76 results on '"Boezio, M."'
Search Results
2. Helium Fluxes Measured by the PAMELA Experiment from the Minimum to the Maximum Solar Activity for Solar Cycle 24.
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Marcelli, N., Boezio, M., Lenni, A., Menn, W., Munini, R., Aslam, O. P. M., Bisschoff, D., Ngobeni, M. D., Potgieter, M. S., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bruno, A., Cafagna, F., Campana, D., and Carlson, P.
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- 2022
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3. Cosmic-ray antinuclei as messengers of new physics: status and outlook for the new decade
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Doetinchem, P. von, primary, Perez, K., additional, Aramaki, T., additional, Baker, S., additional, Barwick, S., additional, Bird, R., additional, Boezio, M., additional, Boggs, S.E., additional, Cui, M., additional, Datta, A., additional, Donato, F., additional, Evoli, C., additional, Fabris, L., additional, Fabbietti, L., additional, Bueno, E. Ferronato, additional, Fornengo, N., additional, Fuke, H., additional, Gerrity, C., additional, Coral, D. Gomez, additional, Hailey, C., additional, Hooper, D., additional, Kachelriess, M., additional, Korsmeier, M., additional, Kozai, M., additional, Lea, R., additional, Li, N., additional, Lowell, A., additional, Manghisoni, M., additional, Moskalenko, I.V., additional, Munini, R., additional, Naskret, M., additional, Nelson, T., additional, Ng, K.C.Y., additional, Nozzoli, F., additional, Oliva, A., additional, Ong, R.A., additional, Osteria, G., additional, Pierog, T., additional, Poulin, V., additional, Profumo, S., additional, Pöschl, T., additional, Quinn, S., additional, Re, V., additional, Rogers, F., additional, Ryan, J., additional, Saffold, N., additional, Sakai, K., additional, Salati, P., additional, Schael, S., additional, Serksnyte, L., additional, Shukla, A., additional, Stoessl, A., additional, Tjemsland, J., additional, Vannuccini, E., additional, Vecchi, M., additional, Winkler, M.W., additional, Wright, D., additional, Xiao, M., additional, Xu, W., additional, Yoshida, T., additional, Zampa, G., additional, and Zuccon, P., additional
- Published
- 2020
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4. Cosmic Rays Investigation by the PAMELA experiment
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Panico, Beatrice, primary, Campana, D., additional, Osteria, G., additional, Barbarino, G. C., additional, Adriani, O., additional, Bongi, M., additional, Spillantini, P., additional, Mori, N., additional, Papini, P., additional, Vannuccini, E., additional, Bazilevskaya, G. A., additional, Kvashnin, A. N., additional, Stozhkov, Y. I., additional, Bellotti, R., additional, Monaco, A., additional, Bruno, A., additional, Cafagna, F., additional, Boezio, M., additional, Bonvicini, V., additional, Mocchiutti, E., additional, Munini, R., additional, Zampa, G., additional, Zampa, N., additional, Vacchi, A., additional, Bogomolov, E. A., additional, Krutkov, S. Y., additional, Vasilyev, G. I., additional, Carlson, P., additional, Pearce, M., additional, Casolino, M., additional, Castellini, G., additional, De Santis, C., additional, Marcelli, L., additional, Mergé, M., additional, Picozza, P., additional, Sparvoli, R., additional, Di Felice, V., additional, Galper, A. M., additional, Karelin, A. V., additional, Koldashov, S. V., additional, Koldobskiy, S., additional, Yurkin, Y. T., additional, Malakhov, V., additional, Leonov, A., additional, Mayorov, A. G., additional, Mikhailov, V. V., additional, Voronov, S. A., additional, Martucci, M., additional, Menn, W., additional, Simon, M., additional, Ricci, M., additional, and Ricciarini, S. B., additional
- Published
- 2020
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5. Time dependence of the proton and helium flux measured by PAMELA
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Panico, Beatrice, primary, Campana, D., additional, Osteria, G., additional, Barbarino, G. C., additional, Adriani, O., additional, Bongi, M., additional, Spillantini, P., additional, Mori, N., additional, Papini, P., additional, Vannuccini, E., additional, Bazilevskaya, G. A., additional, Kvashnin, A. N., additional, Stozhkov, Y. I., additional, Bellotti, R., additional, Monaco, A., additional, Bruno, A., additional, Cafagna, F., additional, Boezio, M., additional, Bonvicini, V., additional, Mocchiutti, E., additional, Munini, R., additional, Zampa, G., additional, Zampa, N., additional, Vacchi, A., additional, Bogomolov, E. A., additional, Krutkov, S. Y., additional, Vasilyev, G. I., additional, Carlson, P., additional, Pearce, M., additional, Casolino, M., additional, Castellini, G., additional, De Santis, C., additional, Marcelli, L., additional, Mergè, M., additional, Picozza, P., additional, Sparvoli, R., additional, Di Felice, V., additional, Galper, A. M., additional, Karelin, A. V., additional, Koldashov, S. V., additional, Koldobskiy, S., additional, Yurkin, Y. T., additional, Malakhov, V., additional, Leonov, A., additional, Mayorov, A. G., additional, Mikhailov, V. V., additional, Voronov, S. A., additional, Martucci, M., additional, Menn, W., additional, Simon, M., additional, Ricci, M., additional, and Ricciarini, S. B., additional
