Monaghan, P, Monakhov, I, Moody, T, Moon, S, Mooney, R, Moradi, S, Morales, J, Morales, R, Mordijck, S, Moreira, L, Morgan, L, Moro, F, Morris, J, Morrison, K, Moser, L, Moulton, D, Mrowetz, T, Mundy, T, Muraglia, M, Murari, A, Muraro, A, Muthusonai, N, N'Konga, B, Na, Y, Nabais, F, Naden, M, Naish, J, Naish, R, Napoli, F, Nardon, E, Naulin, V, Nave, M, Nedzelskiy, I, Nestoras, I, Neu, R, Ng, S, Nicassio, M, Nielsen, A, Nina, D, Nishijima, D, Noble, C, Nobs, C, Nodwell, D, Nordlund, K, Nordman, H, Normanton, R, Noterdaeme, J, Nowak, S, Nunn, E, Nystrom, H, Oberparleiter, M, Obryk, B, O'Callaghan, J, Odupitan, T, Oliver, H, Olney, R, O'Mullane, M, Organ, E, Orsitto, F, Orszagh, J, Osborne, T, Otin, R, Otsuka, T, Owen, A, Oya, Y, Oyaizu, M, Paccagnella, R, Pace, N, Packer, L, Paige, S, Pajuste, E, Palade, D, Pamela, S, Panadero, N, Panontin, E, Papadopoulos, A, Papp, G, Papp, P, Parail, V, Pardanaud, C, Parisi, J, Parra Diaz, F, Parsloe, A, Parsons, M, Parsons, N, Passeri, M, Patel, A, Pau, A, Pautasso, G, Pavlichenko, R, Pavone, A, Pawelec, E, Soldan, C, Peacock, A, Pearce, M, Peluso, E, Penot, C, Pepperell, K, Pereira, R, Pereira, T, Cippo, E, Pereslavtsev, P, von Thun, C, Pericoli, V, Perry, D, Peterka, M, Petersson, P, Petravich, G, Petrella, N, Peyman, M, Pillon, M, Pinches, S, Pintsuk, G, de Sa, W, dos Reis, A, Piron, C, Piron, L, Pironti, A, Pitts, R, van de Plassche, K, Platt, N, Plyusnin, V, Podesta, M, Pokol, G, Poli, F, Pompilian, O, Popovichev, S, Poradzinski, M, Porfiri, M, Porkolab, M, Porosnicu, C, Porton, M, Poulipoulis, G, Predebon, I, Prestopino, G, Price, C, Price, D, Price, M, Primetzhofer, D, Prior, P, Provatas, G, Pucella, G, Puglia, P, Purahoo, K, Pusztai, I, Putignano, O, Putterich, T, Quercia, A, Rachlew, E, Radulescu, G, Radulovic, V, Rainford, M, Raj, P, Ralph, G, Ramogida, G, Rasmussen, D, Rasmussen, J, Ratta, G, Ratynskaia, S, Rebai, M, Refy, D, Reichle, R, Reinke, M, Reiser, D, Reux, C, Reynolds, S, Richiusa, M, Richyal, S, Rigamonti, D, Rimini, F, Risner, J, Riva, M, Rivero-Rodriguez, J, Roach, C, Robins, R, Robinson, S, Robson, D, Rodrigues, P, Rodriguez Ramos, M, Rodriguez-Fernandez, P, Romanelli, F, Romanelli, M, Romanelli, S, Romazanov, J, Rossi, R, Rowe, S, Rowlands, D, Rubel, M, Rubinacci, G, Rubino, G, Ruchko, L, Ruiz, M, Ruiz, J, Ruset, C, Rzadkiewicz, J, Saarelma, S, Safi, E, Salewski, M, Salmi, A, Salmon, R, Salzedas, F, Sanders, I, Sandiford, D, Santos, B, Santucci, A, Sarkimaki, K, Sarwar, R, Sarychev, I, Sauter, O, Sauwan, P, Scapin, N, Schluck, F, Schmid, K, Schmuck, S, Schneider, M, Schneider, P, Schworer, D, Scott, G, Scott, M, Scraggs, D, Scully, S, Segato, M, Seo, J, Sergienko, G, Sertoli, M, Sharapov, S, Shaw, A, Sheikh, H, Sheikh, U, Shepherd, A, Shigin, P, Shinohara, K, Shiraiwa, S, Shiraki, D, Short, M, Sias, G, Silburn, S, Silva, A, Silva, C, Silva, J, Silvagni, D, Simfukwe, D, Simpson, J, Sinclair, D, Sipila, S, Sips, A, Siren, P, Sirinelli, A, Sjostrand, H, Skinner, N, Slater, J, Smith, N, Smith, P, Snell, J, Snoep, G, Snoj, L, Snyder, P, Soare, S, Solano, E, Solokha, V, Somers, A, Sommariva, C, Soni, K, Sorokovoy, E, Sos, M, Sousa, J, Sozzi, C, Spagnolo, S, Spelzini, T, Spineanu, F, Spong, D, Sprada, D, Sridhar, S, Srinivasan, C, Stables, G, Staebler, G, Stamatelatos, I, Staniec, P, Stankunas, G, Stead, M, Stefanikova, E, Stephen, A, Stephens, J, Stevenson, P, Stojanov, M, Strand, P, Strauss, H, Strikwerda, S, Strom, P, Stuart, C, Studholme, W, Subramani, M, Suchkov, E, Sumida, S, Sun, H, Susts, T, Svensson, J, Svoboda, J, Sweeney, R, Sytnykov, D, Szabolics, T, Tabia, B, Tadic, T, Tal, B, Tala, T, Tallargio, A, Tamain, P, Tan, H, Tanaka, K, Tang, W, Tardocchi, M, Taylor, D, Teimane, A, Telesca, G, Teplukhina, A, Terentyev, D, Terra, A, Terranova, D, Terranova, N, Testa, D, Tholerus, E, Thomas, J, Thoren, E, Thorman, A, Tierens, W, Tinguely, R, Tipton, A, Todd, H, Tokitani, M, Tolias, P, Tomes, M, Tookey, A, Torikai, Y, von Toussaint, U, Tsavalas, P, Tskhakaya, D, Turner, I, Turner, M, Turnyanskiy, M, Tvalashvili, G, Tyrrell, S, Tyshchenko, M, Uccello, A, Udintsev, V, Urbanczyk, G, Vadgama, A, Valcarcel, D, Valisa, M, Vallejos Olivares, P, Vallhagen, O, Valovic, M, Van Eester, D, Varje, J, Vartanian, S, Vasilopoulou, T, Vayakis, G, Vecsei, M, Vega, J, Ventre, S, Verdoolaege, G, Verona, C, Rinati, G, Veshchev, E, Vianello, N, Viezzer, E, Vignitchouk, L, Vila, R, Villari, R, Villone, F, Vincenzi, P, Viola, B, Virtanen, A, Vitins, A, Vizvary, Z, Vlad, G, Vlad, M, Vondracek, P, de Vries, P, Wakeling, B, Walkden, N, Walker, M, Walker, R, Walsh, M, Wang, E, Wang, N, Warder, S, Warren, R, Waterhouse, J, Watts, C, Wauters, T, Weckmann, A, Wedderburn Maxwell, H, Weiland, M, Weisen, H, Weiszflog, M, Welch, P, Wendler, N, West, A, Wheatley, M, Wheeler, S, Whitehead, A, Whittaker, D, Widdowson, A, Wiesen, S, Wilkinson, J, Williams, J, Willoughby, D, Wilson, I, Wilson, J, Wilson, T, Wischmeier, M, Wise, P, Withenshaw, G, Withycombe, A, Witts, D, Wojcik-Gargula, A, Wolfrum, E, Wood, R, Woodley, C, Woodley, R, Woods, B, Wright, J, Xu, T, Yadikin, D, Yajima, M, Yakovenko, Y, Yang, Y, Yanling, W, Yanovskiy, V, Young, I, Young, R, Zabolockis, R, Zacks, J, Zagorski, R, Zaitsev, F, Zakharov, L, Zarins, A, Zastrow, K, Zayachuk, Y, Zerbini, M, Zhang, W, Zhou, Y, Zlobinski, M, Zocco, A, Zohar, A, Zoita, V, Zoletnik, S, Zotta, V, Zoulias, I, Zwingmann, W, Zychor, I, Mazzi S., Garcia J., Zarzoso D., Kazakov Y. O., Ongena J., Dreval M., Nocente M., Stancar Z., Szepesi G., Eriksson J., Sahlberg A., Benkadda S., Abid N., Abraham K., Abreu P., Adabonyan O., Adrich P., Afzal M., Ahlgren T., Aho-Mantila L., Aiba N., Airila M., Akhtar M., Albanese R., Alderson-Martin M., Alegre D., Aleiferis S., Aleksa A., Alessi E., Aleynikov P., Algualcil J., Ali M., Allinson M., Alper B., Alves E., Ambrosino G., Ambrosino R., Andersson Sunden E., Andrew P., Angelini B. M., Angioni C., Antoniou I., Appel L. C., Appelbee C., Aria S., Ariola M., Artaserse G., Arter W., Artigues V., Asakura N., Ash A., Ashikawa N., Aslanyan V., Astrain M., Asztalos O., Auld D., Auriemma F., Austin Y., Avotina L., Aymerich E., Baciero A., Bairaktaris F., Balbin J., Balbinot L., Balboa I., Balden M., Balshaw C., Balshaw N., Bandaru V. K., Banks J., Baranov Y. F., Barcellona C., Barnard A., Barnard M., Barnsley R., Barth A., Baruzzo M., Barwell S., Bassan M., Batista A., Batistoni P., Baumane L., Bauvir B., Baylor L., Beaumont P. S., Beckett D., Begolli A., Beidler M., Bekris N., Beldishevski M., Belli E., Belli F., Belonohy