- Published
- 2020
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6. Cosmic ray electrons and positrons over decade with the PAMELA experiment
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Mikhailov, V V, primary, Adriani, O, additional, Barbarino, G, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bruno, A, additional, Cafagna, F S, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Santis, C, additional, Di Felice, V, additional, Galper, A M, additional, Karelin, A V, additional, Kleymenova, S O, additional, Koldashov, S V, additional, Koldobskiy, S, additional, Krutkov, S Yu, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorova, A G, additional, Menn, W, additional, Merge, M, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N., additional, Munini, R, additional, Osteria, G, additional, Papini, P, additional, Panico, B, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasiliev, G I, additional, Voronov, S A, additional, Yurkin, Yu T, additional, Zampa, G, additional, and Zampa, N, additional
- Published
- 2019
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7. Eastâ€"West Proton Flux Anisotropy Observed with the PAMELA Mission.
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Bruno, A., Martucci, M., Cafagna, F. S., Sparvoli, R., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Campana, D., Carlson, P., Casolino, M., Castellini, G., Santis, C. De, Galper, A. M., Koldashov, S. V., and Koldobskiy, S.
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ANISOTROPY ,PROTONS ,ASTROPHYSICS ,COSMIC rays ,ANTIMATTER - Abstract
We present a study of the eastâ€"west anisotropy of trapped-proton fluxes in low-Earth orbit based on the measurements of the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) experiment. The differential intensities of eastward- and westward-traveling protons detected in the South Atlantic Anomaly region were estimated as a function of equatorial pitch angle and drift shell, for six energy bins between 80 MeV and 2 GeV. We found that, as a consequence of the strong atmospheric gradient coupled with the large gyroradius in this energy range, the intensities of eastward fluxes exceed those of westward fluxes by a factor of âĽ10â€"20. However, the reported directional asymmetry also depends on the sign of the local flux gradient, resulting in more intense westward fluxes beyond the radial distances where the inner belt peaks. PAMELA observations can be used to improve the description of the near-Earth radiation environment at lowest altitudes and highest trapping energies, where current theoretical and empirical models are affected by the largest uncertainties. [ABSTRACT FROM AUTHOR]
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- 2021
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8. Solar-cycle Variations of South Atlantic Anomaly Proton Intensities Measured with the PAMELA Mission.
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Bruno, A., Martucci, M., Cafagna, F. S., Sparvoli, R., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Campana, D., Carlson, P., Casolino, M., Castellini, G., De Santis, C., Galper, A. M., Koldashov, S. V., and Koldobskiy, S.
- Published
- 2021
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9. Study of the 27 Day Variations in GCR Fluxes during 2007–2008 Based on PAMELA and ARINA Observations.
- Author
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Modzelewska, R., Bazilevskaya, G. A., Boezio, M., Koldashov, S. V., Krainev, M. B., Marcelli, N., Mayorov, A. G., Mayorova, M. A., Munini, R., Troitskaya, I. K., Yulbarisov, R. F., Luo, X., Potgieter, M. S., and Aslam, O. P. M.
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PLASMA sheaths ,GALACTIC cosmic rays ,SOLAR oscillations ,SOLAR wind ,FLUX (Energy) - Abstract
Using measurements from the PAMELA and ARINA spectrometers on board the Resurs-DK1 satellite, we have examined the 27 day intensity variations in galactic cosmic ray (GCR) proton fluxes in 2007–2008. The PAMELA and ARINA data allow for the first time a study of time profiles and the rigidity dependence of the 27 day variations observed directly in space in a wide rigidity range from ∼300 MV to several gigavolts. We find that the rigidity dependence of the amplitude of the 27 day GCR variations cannot be described by the same power law at both low and high energies. A flat interval occurs at rigidity GV with a power-law index γ = −0.13 ± 0.44 for PAMELA, whereas for R ≥ 1 GV, the power-law dependence is evident with index γ = −0.51 ± 0.11. We describe the rigidity dependence of the 27 day GCR variations for PAMELA and ARINA data in the framework of the modulation potential concept using the force-field approximation for GCR transport. For a physical interpretation, we have considered the relationship between the 27 day GCR variations and solar wind plasma and other heliospheric parameters. Moreover, we have discussed possible implications of MHD modeling of the solar wind plasma together with a stochastic GCR transport model concerning the effects of corotating interaction regions. [ABSTRACT FROM AUTHOR]
- Published
- 2020
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10. Time Dependence of the Flux of Helium Nuclei in Cosmic Rays Measured by the PAMELA Experiment between 2006 July and 2009 December.
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Marcelli, N., Boezio, M., Lenni, A., Menn, W., Munini, R., Aslam, O. P. M., Bisschoff, D., Ngobeni, M. D., Potgieter, M. S., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bruno, A., Cafagna, F., Campana, D., and Carlson, P.
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HELIUM , *COSMIC rays , *THRESHOLD energy , *HELIOSPHERE , *THREE-dimensional modeling , *MEASURING instruments - Abstract
Precise time-dependent measurements of the Z = 2 component in the cosmic radiation provide crucial information about the propagation of charged particles through the heliosphere. The PAMELA experiment, with its long flight duration (2006 June 15–2016 January 23) and the low energy threshold (80 MeV/n) is an ideal detector for cosmic-ray solar modulation studies. In this paper, the helium nuclei spectra measured by the PAMELA instrument from 2006 July to 2009 December over a Carrington rotation time basis are presented. A state-of-the-art three-dimensional model for cosmic-ray propagation inside the heliosphere was used to interpret the time-dependent measured fluxes. Proton-to-helium flux ratio time profiles at various rigidities are also presented in order to study any features that could result from the different masses and local interstellar spectra shapes. [ABSTRACT FROM AUTHOR]
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- 2020
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11. Modifications of a method for low energy gamma-ray incident angle reconstruction in the GAMMA-400 gamma-ray telescope
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Leonov, Aa, Galper, Am, Topchiev, Np, Bonvicini, V, Adriani, O, Arkhangelskaja, Iv, Arkhangelskiy, Ai, Bakaldin, Av, Bobkov, Sg, Boezio, M, Dalkarov, Od, Egorov, Ae, Glushkov, Na, Gorbunov, Ms, Gusakov, u. V., Y, Hnatyk, Bi, Kadilin, Vv, Kaplin, Va, Kheymits, Md, Korepanov, Ve, Longo, F, Mikhailov, Vv, Mocchiutti, E, Moiseev, Aa, Moskalenko, Iv, Naumov, Py, Picozza, P, Runtso, Mf, Serdin, Ov, Sparvoli, R, Spillantini, P, Stozhkov, Yi, Suchkov, Si, Taraskin, Aa, Tavani, M, Yurkin, Yt, Zverev, Vg, M. Strikhanov, O. Nagornov, S. Rubin, Leonov, A. A., Galper, A. M., Topchiev, N. P., Bonvicini, V., Adriani, O., Arkhangelskaja, I. V., Arkhangelskiy, A. I., Bakaldin, A. V., Bobkov, S. G., Boezio, M., Dalkarov, O. D., Egorov, A. E., Glushkov, N. A., Gorbunov, M. S., Gusakov, Yu. V., Hnatyk, B. I., Kadilin, V. V., Kaplin, V. A., Kheymits, M. D., Korepanov, V. E., Longo, F., Mikhailov, V. V., Mocchiutti, E., Moiseev, A. A., Moskalenko, I. V., Naumov, P. Y., Picozza, P., Runtso, M. F., Serdin, O. V., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Suchkov, S. I., Taraskin, A. A., Tavani, M., Yurkin, Y. T., and Zverev, V. G.