E., Ben Yaala M., Benayas J., Bentley J., Bergsaker H., Bernardo J., Bernert M., Berry M., Bertalot L., Betar H., Beurskens M., Bickerton S., Bieg B., Bielecki J., Bierwage A., Biewer T., Bilato R., Bilkova P., Birkenmeier G., Bishop H., Bizarro J. P. S., Blackburn J., Blanchard P., Blatchford P., Bobkov V., Boboc A., Bohm P., Bohm T., Bolshakova I., Bolzonella T., Bonanomi N., Bonfiglio D., Bonnin X., Bonofiglo P., Boocock S., Booth A., Booth J., Borba D., Borodin D., Borodkina I., Boulbe C., Bourdelle C., Bowden M., Boyd K., Bozicevic Mihalic I., Bradnam S. C., Braic V., Brandt L., Bravanec R., Breizman B., Brett A., Brezinsek S., Brix M., Bromley K., Brown B., Brunetti D., Buckingham R., Buckley M., Budny R., Buermans J., Bufferand H., Buratti P., Burgess A., Buscarino A., Busse A., Butcher D., de la Cal E., Calabro G., Calacci L., Calado R., Camenen Y., Canal G., Cannas B., Cappelli M., Carcangiu S., Card P., Cardinali A., Carman P., Carnevale D., Carr M., Carralero D., Carraro L., Carvalho I. S., Carvalho P., Casiraghi I., Casson F. J., Castaldo C., Catalan J. P., Catarino N., Causa F., Cavedon M., Cecconello M., Challis C. D., Chamberlain B., Chang C. S., Chankin A., Chapman B., Chernyshova M., Chiariello A., Chmielewski P., Chomiczewska A., Chone L., Ciraolo G., Ciric D., Citrin J., Ciupinski L., Clark M., Clarkson R., Clements C., Cleverly M., Coad J. P., Coates P., Cobalt A., Coccorese V., Coelho R., Coenen J. W., Coffey I. H., Colangeli A., Colas L., Collins C., Collins J., Collins S., Conka D., Conroy S., Conway B., Conway N. J., Coombs D., Cooper P., Cooper S., Corradino C., Corrigan G., Coster D., Cox P., Craciunescu T., Cramp S., Crapper C., Craven D., Craven R., Crialesi Esposito M., Croci G., Croft D., Croitoru A., Crombe K., Cronin T., Cruz N., Crystal C., Cseh G., Cufar A., Cullen A., Curuia M., Czarski T., Dabirikhah H., Molin A. D., Dale E., Dalgliesh P., Dalley S., Dankowski J., David P., Davies A., Davies S., Davis G., Dawson K., Dawson S., Day I. E., De Bock M., De Temmerman G., De Tommasi G., Deakin K., Deane J., Dejarnac R., Del Sarto D., Delabie E., Del-Castillo-Negrete D., Dempsey A., Dendy R. O., Devynck P., Di Siena A., Di Troia C., Dickson T., Dinca P., Dittmar T., Dobrashian J., Doerner R. P., Donne A. J. H., Dorling S., Dormido-Canto S., Douai D., Dowson S., Doyle R., Drewelow P., Drews P., Drummond G., Duckworth P., Dudding H., Dumont R., Dumortier P., Dunai D., Dunatov T., Dunne M., Duran I., Durodie F., Dux R., Dvornova A., Eastham R., Edwards J., Eich T., Eichorn A., Eidietis N., Eksaeva A., El Haroun H., Ellwood G., Elsmore C., Embreus O., Emery S., Ericsson G., Eriksson B., Eriksson F., Eriksson L. G., Ertmer S., Esquembri S., Esquisabel A. L., Estrada T., Evans G., Evans S., Fable E., Fagan D., Faitsch M., Falessi M., Fanni A., Farahani A., Farquhar I., Fasoli A., Faugeras B., Fazinic S., Felici F., Felton R., Fernandes A., Fernandes H., Ferrand J., Ferreira D. R., Ferreira J., Ferro G., Fessey J., Ficker O., Field A. R., Figueiredo A., Figueiredo J., Fil A., Fil N., Finburg P., Fiorucci D., Fischer U., Fishpool G., Fittill L., Fitzgerald M., Flammini D., Flanagan J., Flinders K., Foley S., Fonnesu N., Fontana M., Fontdecaba J. M., Forbes S., Formisano A., Fornal T., Fortuna L., Fortuna-Zalesna E., Fortune M., Fowler C., Fransson E., Frassinetti L., Freisinger M., Fresa R., Fridstrom R., Frigione D., Fulop T., Furseman M., Fusco V., Futatani S., Gadariya D., Gal K., Galassi D., Galazka K., Galeani S., Gallart D., Galvao R., Gao Y., Garcia-Munoz M., Gardener M., Garzotti L., Gaspar J., Gatto R., Gaudio P., Gear D., Gebhart T., Gee S., Gelfusa M., George R., Gerasimov S. N., Gervasini G., Gethins M., Ghani Z., Gherendi M., Ghezzi F., Giacalone J. C., Giacomelli L., Giacometti G., Gibson C., Gibson K. J., Gil L., Gillgren A., Giovannozzi E., Giroud C., Glen R., Gloggler S., Goff J., Gohil P., Goloborodko V., Gomes R., Goncalves B., Goniche M., Goodyear A., Gore S., Gorini G., Gorler T., Gotts N., Goulding R., Gow E., Graham B., Graves J. P., Greuner H., Grierson B., Griffiths J., Griph S., Grist D., Gromelski W., Groth M., Grove R., Gruca M., Guard D., Gupta N., Gurl C., Gusarov A., Hackett L., Hacquin S., Hager R., Hagg L., Hakola A., Halitovs M., Hall S., Hall S. A., Hallworth-Cook S., Ham C. J., Hamaguchi D., Hamed M., Hamlyn-Harris C., Hammond K., Harford E., Harrison J. R., Harting D., Hatano Y., Hatch D. R., Haupt T., Hawes J., Hawkes N. C., Hawkins J., Hayashi T., Hazael S., Hazel S., Heesterman P., Heidbrink B., Helou W., Hemming O., Henderson S. S., Henriques R. B., Hepple D., Herfindal J., Hermon G., Hill J., Hillesheim J. C., Hizanidis K., Hjalmarsson A., Ho A., Hobirk J., Hoenen O., Hogben C., Hollingsworth A., Hollis S., Hollmann E., Holzl M., Homan B., Hook M., Hopley D., Horacek J., Horsley D., Horsten N., Horton A., Horton L. D., Horvath L., Hotchin S., Howell R., Hu Z., Huber A., Huber V., Huddleston T., Huijsmans G. T. A., Huynh P., Hynes A., Imrie D., Imrisek M., Ingleby J., Innocente P., Insulander Bjork K., Isernia N., Ivanova-Stanik I., Ivings E., Jablonski S., Jachmich S., Jackson T., Jacquet P., Jarleblad H., Jaulmes F., Rodriguez J. J., Jepu I., Joffrin E., Johnson R., Johnson T., Johnston J., Jones C., Jones G., Jones L., Jones N., Jones T., Joyce A., Juarez R., Juvonen M., Kalnina P., Kaltiaisenaho T., Kaniewski J., Kantor A., Kappatou A., Karhunen J., Karkinsky D., Kaufman M., Kaveney G., Kazantzidis V., Keeling D. L., Kelly R., Kempenaars M., Kennedy C., Kennedy D., Kent J., Khan K., Kiefer C., Kilpelainen J., Kim C., Kim H. -T., Kim S. H., King D. B., King R., Kinna D., Kiptily V. G., Kirjasuo A., Kirov K. K., Kirschner A., Kiviniemi T., Kizane G., Klas M., Klepper C., Klix A., Kneale G., Knight M., Knight P., Knights R., Knipe S., Knolker M., Knott S., Kocan M., Kochl F., Kodeli I., Kolesnichenko Y., Kominis Y., Kong M., Korovin V., Kos B., Kos D., Koslowski H. R., Kotschenreuther M., Koubiti M., Kowalska-Strzeciwilk E., Koziol K., Krasilnikov V., Kresina M., Krieger K., Krishnan N., Krivska A., Kruezi U., Ksiazek I., Kukushkin A. B., Kumpulainen H., Kurki-Suonio T., Kurotaki H., Kwak S., Kwon O. J., Laguardia L., Lagzdina E., Lahtinen A., Laing A., Lam N., Lambertz H. T., Lane B., Lane C., Lascas Neto E., Laszynska E., Lawson K. D., Lazaros A., Lazzaro E., Learoyd G., Lee C., Lee S. E., Leerink S., Leeson T., Lefebvre X., Leggate H. J., Lehmann J., Lehnen M., Leichtle D., Leipold F., Lengar I., Lennholm M., Leon Gutierrez E., Lepiavko B., Leppanen