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Settore FIS/01 ,Physics ,History ,business.industry ,Gamma ray ,gamma-ray telescopes ,gamma-ray telescope ,Computer Science Applications ,Education ,gamma-ray astrophysics ,Low energy ,Optics ,business ,Gamma Ray, Gamm400 ,Fermi Gamma-ray Space Telescope - Abstract
The GAMMA-400 gamma-ray telescope is designed to measure the gamma-ray fluxes in the energy range from ∼20 MeV to ∼1 TeV, performing a sensitive search for high-energy gamma-ray emission when annihilating or decaying dark matter particles. Such measurements will be also associated with the following scientific goals: searching for new and studying known Galactic and extragalactic discrete high-energy gamma-ray sources (supernova remnants, pulsars, accreting objects, microquasars, active galactic nuclei, blazars, quasars). It will be possible to study their structure with high angular resolution and measuring their energy spectra and luminosity with high-energy resolution; identify discrete gamma-ray sources with known sources in other energy ranges. The major advantage of the GAMMA-400 instrument is excellent angular and energy resolutions for gamma rays above 10 GeV. The gamma-ray telescope angular and energy resolutions for the main aperture at 100-GeV gamma rays are ∼0.01% and ∼1%, respectively. The motivation of presented results is to improve physical characteristics of the GAMMA-400 gamma-ray telescope in the energy range of ∼20-100 MeV, most unexplored range today. Such observations are crucial today for a number of high-priority problems faced by modern astrophysics and fundamental physics, including the origin of chemical elements and cosmic rays, the nature of dark matter, and the applicability range of the fundamental laws of physics. To improve the reconstruction accuracy of incident angle for low-energy gamma rays the special analysis of topology of pair-conversion events in thin layers of converter performed. Choosing the pair-conversion events with more precise vertical localization allows us to obtain significantly better angular resolution in comparison with previous and current space and ground-based experiments. For 50-MeV gamma rays the GAMMA-400 gamma-ray telescope angular resolution is better than 50.
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- 2017
12. Sharp increasing of positron to electron fluxes ratio below 2 GV measured by the PAMELA
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Mikhailov, V V, primary, Adriani, O, additional, Barbarino, G, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F S, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C., additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V., additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobsky, S, additional, Krutkov, S Yu, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Merge, M, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N., additional, Munini, R, additional, Osteria, G, additional, Papini, P, additional, Palma, F, additional, Panico, B, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasiliev, G I, additional, Voronov, S A, additional, Yurkin, Yu T, additional, Zampa, G, additional, and Zampa, N, additional
- Published
- 2017
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13. High-energy gamma-ray studying with GAMMA-400 after Fermi-LAT
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Topchiev, N P, primary, Galper, A M, additional, Bonvicini, V, additional, Adriani, O, additional, Arkhangelskaja, I V, additional, Arkhangelskiy, A I, additional, Bakaldin, A V, additional, Bobkov, S G, additional, Boezio, M, additional, Dalkarov, O D, additional, Egorov, A E, additional, Gorbunov, M S, additional, Gusakov, Yu V, additional, Hnatyk, B I, additional, Kadilin, V V, additional, Kaplin, V A, additional, Kheymits, M D, additional, Korepanov, V E, additional, Leonov, A A, additional, Longo, F, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Moiseev, A A, additional, Moskalenko, I V, additional, Naumov, P Yu, additional, Picozza, P, additional, Runtso, M F, additional, Serdin, O V, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Suchkov, S I, additional, Taraskin, A A, additional, Tavani, M, additional, Yurkin, Yu T, additional, and Zverev, V G, additional
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- 2017
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14. Solar modulation of galactic cosmic rays during 2006-2015 based on PAMELA and ARINA data
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Mayorov, A G, primary, Adriani, O, additional, Aleksandrin, S Y, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Santis, C, additional, Di Felice, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Kvashnin, A A, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorova, M A, additional, Menn, W, additional, Merge’, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Naumov, P Yu, additional, Osteria, G, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Rodenko, S A, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional
- Published
- 2017
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15. The PAMELA experiment: a decade of Cosmic Ray Physics in space
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Galper, A M, primary, Sparvoli, R, additional, Adriani, O, additional, Barbarino, G, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, Di Felice, V, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mergè, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Simon, M, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional
- Published
- 2017
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16. The measurement of the dipole anisotropy of protons and helium cosmic rays with the PAMELA experiment
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Karelin, A V, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Felice, V Di, additional, Formato, V, additional, Galper, A M, additional, Koldobskiy, S A, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, AA, additional, Malakhov, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mergè, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, GI, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional
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- 2016
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17. Perspectives of the GAMMA-400 space observatory for high-energy gamma rays and cosmic rays measurements