J., Lerche E., Lescinskis A., Lewis J., Leysen W., Li L., Li Y., Likonen J., Linsmeier C., Lipschultz B., Litaudon X., Litherland-Smith E., Liu F., Loarer T., Loarte A., Lobel R., Lomanowski B., Lomas P. J., Lopez J. M., Lorenzini R., Loreti S., Losada U., Loschiavo V. P., Loughlin M., Louka Z., Lovell J., Lowe T., Lowry C., Lubbad S., Luce T., Lucock R., Luna C., de la Luna E., Lungaroni M., Lungu C. P., Lunt T., Lutsenko V., Lyons B., Lyssoivan A., Machielsen M., Macusova E., Maenpaa R., Maggi C. F., Maggiora R., Magness M., Mahesan S., Maier H., Mailloux J., Maingi R., Malinowski K., Manas P., Mantica P., Mantsinen M. J., Manyer J., Manzanares A., Maquet P., Marceca G., Marchetto C., Marchuk O., Mariani A., Mariano G., Marin M., Marinelli M., Markovic T., Marocco D., Marot L., Marsden S., Marsh J., Marshall R., Martellucci L., Martin A., Martin A. J., Martone R., Maruyama S., Maslov M., Masuzaki S., Matejcik S., Mattei M., Matthews G. F., Matveev D., Matveeva E., Mauriya A., Maviglia F., Mayer M., Mayoral M. -L., Mazzotta C., McAdams R., McCarthy P. J., McClements K. G., McClenaghan J., McCullen P., McDonald D. C., McGuckin D., McHugh D., McIntyre G., McKean R., McKehon J., McMillan B., McNamee L., McShee A., Meakins A., Medley S., Meekes C. 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R., Kotschenreuther M., Koubiti M., Kowalska-Strzeciwilk E., Koziol K., Krasilnikov V., Kresina M., Krieger K., Krishnan N., Krivska A., Kruezi U., Ksiazek I., Kukushkin A. B., Kumpulainen H., Kurki-Suonio T., Kurotaki H., Kwak S., Kwon O. J., Laguardia L., Lagzdina E., Lahtinen A., Laing A., Lam N., Lambertz H. T., Lane B., Lane C., Lascas Neto E., Laszynska E., Lawson K. D., Lazaros A., Lazzaro E., Learoyd G., Lee C., Lee S. E., Leerink S., Leeson T., Lefebvre X., Leggate H. J., Lehmann J., Lehnen M., Leichtle D., Leipold F., Lengar I., Lennholm M., Leon Gutierrez E., Lepiavko B., Leppanen J., Lerche E., Lescinskis A., Lewis J., Leysen W., Li L., Li Y., Likonen J., Linsmeier C., Lipschultz B., Litaudon X., Litherland-Smith E., Liu F., Loarer T., Loarte A., Lobel R., Lomanowski B., Lomas P. J., Lopez J. M., Lorenzini R., Loreti S., Losada U., Loschiavo V. P., Loughlin M., Louka Z., Lovell J., Lowe T., Lowry C., Lubbad S., Luce T., Lucock R., Luna C., de la Luna E., Lungaroni M., Lungu C. P., Lunt T., Lutsenko V., Lyons B., Lyssoivan A., Machielsen M., Macusova E., Maenpaa R., Maggi C. F., Maggiora R., Magness M., Mahesan S., Maier H., Mailloux J., Maingi R., Malinowski K., Manas P., Mantica P., Mantsinen M. J., Manyer J., Manzanares A., Maquet P., Marceca G., Marchetto C., Marchuk O., Mariani A., Mariano G., Marin M., Marinelli M., Markovic T., Marocco D., Marot L., Marsden S., Marsh J., Marshall R., Martellucci L., Martin A., Martin A. J., Martone R., Maruyama S., Maslov M., Masuzaki S., Matejcik S., Mattei M., Matthews G. F., Matveev D., Matveeva E., Mauriya A., Maviglia F., Mayer M., Mayoral M. -L., Mazzotta C., McAdams R., McCarthy P. J., McClements K. G., McClenaghan J., McCullen P., McDonald D. C., McGuckin D., McHugh D., McIntyre G., McKean R., McKehon J., McMillan B., McNamee L., McShee A., Meakins A., Medley S., Meekes C. J., Meghani K., Meigs A. G., Meisl G., Meitner S., Menmuir S., Mergia K., Merriman S., Mertens P., Messiaen A., Michling R., Middleton P., Middleton-Gear D., Mietelski J., Milanesio D., Milani E., Militello F., Militello Asp A., Milnes J., Milocco A., Miloshevsky G., Minghao C., Minucci S., Miron I., Miyamoto M., Mlynar J., Moiseenko V., Monaghan P., Monakhov I., Moody T., Moon S., Mooney R., Moradi S., Morales J., Morales R. B., Mordijck S., Moreira L., Morgan L., Moro F., Morris J., Morrison K. -M., Moser L., Moulton D., Mrowetz T., Mundy T., Muraglia M., Murari A., Muraro A., Muthusonai N., N'Konga B., Na Y. -S., Nabais F., Naden M., Naish J., Naish R., Napoli F., Nardon E., Naulin V., Nave M. F. F., Nedzelskiy I., Nestoras I., Neu R., Ng S., Nicassio M., Nielsen A. H., Nina D., Nishijima D., Noble C., Nobs C. R., Nodwell D., Nordlund K., Nordman H., Normanton R., Noterdaeme J. -M., Nowak S., Nunn E., Nystrom H., Oberparleiter M., Obryk B., O'Callaghan J., Odupitan T., Oliver H. J. C., Olney R., O'Mullane M., Organ E., Orsitto F., Orszagh J., Osborne T., Otin R., Otsuka T., Owen A., Oya Y., Oyaizu M., Paccagnella R., Pace N., Packer L. W., Paige S., Pajuste E., Palade D., Pamela S. J. P., Panadero N., Panontin E., Papadopoulos A., Papp G., Papp P., Parail V. V., Pardanaud C., Parisi J., Parra Diaz F., Parsloe A., Parsons M., Parsons N., Passeri M., Patel A., Pau A., Pautasso G., Pavlichenko R., Pavone A., Pawelec E., Soldan C. P., Peacock A., Pearce M., Peluso E., Penot C., Pepperell K., Pereira R., Pereira T., Cippo E. P., Pereslavtsev P., von Thun C. P., Pericoli V., Perry D., Peterka M., Petersson P., Petravich G., Petrella N., Peyman M., Pillon M., Pinches S., Pintsuk G., de Sa W. P., dos Reis A. P., Piron C., Piron L., Pironti A., Pitts R., van de Plassche K. L., Platt N., Plyusnin V., Podesta M., Pokol G., Poli F. M., Pompilian O. G., Popovichev S., Poradzinski M., Porfiri M. T., Porkolab M., Porosnicu C., Porton M., Poulipoulis G., Predebon I., Prestopino G., Price C., Price D., Price M., Primetzhofer D., Prior P., Provatas G., Pucella G., Puglia P., Purahoo K., Pusztai I., Putignano O., Putterich T., Quercia A., Rachlew E., Radulescu G., Radulovic V., Rainford M., Raj P., Ralph G., Ramogida G., Rasmussen D., Rasmussen J. J., Ratta G., Ratynskaia S., Rebai M., Refy D., Reichle R., Reinke M., Reiser D., Reux C., Reynolds S., Richiusa M. L., Richyal S., Rigamonti D., Rimini F. G., Risner J., Riva M., Rivero-Rodriguez J., Roach C. M., Robins R., Robinson S., Robson D., Rodrigues P., Rodriguez Ramos M., Rodriguez-Fernandez P., Romanelli F., Romanelli M., Romanelli S., Romazanov J., Rossi R., Rowe S., Rowlands D., Rubel M., Rubinacci G., Rubino G., Ruchko L., Ruiz M., Ruiz J. 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C., Willoughby D., Wilson I., Wilson J., Wilson T., Wischmeier M., Wise P., Withenshaw G., Withycombe A., Witts D., Wojcik-Gargula A., Wolfrum E., Wood R., Woodley C., Woodley R., Woods B., Wright J., Wright J. C., Xu T., Yadikin D., Yajima M., Yakovenko Y., Yang Y., Yanling W., Yanovskiy V., Young I., Young R., Zabolockis R. J., Zacks J., Zagorski R., Zaitsev F. S., Zakharov L., Zarins A., Zastrow K. -D., Zayachuk Y., Zerbini M., Zhang W., Zhou Y., Zlobinski M., Zocco A., Zohar A., Zoita V., Zoletnik S., Zotta V. K., Zoulias I., Zwingmann W., and Zychor I.

Abstract

Alpha particles with energies on the order of megaelectronvolts will be the main source of plasma heating in future magnetic confinement fusion reactors. Instead of heating fuel ions, most of the energy of alpha particles is transferred to electrons in the plasma. Furthermore, alpha particles can also excite Alfvénic instabilities, which were previously considered to be detrimental to the performance of the fusion device. Here we report improved thermal ion confinement in the presence of megaelectronvolts ions and strong fast ion-driven Alfvénic instabilities in recent experiments on the Joint European Torus. Detailed transport analysis of these experiments reveals turbulence suppression through a complex multi-scale mechanism that generates large-scale zonal flows. This holds promise for more economical operation of fusion reactors with dominant alpha particle heating and ultimately cheaper fusion electricity.

Published
2022

40. Langmuir probe measurements in a magnetized capacitive discharge around a tilted RF electrode.

Author

Cherukulappurath, A., Faudot, E., Brochard, F., Heuraux, S., Hiret, P., Marot, L., Soni, K., and Moser, L.

Subjects
LANGMUIR probes, HEAT flux measurement, ELECTRODES, HOT carriers, CURRENT-voltage curves
Abstract

Applications of magnetized Radio Frequency (RF) capacitive discharges for mirror cleaning applications of optical diagnostic systems in fusion devices and heat flux measurements have received a large interest in last years. Ensuring the ho-mogeneity of heat flux to the RF electrode requires localized measurements of plasma parameters in front of the RF electrode. Langmuir probe measurements were taken in the ALINE plasma device around the active RF electrode with the help of a 3D manipulator equipped with RF compensation. Highly negative floating potential values were recorded inside the magnetic flux tube connected to the active RF electrode whilst plasma potential remained positive. Since the difference between the plasma po-tential and the floating potential is proportional to the average electron temperature, experimental investigations were carried out in capacitive coupling and direct coupling to study the change in floating potential as a function of input gas pressure, magnetic field strength (B), and the angle between the RF electrode and magnetic field. The observed change in floating potential is attributed to the stochastic heating leading to the generation of hot electrons, which was confirmed using the Langmuir probe current-voltage curves. The experimental results are found to agree with the analytical model based on the flux balance equations. [ABSTRACT FROM AUTHOR]

Published
2023
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42. Decentralized Mobile Search and Retrieval Using SMS and HTTP to Support Social Change

Author

Michel Lombera, Isaí, Chuang, Yung-Ting, Moser, L. E., Melliar-Smith, P. M., Akan, Ozgur, Series editor, Bellavista, Paolo, Series editor, Cao, Jiannong, Series editor, Dressler, Falko, Series editor, Ferrari, Domenico, Series editor, Gerla, Mario, Series editor, Kobayashi, Hisashi, Series editor, Palazzo, Sergio, Series editor, Sahni, Sartaj, Series editor, Shen, Xuemin (Sherman), Series editor, Stan, Mircea, Series editor, Xiaohua, Jia, Series editor, Zomaya, Albert, Series editor, Coulson, Geoffrey, Series editor, Zhang, Joy Ying, editor, Wilkiewicz, Jarek, editor, and Nahapetian, Ani, editor

Published
2012
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43. Disruption prediction with artificial intelligence techniques in tokamak plasmas