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Topchiev, N P, primary, Galper, A M, additional, Bonvicini, V, additional, Adriani, O, additional, Aptekar, R L, additional, Arkhangelskaja, I V, additional, Arkhangelskiy, A I, additional, Bakaldin, A V, additional, Bergstrom, L, additional, Berti, E, additional, Bigongiari, G, additional, Bobkov, S G, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, S, additional, Bongi, M, additional, Bottai, S, additional, Castellini, G, additional, Cattaneo, P W, additional, Cumani, P, additional, Dalkarov, O D, additional, Dedenko, G L, additional, De Donato, C, additional, Dogiel, V A, additional, Finetti, N, additional, Gorbunov, M S, additional, Gusakov, Yu V, additional, Hnatyk, B I, additional, Kadilin, V V, additional, Kaplin, V A, additional, Kaplun, A A, additional, Kheymits, M D, additional, Korepanov, V E, additional, Larsson, J, additional, Leonov, A A, additional, Loginov, V A, additional, Longo, F, additional, Maestro, P, additional, Marrocchesi, P S, additional, Men'shenin, A L, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Moiseev, A A, additional, Mori, N, additional, Moskalenko, I V, additional, Naumov, P Yu, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Rappoldi, A, additional, Ricciarini, S, additional, Runtso, M F, additional, Ryde, F, additional, Serdin, O V, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Suchkov, S I, additional, Taraskin, A A, additional, Tavani, M, additional, Tiberio, A, additional, Tyurin, E M, additional, Ulanov, M V, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Yurkin, Yu T, additional, Zampa, N, additional, Zirakashvili, V N, additional, and Zverev, V G, additional
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- 2016
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18. H, He, Li and Be Isotopes in the PAMELA-Experiment
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Menn, W, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V., additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, di Felice, V, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malakhov, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Mergè, M, additional, Mikhailov, V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V., additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, Potgieter, M S, additional, and Vos, E E, additional
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- 2016
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19. The May 17, 2012 solar event: back-tracing analysis and flux reconstruction with PAMELA
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Bruno, A, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A., additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bravar, U, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Christian, E C, additional, De Donato, C, additional, de Nolfo, G A, additional, De Santis, C, additional, De Simone, N, additional, Felice, V Di, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Lee, M, additional, Leonov, A, additional, Malakhov, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mergè, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Ryan, J M, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stochaj, S, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional
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- 2016
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20. Features of re-entrant albedo deuteron trajectories in near Earth orbit with PAMELA experiment
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Koldobskiy, S A, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Felice, V Di, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, AA, additional, Malakhov, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mergè, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, GI, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional
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- 2016
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21. The GAMMA-400 gamma-ray telescope for precision gamma-ray emission investigations
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Topchiev, N P, primary, Galper, A M, additional, Bonvicini, V, additional, Adriani, O, additional, Aptekar, R L, additional, Arkhangelskaja, I V, additional, Arkhangelskiy, A I, additional, Bakaldin, A V, additional, Bergstrom, L, additional, Berti, E, additional, Bigongiari, G, additional, Bobkov, S G, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bottai, S, additional, Castellini, G, additional, Cattaneo, P W, additional, Cumani, P, additional, Dalkarov, O D, additional, Dedenko, G L, additional, De Donato, C, additional, Dogiel, V A, additional, Finetti, N, additional, Gascon, D, additional, Gorbunov, M S, additional, Gusakov, Yu V, additional, Hnatyk, B I, additional, Kadilin, V V, additional, Kaplin, V A, additional, Kaplun, A A, additional, Kheymits, M D, additional, Korepanov, V E, additional, Larsson, J, additional, Leonov, A A, additional, Loginov, V A, additional, Longo, F, additional, Maestro, P, additional, Marrocchesi, P S, additional, Martinez, M, additional, Men'shenin, A L, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Moiseev, A A, additional, Mori, N, additional, Moskalenko, I V, additional, Naumov, P Yu, additional, Papini, P, additional, Paredes, J M, additional, Pearce, M, additional, Picozza, P, additional, Rappoldi, A, additional, Ricciarini, S, additional, Runtso, M F, additional, Ryde, F, additional, Serdin, O V, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Suchkov, S I, additional, Taraskin, A A, additional, Tavani, M, additional, Tiberio, A, additional, Tyurin, E M, additional, Ulanov, M V, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Ward, J E, additional, Yurkin, Yu T, additional, Zampa, N, additional, Zirakashvili, V N, additional, and Zverev, V G, additional
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- 2016
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22. Trapped positrons observed by PAMELA experiment
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Mikhailov, V V, primary, Adriani, O, additional, Barbarino, G, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F S, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Santis, C, additional, De Simone, N, additional, Felice, V. Di, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobsky, S, additional, Krutkov, S Yu, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Merge, M, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N., additional, Munini, R, additional, Osteria, G, additional, Papini, P, additional, Palma, F, additional, Panico, B, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasiliev, G I, additional, Voronov, S A, additional, Yurkin, Yu T, additional, Zampa, G, additional, and Zampa, N, additional
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- 2016
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23. Study of deuteron spectra under radiation belt with PAMELA instrument