Author

Vega, J., Murari, A., Dormido-Canto, S., Rattá, G. A., Gelfusa, M., Mailloux, J., Abid, N., Abraham, K., Abreu, P., Adabonyan, O., Adrich, P., Afanasev, V., Afzal, M., Ahlgren, T., Aho-Mantila, L., Aiba, N., Airila, M., Akhtar, M., Albanese, R., Alderson-Martin, M., Alegre, D., Aleiferis, S., Aleksa, A., Alekseev, A. G., Alessi, E., Aleynikov, P., Algualcil, J., Ali, M., Allinson, M., Alper, B., Alves, E., Ambrosino, G., Ambrosino, R., Amosov, V., Andersson Sundén, E., Andrew, P., Angelini, B. M., Angioni, C., Antoniou, I., Appel, L. C., Appelbee, C., Aria, S., Ariola, M., Artaserse, G., Arter, W., Artigues, V., Asakura, N., Ash, A., Ashikawa, N., Aslanyan, V., Astrain, M., Asztalos, O., Auld, D., Auriemma, F., Austin, Y., Avotina, L., Aymerich, E., Baciero, A., Bairaktaris, F., Balbin, J., Balbinot, L., Balboa, I., Balden, M., Balshaw, C., Balshaw, N., Bandaru, V. K., Banks, J., Baranov, Yu. F., Barcellona, C., Barnard, A., Barnard, M., Barnsley, R., Barth, A., Baruzzo, M., Barwell, S., Bassan, M., Batista, A., Batistoni, P., Baumane, L., Bauvir, B., Baylor, L., Beaumont, P. S., Beckett, D., Begolli, A., Beidler, M., Bekris, N., Beldishevski, M., Belli, E., Belli, F., Belonohy, É., Ben Yaala, M., Benayas, J., Bentley, J., Bergsaker, H., Bernardo, J., Bernert, M., Berry, M., Bertalot, L., Betar, H., Beurskens, M., Bickerton, S., Bieg, B., Bielecki, J., Bierwage, A., Biewer, T., Bilato, R., Bílková, P., Birkenmeier, G., Bishop, H., Bizarro, J. P. S., Blackburn, J., Blanchard, P., Blatchford, P., Bobkov, V., Boboc, A., Bohm, P., Bohm, T., Bolshakova, I., Bolzonella, T., Bonanomi, N., Bonfiglio, D., Bonnin, X., Bonofiglo, P., Boocock, S., Booth, A., Booth, J., Borba, D., Borodin, D., Borodkina, I., Boulbe, C., Bourdelle, C., Bowden, M., Boyd, K., Božičević Mihalić, I., Bradnam, S. C., Braic, V., Brandt, L., Bravanec, R., Breizman, B., Brett, A., Brezinsek, S., Brix, M., Bromley, K., Brown, B., Brunetti, D., Buckingham, R., Buckley, M., Budny, R., Buermans, J., Bufferand, H., Buratti, P., Burgess, A., Buscarino, A., Busse, A., Butcher, D., de la Cal, E., Calabro, G., Calacci, L., Calado, R., Camenen, Y., Canal, G., Cannas, B., Cappelli, M., Carcangiu, S., Card, P., Cardinali, A., Carman, P., Carnevale, D., Carr, M., Carralero, D., Carraro, L., Carvalho, I. S., Carvalho, P., Casiraghi, I., Casson, F. J., Castaldo, C., Catalan, J. P., Catarino, N., Causa, F., Cavedon, M., Cecconello, M., Challis, C. D., Chamberlain, B., Chang, C. S., Chankin, A., Chapman, B., Chernyshova, M., Chiariello, A., Chmielewski, P., Chomiczewska, A., Chone, L., Ciraolo, G., Ciric, D., Citrin, J., Ciupinski, T., Clark, M., Clarkson, R., Clements, C., Cleverly, M., Coad, J. P., Coates, P., Cobalt, A., Coccorese, V., Coelho, R., Coenen, J. W., Coffey, I. H., Colangeli, A., Colas, L., Collins, C., Collins, J., Collins, S., Conka, D., Conroy, S., Conway, B., Conway, N. J., Coombs, D., Cooper, P., Cooper, S., Corradino, C., Corrigan, G., Coster, D., Cox, P., Craciunescu, T., Cramp, S., Crapper, C., Craven, D., Craven, R., Crialesi Esposito, M., Croci, G., Croft, D., Croitoru, A., Crombé, K., Cronin, T., Cruz, N., Crystal, C., Cseh, G., Cufar, A., Cullen, A., Curuia, M., Czarski, T., Dabirikhah, H., Dal Molin, A., Dale, E., Dalgliesh, P., Dalley, S., Dankowski, J., David, P., Davies, A., Davies, S., Davis, G., Dawson, K., Dawson, S., Day, I. E., De Bock, M., De Temmerman, G., De Tommasi, G., Deakin, K., Deane, J., Dejarnac, R., Del Sarto, D., Delabie, E., Del-Castillo-Negrete, D., Dempsey, A., Dendy, R. O., Devynck, P., Di Siena, A., Di Troia, C., Dickson, T., Dinca, P., Dittmar, T., Dobrashian, J., Doerner, R. P., Donné, A. J. H., Dorling, S., Douai, D., Dowson, S., Doyle, R., Dreval, M., Drewelow, P., Drews, P., Drummond, G., Duckworth, Ph., Dudding, H., Dumont, R., Dumortier, P., Dunai, D., Dunatov, T., Dunne, M., Duran, I., Durodié, F., Dux, R., Dvornova, A., Eastham, R., Edwards, J., Eich, Th., Eichorn, A., Eidietis, N., Eksaeva, A., El Haroun, H., Ellwood, G., Elsmore, C., Embreus, O., Emery, S., Ericsson, G., Eriksson, B., Eriksson, F., Eriksson, J., Eriksson, L. G., Ertmer, S., Esquembri, S., Esquisabel, A. L., Estrada, T., Evans, G., Evans, S., Fable, E., Fagan, D., Faitsch, M., Falessi, M., Fanni, A., Farahani, A., Farquhar, I., Fasoli, A., Faugeras, B., Fazinié, S., Felici, F., Felton, R., Fernandes, A., Fernandes, H., Ferrand, J., Ferreira, D. R., Ferreira, J., Ferro, G., Fessey, J., Ficker, O., Field, A. 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L., Kelly, R., Kempenaars, M., Kennedy, C., Kennedy, D., Kent, J., Khan, K., Khilkevich, E., Kiefer, C., Kilpeläinen, J., Kim, C., Hyun-Tae, Kim, Kim, S. H., King, D. B., King, R., Kinna, D., Kiptily, V. G., Kirjasuo, A., Kirov, K. K., Kirschner, A., Kiviniemi, T., Kizane, G., Klas, M., Klepper, C., Klix, A., Kneale, G., Knight, M., Knight, P., Knights, R., Knipe, S., Knolker, M., Knott, S., Kocan, M., Kochl, F., Kodeli, I., Kolesnichenko, Y., Kominis, Y., Kong, M., Korovin, V., Kos, B., Kos, D., Koslowski, H. R., Kotschenreuther, M., Koubiti, M., Kowalska-Strzęciwilk, E., Koziol, K., Krasilnikov, A., Krasilnikov, V., Kresina, M., Krieger, K., Krishnan, N., Krivska, A., Kruezi, U., Ksiézek, I., Kukushkin, A. B., Kumpulainen, H., Kurki-Suonio, T., Kurotaki, H., Kwak, S., Kwon, O. J., Laguardia, L., Lagzdina, E., Lahtinen, A., Laing, A., Lam, N., Lambertz, H. T., Lane, B., Lane, C., Lascas Neto, E., Łaszyríska, E., Lawson, K. D., Lazaros, A., Lazzaro, E., Learoyd, G., Chanyoung, Lee, Lee, S. E., Leerink, S., Leeson, T., Lefebvre, X., Leggate, H. J., Lehmann, J., Lehnen, M., Leichtle, D., Leipold, F., Lengar, I., Lennholm, M., Leon Gutierrez, E., Lepiavko, B., Leppanen, J., Lerche, E., Lescinskis, A., Lewis, J., Leysen, W., Li, L., Li, Y., Likonen, J., Linsmeier, Ch., Lipschultz, B., Litaudon, X., Litherland-Smith, E., Liu, F., Loarer, T., Loarte, A., Lobel, R., Lomanowski, B., Lomas, P. J., López, J. M., Lorenzini, R., Loreti, S., Losada, U., Loschiavo, V. P., Loughlin, M., Louka, Z., Lovell, J., Lowe, T., Lowry, C., Lubbad, S., Luce, T., Lucock, R., Lukin, A., Luna, C., de la Luna, E., Lungaroni, M., Lungu, C. P., Lunt, T., Lutsenko, V., Lyons, B., Lyssoivan, A., Machielsen, M., Macusova, E., Mäenpää, R., Maggi, C. F., Maggiora, R., Magness, M., Mahesan, S., Maier, H., Maingi, R., Malinowski, K., Manas, P., Mantica, P., Mantsinen, M. J., Manyer, J., Manzanares, A., Maquet, Ph., Marceca, G., Marcenko, N., Marchetto, C., Marchuk, O., Mariani, A., Mariano, G., Marin, M., Marinelli, M., Markovič, T., Marocco, D., Marot, L., Marsden, S., Marsh, J., Marshall, R., Martellucci, L., Martin, A., Martin, A. J., Martone, R., Maruyama, S., Maslov, M., Masuzaki, S., Matejcik, S., Mattei, M., Matthews, G. F., Matveev, D., Matveeva, E., Mauriya, A., Maviglia, F., Mayer, M., Mayoral, M-L., Mazzi, S., Mazzotta, C., Mcadams, R., Mccarthy, P. J., Mcclements, K. G., Mcclenaghan, J., Mccullen, P., Mcdonald, D. C., Mcguckin, D., Mchugh, D., Mclntyre, G., Mckean, R., Mckehon, J., Mcmillan, B., Mcnamee, L., Mcshee, A., Meakins, A., Medley, S., Meekes, C. J., Meghani, K., Meigs, A. G., Meisl, G., Meitner, S., Menmuir, S., Mergia, K., Merriman, S., Mertens, Ph., Meshchaninov, S., Messiaen, A., Michling, R., Middleton, P., Middleton-Gear, D., Mietelski, J., Milanesio, D., Milani, E., Militello, F., Militello