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Koldobskiy, S A, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Felice, V Di, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A A, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Merge’, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional
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- 2015
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24. Measurement of electron-positron spectrum in high-energy cosmic rays in the PAMELA experiment
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Karelin, A V, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Felice, V Di, additional, Formato, V., additional, Galper, A M, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A A, additional, Mayorov, A G, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M., additional, Menn, W, additional, Merge, M., additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R., additional, Osteria, G, additional, Palma, F, additional, Panico, B., additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V., additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional
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- 2015
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25. PAMELA measurements of the boron and carbon spectra
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Mori, N, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Felice, V Di, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malakhov, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mergé, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional
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- 2015
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26. Solar modulation of GCR electrons over the 23rd solar minimum with PAMELA
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Munini, R, primary, Di Felice, V, additional, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malakhov, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Merge, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, Potgieter, M S, additional, and Vos, E E, additional
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- 2015
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27. Time variations of proton flux in Earth inner radiation belt during 23/24 solar cycles based on the PAMELA and the ARINA data
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Malakhov, V V, primary, Koldashov, S V, additional, Mayorov, A G, additional, Mayorova, M A, additional, Mikhailov, V V, additional, Aleksandrin, S Yu, additional, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Krutkov, S Yu, additional, Kvashnin, A A, additional, Kvashnin, A N, additional, Leonov, A A, additional, Marcelli, L, additional, Martucci, M, additional, Menn, W, additional, Merge, M, additional, Mocchuuitti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Vacci, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Yu T, additional, Zampa, G, additional, and Zampa, N, additional
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- 2015
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28. CALOCUBE: an approach to high-granularity and homogenous calorimetry for space based detectors
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Bongi, M, primary, Adriani, O, additional, Albergo, S, additional, Auditore, L, additional, Bagliesi, M G, additional, Berti, E, additional, Bigongiari, G, additional, Boezio, M, additional, Bonechi, L, additional, Bonechi, S, additional, Bonvicini, V, additional, Bottai, S, additional, Brogi, P, additional, Carotenuto, G, additional, Cassese, A, additional, Castellini, G, additional, Cattaneo, P W, additional, Cauz, D, additional, Cumani, P, additional, D'Alessandro, R, additional, Detti, S, additional, Fasoli, M, additional, Gregorio, A, additional, Lamberto, A, additional, Lenzi, P, additional, Maestro, P, additional, Marrocchesi, P S, additional, Mezzasalma, A, additional, Miritello, M, additional, Mori, N, additional, Papini, P, additional, Pauletta, G, additional, Rappazzo, G F, additional, Rappoldi, A, additional, Ricciarini, S, additional, Spillantini, P, additional, Starodubtsev, O, additional, Sulaj, A, additional, Tiberio, A, additional, Trifirò, A, additional, Trimarchi, M, additional, Vannuccini, E, additional, Vedda, A, additional, Zampa, G, additional, Zampa, N, additional, and Zerbo, B, additional
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- 2015
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29. Study of solar modulation of galactic cosmic rays with the PAMELA and ARINA spectrometers in 2006-2012
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Bzheumikhova, M A, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, Pascale, M P De, additional, Santis, C De, additional, Simone, N De, additional, Felice, V Di, additional, Galper, A M, additional, Gillard, W, additional, Jerse, G, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Losev, D S, additional, Malakhov, V, additional, Marcelli, L, additional, Mayorov, A G, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Sidorov, A V, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Ulitin, A A, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional
- Published
- 2013
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30. The PAMELA experiment: light-nuclei selection with stand-alone detectors
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Carbone, R, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Bianco, A, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Formato, V, additional, Galper, A M, additional, Giaccari, U, additional, Grishantseva, L, additional, Jerse, G, additional, Karelin, A V, additional, Kheymits, M D, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malakhov, V, additional, Malvezzi, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Rossetto, L, additional, Sarkar, R, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional
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- 2013
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31. A search algorithm for finding Cosmic-Ray anisotropy with the PAMELA calorimeter
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Karelin, A V, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Galper, A M, additional, Gillard, W, additional, Jerse, G, additional, Kheymits, M D, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A A, additional, Mayorov, A G, additional, Malakhov, V V, additional, Marcelli, L, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional
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- 2013
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32. Cosmic ray electron and positron spectra measured with PAMELA
- Author
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Mikhailov, Vladimir, primary, Adriani, O, additional, Barbarino, G, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F S, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Galper, A M, additional, Jerse, G, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobsky, S, additional, Yu Krutkov, S, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Malvezzi, V, additional, Marcelli, L, additional, Mayorov, A G, additional, Menn, W, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Osteria, G, additional, Papini, P, additional, Palma, F, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Rossetto, L, additional, Sarkar, R, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasiliev, G I, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Yu T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional
- Published
- 2013
- Full Text
- View/download PDF
33. Measurement of antiproton flux in primary cosmic radiation with PAMELA experiment
- Author
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Mayorov, A G, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Galper, A M, additional, Gillard, W, additional, Jerse, G, additional, Karelin, A V, additional, Kheymits, M D, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Nikonov, N N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional
- Published
- 2013
- Full Text
- View/download PDF
34. Cosmic Ray Study with the PAMELA Experiment
- Author
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Picozza, P, primary, Marcelli, L, additional, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Galper, A M, additional, Grishantseva, L, additional, Jerse, G, additional, Karelin, A V, additional, Kheymits, M D, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malakhov, V, additional, Mayorov, A G, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Yurkin, Y T, additional, Wu, J, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional
- Published
- 2013
- Full Text
- View/download PDF
35. Search for cosmic ray electron-positron anisotropies with the Pamela data
- Author
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Campana, D, primary, Giaccari, U, additional, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Bianco, A, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Formato, V, additional, Galper, A M, additional, Grishantseva, L, additional, Jerse, G, additional, Karelin, A V, additional, Kheymits, M D, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malakhov, V, additional, Malvezzi, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Rossetto, L, additional, Sarkar, R, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional
- Published
- 2013
- Full Text
- View/download PDF
36. Galactic deuteron spectrum measured in PAMELA experiment
- Author
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Koldobskiy, S A, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Galper, A M, additional, Gillard, W, additional, Jerse, G, additional, Karelin, A V, additional, Kheymits, M D, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Mayorov, A G, additional, Menn, W, additional, Mikhailov, Y V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional
- Published
- 2013
- Full Text
- View/download PDF
37. PAMELA and indirect dark matter searches
- Author
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Boezio, M, primary, Pearce, M, additional, Picozza, P, additional, Sparvoli, R, additional, Spillantini, P, additional, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Pascale, M P, additional, Santis, C De, additional, Simone, N De, additional, Felice, V Di, additional, Galper, A M, additional, Grishantseva, L, additional, Gillard, W, additional, Hofverberg, P, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malvezzi, V, additional, Marcelli, L, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Mori, N, additional, Nikonov, N, additional, Osteria, G, additional, Papini, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Simon, M, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional
- Published
- 2009
- Full Text
- View/download PDF
38. Performance of the PAMELA Si-W imaging calorimeter in space
- Author
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Bonvicini, V, primary, Boezio, M, additional, Mocchiutti, E, additional, Vacchi, A, additional, Zampa, G, additional, Zampa, N, additional, Bellotti, R, additional, Bruno, A, additional, Cafagna, F, additional, Adriani, O, additional, Bonechi, L, additional, Bongi, M, additional, Bottai, S, additional, Fedele, D, additional, Papini, P, additional, Ricciarini, S, additional, Spillantini, P, additional, Taddei, E, additional, Vannuccini, E, additional, Castellini, G, additional, Ricci, M, additional, Basilevskaja, G A, additional, Kvashnin, A N, additional, Stozhkov, Y I, additional, Galper, A M, additional, Grishantseva, L, additional, Koldashov, S V, additional, Leonov, A, additional, Mikhailov, V V, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zverev, V G, additional, Barbarino, G, additional, Rosa, G De, additional, Osteria, G, additional, Campana, D, additional, Casolino, M, additional, Pascale, M P De, additional, Malvezzi, V, additional, Marcelli, L, additional, Minori, M, additional, Picozza, P, additional, Sparvoli, R, additional, Bogomolov, E A, additional, Krutkov, S Y, additional, Vasilyev, G, additional, Menn, W, additional, Simon, M, additional, Carlson, P, additional, Hofverberg, P, additional, Orsi, S, additional, and Pearce, M, additional
- Published
- 2009
- Full Text
- View/download PDF
39. The PAMELA space experiment: first year of operation
- Author
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Boezio, M, primary and Collaboration, the PAMELA, additional
- Published
- 2008
- Full Text
- View/download PDF
40. In-flight performance of SilEye-2 experiment and cosmic ray abundances inside the Mir space station
- Author
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Bidoli, V, primary, Casolino, M, additional, Grandis, E De, additional, Pascale, M P De, additional, Furano, G, additional, Morselli, A, additional, Narici, L, additional, Picozza, P, additional, Reali, E, additional, Sparvoli, R, additional, Galper, A, additional, Khodarovich, A, additional, Korotkov, M, additional, Popov, A, additional, Vavilov, N, additional, Mazzenga, G, additional, Ricci, M, additional, Castellini, G, additional, Avdeev, S, additional, Boezio, M, additional, Bonvicini, W, additional, Vacchi, A, additional, Zampa, N, additional, Papini, P, additional, Spillantini, P, additional, Carlson, P, additional, and Fuglesang, C, additional