Asp, A., Milnes, J., Milocco, A., Miloshevsky, G., Minghao, C., Minucci, S., Miron, I., Miyamoto, M., Mlynář, J., Moiseenko, V., Monaghan, P., Monakhov, I., Moody, T., Moon, S., Mooney, R., Moradi, S., Morales, J., Morales, R. B., Mordijck, S., Moreira, L., Morgan, L., Moro, F., Morris, J., Morrison, K-M., Moser, L., Moulton, D., Mrowetz, T., Mundy, T., Muraglia, M., Muraro, A., Muthusonai, N., N’Konga, B., Yong-Su, Na, Nabais, F., Naden, M., Naish, J., Naish, R., Napoli, F., Nardon, E., Naulin, V., Nave, M. F. F., Nedzelskiy, I., Nemtsev, G., Nesenevich, V., Nestoras, I., Neu, R., Neverov, V. S., Ng, S., Nicassio, M., Nielsen, A. H., Nina, D., Nishijima, D., Noble, C., Nobs, C. R., Nocente, M., Nodwell, D., Nordlund, K., Nordman, H., Normanton, R., Noterdaeme, J. M., Nowak, S., Nunn, E., Nystrom, H., Oberparleiter, M., Obryk, B., O’Callaghan, J., Odupitan, T., Oliver, H. J. C., Olney, R., O’Mullane, M., Ongena, J., Organ, E., Orsitto, F., Orszagh, J., Osborne, T., Otin, R., Otsuka, T., Owen, A., Oya, Y., Oyaizu, M., Paccagnella, R., Pace, N., Packer, L. W., Paige, S., Pajuste, E., Palade, D., Pamela, S. J. P., Panadero, N., Panontin, E., Papadopoulos, A., Papp, G., Papp, P., Parail, V. V., Pardanaud, C., Parisi, J., Parra Diaz, F., Parsloe, A., Parsons, M., Parsons, N., Passeri, M., Patel, A., Pau, A., Pautasso, G., Pavlichenko, R., Pavone, A., Pawelec, E., Paz Soldan, C., Peacock, A., Pearce, M., Peluso, E., Penot, C., Pepperell, K., Pereira, R., Pereira, T., Perelli Cippo, E., Pereslavtsev, P., Perez von Thun, C., Pericoli, V., Perry, D., Peterka, M., Petersson, P., Petravich, G., Petrella, N., Peyman, M., Pillon, M., Pinches, S., Pintsuk, G., Pires de Sá, W., Pires dos Reis, A., Piron, C., Piron, L., Pironti, A., Pitts, R., van de Plassche, K. L., Platt, N., Plyusnin, V., Podesta, M., Pokol, G., Poli, F. M., Pompilian, O. G., Popovichev, S., Poradziński, M., Porfiri, M. T., Porkolab, M., Porosnicu, C., Porton, M., Poulipoulis, G., Predebon, I., Prestopino, G., Price, C., Price, D., Price, M., Primetzhofer, D., Prior, P., Provatas, G., Pucella, G., Puglia, P., Purahoo, K., Pusztai, I., Putignano, O., Pütterich, T., Quercia, A., Rachlew, E., Radulescu, G., Radulovic, V., Rainford, M., Raj, P., Ralph, G., Ramogida, G., Rasmussen, D., Rasmussen, J. J., Rattá, G., Ratynskaia, S., Rebai, M., Réfy, D., Reichle, R., Reinke, M., Reiser, D., Reux, C., Reynolds, S., Richiusa, M. L., Richyal, S., Rigamonti, D., Rimini, F. G., Risner, J., Riva, M., Rivero-Rodriguez, J., Roach, C. M., Robins, R., Robinson, S., Robson, D., Rodionov, R., Rodrigues, P., Rodriguez Ramos, M., Rodriguez-Fernandez, P., Romanelli, F., Romanelli, M., Romanelli, S., Romazanov, J., Rossi, R., Rowe, S., Rowlands, D., Rubel, M., Rubinacci, G., Rubino, G., Ruchko, L., Ruiz, M., Ruiz Ruiz, J., Ruset, C., Rzadkiewicz, J., Saarelma, S., Safi, E., Sahlberg, A., Salewski, M., Salmi, A., Salmon, R., Salzedas, F., Sanders, I., Sandiford, D., Santos, B., Santucci, A., Sarkimaki, K., Sarwar, R., Sarychev, I., Sauter, O., Sauwan, P., Scapin, N., Schluck, F., Schmid, K., Schmuck, S., Schneider, M., Schneider, P. A., Schworer, D., Scott, G., Scott, M., Scraggs, D., Scully, S., Segato, M., Jaemin, Seo, Sergienko, G., Sertoli, M., Sharapov, S. E., Shaw, A., Sheikh, H., Sheikh, U., Shepherd, A., Shevelev, A., Shigin, P., Shinohara, K., Shiraiwa, S., Shiraki, D., Short, M., Sias, G., Silburn, S. A., Silva, A., Silva, C., Silva, J., Silvagni, D., Simfukwe, D., Simpson, J., Sinclair, D., Sipilä, S. K., Sips, A. C. C., Sirén, P., Sirinelli, A., Sjöstrand, H., Skinner, N., Slater, J., Smith, N., Smith, P., Snell, J., Snoep, G., Snoj, L., Snyder, P., Soare, S., Solano, E. R., Solokha, V., Somers, A., Sommariva, C., Soni, K., Sorokovoy, E., Sos, M., Sousa, J., Sozzi, C., Spagnolo, S., Spelzini, T., Spineanu, F., Spong, D., Sprada, D., Sridhar, S., Srinivasan, C., Stables, G., Staebler, G., Stamatelatos, I., Stancar, Z., Staniec, P., Stankūnas, G., Stead, M., Stefanikova, E., Stephen, A., Stephens, J., Stevenson, P., Stojanov, M., Strand, P., Strauss, H. R., Strikwerda, S., Ström, P., Stuart, C. I., Studholme, W., Subramani, M., Suchkov, E., Sumida, S., Sun, H. J., Susts, T. E., Svensson, J., Svoboda, J., Sweeney, R., Sytnykov, D., Szabolics, T., Szepesi, G., Tabia, B., Tadić, T., Tál, B., Tala, T., Tallargio, A., Tamain, P., Tan, H., Tanaka, K., Tang, W., Tardocchi, M., Taylor, D., Teimane, A. S., Telesca, G., Teplova, N., Teplukhina, A., Terentyev, D., Terra, A., Terranova, D., Terranova, N., Testa, D., Tholerus, E., Thomas, J., Thoren, E., Thorman, A., Tierens, W., Tinguely, R. A., Tipton, A., Todd, H., Tokitani, M., Tolias, P., Tomes, M., Tookey, A., Torikai, Y., von Toussaint, U., Tsavalas, P., Tskhakaya, D., Turner, I., Turner, M., Turner, M. M., Turnyanskiy, M., Tvalashvili, G., Tyrrell, S., Tyshchenko, M., Uccello, A., Udintsev, V., Urbanczyk, G., Vadgama, A., Valcarcel, D., Valisa, M., Vallejos Olivares, P., Vallhagen, O., Valovič, M., Van Eester, D., Varje, J., Vartanian, S., Vasilopoulou, T., Vayakis, G., Vecsei, M., Ventre, S., Verdoolaege, G., Verona, C., Verona Rinati, G., Veshchev, E., Vianello, N., Viezzer, E., Vignitchouk, L., Vila, R., Villari, R., Villone, F., Vincenzi, P., Vinyar, I., Viola, B., Virtanen, A. J., Vitins, A., Vizvary, Z., Vlad, G., Vlad, M., Vondráček, P., de Vries, P., Wakeling, B., Walkden, N. R., Walker, M., Walker, R., Walsh, M., Wang, E., Wang, N., Warder, S., Warren, R., Waterhouse, J., Watts, C., Wauters, T., Weckmann, A., Wedderburn Maxwell, H., Weiland, M., Weisen, H., Weiszflog, M., Welch, P., Wendler, N., West, A., Wheatley, M., Wheeler, S., Whitehead, A., Whittaker, D., Widdowson, A., Wiesen, S., Wilkinson, J., Williams, J. C., Willoughby, D., Wilson, I., Wilson, J., Wilson, T., Wischmeier, M., Wise, P., Withenshaw, G., Withycombe, A., Witts, D., Wojcik-Gargula, A., Wolfrum, E., Wood, R., Woodley, C., Woodley, R., Woods, B., Wright, J., Wright, J. C., Xu, T., Yadikin, D., Yajima, M., Yakovenko, Y., Yang, Y., Yanling, W., Yanovskiy, V., Young, I., Young, R., Zabolockis, R. J., Zacks, J., Zagorski, R., Zaitsev, F. S., Zakharov, L., Zarins, A., Zarzoso Fernandez, D., Zastrow, K. -D., Zayachuk, Y., Zerbini, M., Zhang, W., Zhou, Y., Zlobinski, M., Zocco, A., Zohar, A., Zoita, V., Zoletnik, S., Zotta, V. K., Zoulias, I., Zwingmann &amp, Zychor, I., Vega, J, Murari, A, Dormido-Canto, S, Ratta, Ga, Gelfusa, M, Chiariello, A, JET Contributors, VTT Technical Research Centre of Finland, Culham Science Centre, Princeton Plasma Physics Laboratory, Department of Applied Physics, Uppsala University, European Commission, Forschungszentrum Jülich, Universidade Lisboa, Fusion and Plasma Physics, University of Milan - Bicocca, University of Helsinki, General Atomics, ITER, University of Toyama, CEA, Oak Ridge National Laboratory, Technical University of Madrid, Swiss Federal Institute of Technology Lausanne, Dutch Institute for Fundamental Energy Research, Royal Military Academy, Seoul National University, Chalmers University of Technology, Max Planck Institute for Plasma Physics, KTH Royal Institute of Technology, Aalto-yliopisto, Aalto University, Science and Technology of Nuclear Fusion, EIRES Eng. for Sustainable Energy Systems, Magneto-Hydro-Dynamic Stability of Fusion Plasmas, Vega, J., Murari, A., Dormido-Canto, S., Ratta, G. A., Gelfusa, M., Mailloux, J., Abid, N., Abraham, K., Abreu, P., Adabonyan, O., Adrich, P., Afanasev, V., Afzal, M., Ahlgren, T., Aho-Mantila, L., Aiba, N., Airila, M., Akhtar, M., Albanese, R., Alderson-Martin, M., Alegre, D., Aleiferis, S., Aleksa, A., Alekseev, A. G., Alessi, E., Aleynikov, P., Algualcil, J., Ali, M., Allinson, M., Alper, B., Alves, E., Ambrosino, G., Ambrosino, R., Amosov, V., Sunden, E. A., Andrew, P., Angelini, B. M., Angioni, C., Antoniou, I., Appel, L. C., Appelbee, C., Aria, S., Ariola, M., Artaserse, G., Arter, W., Artigues, V., Asakura, N., Ash, A., Ashikawa, N., Aslanyan, V., Astrain, M., Asztalos, O., Auld, D., Auriemma, F., Austin, Y., Avotina, L., Aymerich, E., Baciero, A., Bairaktaris, F., Balbin, J., Balbinot, L., Balboa, I., Balden, M., Balshaw, C., Balshaw, N., Bandaru, V. K., Banks, J., Baranov, Y. F., Barcellona, C., Barnard, A., Barnard, M., Barnsley, R., Barth, A., Baruzzo, M., Barwell, S., Bassan, M., Batista, A., Batistoni, P., Baumane, L., Bauvir, B., Baylor, L., Beaumont, P. S., Beckett, D., Begolli, A., Beidler, M., Bekris, N., Beldishevski, M., Belli, E., Belli, F., Belonohy, E., Yaala, M. B., Benayas, J., Bentley, J., Bergsaker, H., Bernardo, J., Bernert, M., Berry, M., Bertalot, L., Betar, H., Beurskens, M., Bickerton, S., Bieg, B., Bielecki, J., Bierwage, A., Biewer, T., Bilato, R., Bilkova, P., Birkenmeier, G., Bishop, H., Bizarro, J. P. S., Blackburn, J., Blanchard, P., Blatchford, P., Bobkov, V., Boboc, A., Bohm, P., Bohm, T., Bolshakova, I., Bolzonella, T., Bonanomi, N., Bonfiglio, D., Bonnin, X., Bonofiglo, P., Boocock, S., Booth, A., Booth, J., Borba, D., Borodin, D., Borodkina, I., Boulbe, C., Bourdelle, C., Bowden, M., Boyd, K., Bozicevic Mihalic, I., Bradnam, S. C., Braic, V., Brandt, L., Bravanec, R., Breizman, B., Brett, A., Brezinsek, S., Brix, M., Bromley, K., Brown, B., Brunetti, D., Buckingham, R., Buckley, M., Budny, R., Buermans, J., Bufferand, H., Buratti, P., Burgess, A., Buscarino, A., Busse, A., Butcher, D., de la Cal, E., Calabro, G., Calacci, L., Calado, R., Camenen, Y., Canal, G., Cannas, B., Cappelli, M., Carcangiu, S., Card, P., Cardinali, A., Carman, P., Carnevale, D., Carr, M., Carralero, D., Carraro, L., Carvalho, I. S., Carvalho, P., Casiraghi, I., Casson, F. J., Castaldo, C., Catalan, J. P., Catarino, N., Causa, F., Cavedon, M., Cecconello, M., Challis, C. D., Chamberlain, B., Chang, C. S., Chankin, A., Chapman, B., Chernyshova, M., Chiariello, A., Chmielewski, P., Chomiczewska, A., Chone, L., Ciraolo, G., Ciric, D., Citrin, J., Ciupinski, T., Clark, M., Clarkson, R., Clements, C., Cleverly, M., Coad, J. P., Coates, P., Cobalt, A., Coccorese, V., Coelho, R., Coenen, J. W., Coffey, I. H., Colangeli, A., Colas, L., Collins, C., Collins, J., Collins, S., Conka, D., Conroy, S., Conway, B., Conway, N. J., Coombs, D., Cooper, P., Cooper, S., Corradino, C., Corrigan, G., Coster, D., Cox, P., Craciunescu, T., Cramp, S., Crapper, C., Craven, D., Craven, R., Esposito, M. C., Croci, G., Croft, D., Croitoru, A., Crombe, K., Cronin, T., Cruz, N., Crystal, C., Cseh, G., Cufar, A., Cullen, A., Curuia, M., Czarski, T., Dabirikhah, H., Dal Molin, A., Dale, E., Dalgliesh, P., Dalley, S., Dankowski, J., David, P., Davies, A., Davies, S., Davis, G., Dawson, K., Dawson, S., Day, I. E., De Bock, M., De Temmerman, G., De Tommasi, G., Deakin, K., Deane, J., Dejarnac, R., Del Sarto, D., Delabie, E., Del-Castillo-Negrete, D., Dempsey, A., Dendy, R. O., Devynck, P., Di Siena, A., Di Troia, C., Dickson, T., Dinca, P., Dittmar, T., Dobrashian, J., Doerner, R. P., Donne, A. J. H., Dorling, S., Douai, D., Dowson, S., Doyle, R., Dreval, M., Drewelow, P., Drews, P., Drummond, G., Duckworth, P., Dudding, H., Dumont, R., Dumortier, P., Dunai, D., Dunatov, T., Dunne, M., Duran, I., Durodie, F., Dux, R., Dvornova, A., Eastham, R., Edwards, J., Eich, T., Eichorn, A., Eidietis, N., Eksaeva, A., El Haroun, H., Ellwood, G., Elsmore, C., Embreus, O., Emery, S., Ericsson, G., Eriksson, B., Eriksson, F., Eriksson, J., Eriksson, L. G., Ertmer, S., Esquembri, S., Esquisabel, A. L., Estrada, T., Evans, G., Evans, S., Fable, E., Fagan, D., Faitsch, M., Falessi, M., Fanni, A., Farahani, A., Farquhar, I., Fasoli, A., Faugeras, B., Fazinie, S., Felici, F., Felton, R., Fernandes, A., Fernandes, H., Ferrand, J., Ferreira, D. R., Ferreira, J., Ferro, G., Fessey, J., Ficker, O., Field, A. R., Figueiredo, A., Figueiredo, J., Fil, A., Fil, N., Finburg, P., Fiorucci, D., Fischer, U., Fishpool, G., Fittill, L., Fitzgerald, M., Flammini, D., Flanagan, J., Flinders, K., Foley, S., Fonnesu, N., Fontana, M., Fontdecaba, J. M., Forbes, S., Formisano, A., Fornal, T., Fortuna, L., Fortuna-Zalesna, E., Fortune, M., Fowler, C., Fransson, E., Frassinetti, L., Freisinger, M., Fresa, R., Fridstrom, R., Frigione, D., Fulop, T., Furseman, M., Fusco, V., Futatani, S., Gadariya, D., Gal, K., Galassi, D., Gafezka, K., Galeani, S., Gallart, D., Galvao, R., Gao, Y., Garcia, J., Garcia-Munoz, M., Gardener, M., Garzotti, L., Gaspar, J., Gatto, R., Gaudio, P., Gear, D., Gebhart, T., Gee, S., George, R., Gerasimov, S. N., Gervasini, G., Gethins, M., Ghani, Z., Gherendi, M., Ghezzi, F., Giacalone, J. C., Giacomelli, L., Giacometti, G., Gibson, C., Gibson, K. J., Gil, L., Gillgren, A., Gin, D., Giovannozzi, E., Giroud, C., Glen, R., Gloggler, S., Goff, J., Gohil, P., Goloborodko, V., Gomes, R., Goncalves, B., Goniche, M., Goodyear, A., Gore, S., Gorini, G., Gorler, T., Gotts, N., Goulding, R., Gow, E., Graham, B., Graves, J. P., Greuner, H., Grierson, B., Griffiths, J., Griph, S., Grist, D., Gromelski, W., Groth, M., Grove, R., Gruca, M., Guard, D., Gupta, N., Gurl, C., Gusarov, A., Hackett, L., Hacquin, S., Hager, R., Hagg, L., Hakola, A., Halitovs, M., Hall, S., Hall, S. A., Hallworth-Cook, S., Ham, C. J., Hamaguchi, D., Hamed, M., Hamlyn-Harris, C., Hammond, K., Harford, E., Harrison, J. R., Harting, D., Hatano, Y., Hatch, D. R., Haupt, T., Hawes, J., Hawkes, N. C., Hawkins, J., Hayashi, T., Hazael, S., Hazel, S., Heesterman, P., Heidbrink, B., Helou, W., Hemming, O., Henderson, S. S., Henriques, R. B., Hepple, D., Herfindal, J., Hermon, G., Hill, J., Hillesheim, J. C., Hizanidis, K., Hjalmarsson, A., Ho, A., Hobirk, J., Hoenen, O., Hogben, C., Hollingsworth, A., Hollis, S., Hollmann, E., Holzl, M., Homan, B., Hook, M., Hopley, D., Hora:ek, J., Horsley, D., Horsten, N., Horton, A., Horton, L. D., Horvath, L., Hotchin, S., Howell, R., Hu, Z., Huber, A., Huber, V., Huddleston, T., Huijsmans, G. T. A., Huynh, P., Hynes, A., Iliasova, M., Lmrie, D., Lmrisek, M., Lngleby, J., Innocente, P., Bjork, K. I., Isernia, N., lvanova-Stanik, I., Lvings, E., Jablonski, S., Jachmich, S., Jackson, T., Jacquet, P., Jarleblad, H., Jaulmes, F., Rodriguez, J. J., Jepu, I., Joffrin, E., Johnson, R., Johnson, T., Johnston, J., Jones, C., Jones, G., Jones, L., Jones, N., Jones, T., Joyce, A., Juarez, R., Juvonen, M., Kalnina, P., Kaltiaisenaho, T., Kaniewski, J., Kantor, A., Kappatou, A., Karhunen, J., Karkinsky, D., Kashchuk, Y., Kaufman, M., Kaveney, G., Kazakov, Y. E. O., Kazantzidis, V., Keeling, D. L., Kelly, R., Kempenaars, M., Kennedy, C., Kennedy, D., Kent, J., Khan, K., Khilkevich, E., Kiefer, C., Kilpelainen, J., Kim, C., Kim, H. -T., Kim, S. H., King, D. B., King, R., Kinna, D., Kiptily, V. G., Kirjasuo, A., Kirov, K. K., Kirschner, A., Kiviniemi, T., Kizane, G., Klas, M., Klepper, C., Klix, A., Kneale, G., Knight, M., Knight, P., Knights, R., Knipe, S., Knolker, M., Knott, S., Kocan, M., Kochl, F., Kodeli, I., Kolesnichenko, Y., Kominis, Y., Kong, M., Korovin, V., Kos, B., Kos, D., Koslowski, H. R., Kotschenreuther, M., Koubiti, M., Kowalska-Strzeciwilk, E., Koziol, K., Krasilnikov, A., Krasilnikov, V., Kresina, M., Krieger, K., Krishnan, N., Krivska, A., Kruezi, U., Ksiezek, I., Kukushkin, A. B., Kumpulainen, H., Kurki-Suonio, T., Kurotaki, H., Kwak, S., Kwon, O. J., Laguardia, L., Lagzdina, E., Lahtinen, A., Laing, A., Lam, N., Lambertz, H. T., Lane, B., Lane, C., Neto, E. L., Laszyriska, E., Lawson, K. D., Lazaros, A., Lazzaro, E., Learoyd, G., Lee, C., Lee, S. 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Subjects
JET, Settore ING-IND/18 - Fisica dei Reattori Nucleari, General Physics and Astronomy, artificial intellingence, tokamaks, magnetically confined plasma, disruption predictions, tokamak plasmas, nuclear fusion
Abstract

openaire: EC/H2020/633053/EU//EUROfusion Funding Information: This work was partially funded by the Spanish Ministry of Science and Innovation under projects nos. PID2019-108377RB-C31 and PID2019-108377RB-C32. This work has been carried out within the framework of the EUROfusion Consortium, funded by the European Union via the Euratom Research and Training Programme (grant agreement no. 101052200 — EUROfusion). Views and opinions expressed are however those of the authors only and do not necessarily reflect those of the European Union or the European Commission. Neither the European Union nor the European Commission can be held responsible for them. Publisher Copyright: © 2022, Springer Nature Limited. In nuclear fusion reactors, plasmas are heated to very high temperatures of more than 100 million kelvin and, in so-called tokamaks, they are confined by magnetic fields in the shape of a torus. Light nuclei, such as deuterium and tritium, undergo a fusion reaction that releases energy, making fusion a promising option for a sustainable and clean energy source. Tokamak plasmas, however, are prone to disruptions as a result of a sudden collapse of the system terminating the fusion reactions. As disruptions lead to an abrupt loss of confinement, they can cause irreversible damage to present-day fusion devices and are expected to have a more devastating effect in future devices. Disruptions expected in the next-generation tokamak, ITER, for example, could cause electromagnetic forces larger than the weight of an Airbus A380. Furthermore, the thermal loads in such an event could exceed the melting threshold of the most resistant state-of-the-art materials by more than an order of magnitude. To prevent disruptionsor at least mitigate their detrimental effects, empirical models obtained with artificial intelligence methods, of which an overview is given here, are commonly employed to predict their occurrence—and ideally give enough time to introduce counteracting measures.

Published
2022

44. Integrating Fault Tolerance and Load Balancing in Distributed Systems Based on CORBA

Author

Singh, A. V., Moser, L. E., Melliar-Smith, P. M., Hutchison, David, editor, Kanade, Takeo, editor, Kittler, Josef, editor, Kleinberg, Jon M., editor, Mattern, Friedemann, editor, Mitchell, John C., editor, Naor, Moni, editor, Nierstrasz, Oscar, editor, Pandu Rangan, C., editor, Steffen, Bernhard, editor, Sudan, Madhu, editor, Terzopoulos, Demetri, editor, Tygar, Dough, editor, Vardi, Moshe Y., editor, Weikum, Gerhard, editor, Dal Cin, Mario, editor, Kaâniche, Mohamed, editor, and Pataricza, András, editor

Published
2005
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47. Overview of the InterGroup Protocols

Author

Berket, K., Agarwal, D. A., Melliar-Smith, P. M., Moser, L. E., Goos, G., editor, Hartmanis, J., editor, van Leeuwen, J., editor, Alexandrov, Vassil N., editor, Dongarra, Jack J., editor, Juliano, Benjoe A., editor, Renner, René S., editor, and Tan, C. J. Kenneth, editor

Published
2001
Full Text
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