- Published
- 2001
- Full Text
- View/download PDF
41. MEASUREMENT OF THE ISOTOPIC COMPOSITION OF HYDROGEN AND HELIUM NUCLEI IN COSMIC RAYS WITH THE PAMELA EXPERIMENT.
- Author
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ADRIANI, O., BARBARINO, G. C., BAZILEVSKAYA, G. A., BELLOTTI, R., BOEZIO, M., BOGOMOLOV, E. A., BONGI, M., BONVICINI, V., BORISOV, S., BOTTAI, S., BRUNO, A., CAFAGNA, F., CAMPANA, D., CARBONE, R., CARLSON, P., CASOLINO, M., CASTELLINI, G., DANILCHENKO, I. A., DE PASCALE, M. P., and DE SANTIS, C.
- Subjects
HYDROGEN isotopes ,HELIUM isotopes ,GALACTIC nuclei ,COSMIC rays ,EXPERIMENTS - Abstract
The satellite-borne experiment PAMELA has been used to make new measurements of cosmic ray H and He isotopes. he isotopic compositionwas measured between 100 and 600MeV/n for hydrogen and between 100 and 900MeV/n or helium isotopes over the 23rd solar minimum from 2006 July to 2007 December. The energy spectrum of these omponents carries fundamental information regarding the propagation of cosmic rays in the galaxy which are mpetitive with those obtained from other secondary to primary measurements such as B/C. [ABSTRACT FROM AUTHOR]
- Published
- 2013
- Full Text
- View/download PDF
42. TIME DEPENDENCE OF THE PROTON FLUX MEASURED BY PAMELA DURING THE 2006 JULY-2009 DECEMBER SOLAR MINIMUM.
- Author
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ADRIANI, O., BARBARINO, G. C., BAZILEVSKAYA, G. A., BELLOTTI, R., BOEZIO, M., BOGOMOLOV, E. A., BONGI, M., BONVICINI, V., BORISOV, S., BOTTAI, S., BRUNO, A., CAFAGNA, F., CAMPANA, D., CARBONE, R., CARLSON, P., CASOLINO, M., CASTELLINI, G., DE PASCALE, M. P., DE SANTIS, C., and DE SIMONE, N.
- Subjects
COSMIC rays ,EARTH (Planet) ,SOLAR magnetic fields ,HELIOSPHERE ,SUN ,PROTONS ,SOLAR wind - Abstract
The energy spectra of galactic cosmic rays carry fundamental information regarding their origin and propagation. These spectra, when measured near Earth, are significantly affected by the solar magnetic field. A comprehensive description of the cosmic radiation must therefore include the transport and modulation of cosmic rays inside the heliosphere. During the end of the last decade, the Sun underwent a peculiarly long quiet phase well suited to study modulation processes. In this paper we present proton spectra measured from 2006 July to 2009 December by PAMELA. The large collected statistics of protons allowed the time variation to be followed on a nearly monthly basis down to 400 MV. Data are compared with a state-of-the-art three-dimensional model of solar modulation. [ABSTRACT FROM AUTHOR]
- Published
- 2013
- Full Text
- View/download PDF
43. Solar energetic particle events in 2006-2012 in the PAMELA experiment data.
- Author
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Bazilevskaya, G A, Mayorov, A G, Malakhov, V V, Mikhailov, V V, Adriani, Barbarino, G C, Bellotti, R, Boezio, M, Bogomolov, E A, Bonechi, L, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, and Castellini, G
- Published
- 2013
- Full Text
- View/download PDF
44. OBSERVATIONS OF THE 2006 December 13 AND 14 SOLAR PARTICLE EVENTS IN THE 80 MeV n-1-3 GeV n-1 RANGE FROM SPACE WITH THE PAMELA DETECTOR.
- Author
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Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bonichi, L., Bongi, M., Bonvicini, V., Borisov, S., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., Consiglio, L., and De Pascale, M. P.
- Subjects
SOLAR energetic particles ,SPACE spectrometry ,SOLAR energy ,PROTON spectra ,HELIUM spectra - Abstract
We present the space spectrometer PAMELA observations of proton and helium fluxes during the 2006 December 13 and 14 solar particle events. This is the first direct measurement of the solar energetic particles in space with a single instrument in the energy range from ~80 MeV n
-1 up to ~3 GeV n-1 . For the December 13 event, measured energy spectra of solar protons and helium are compared with results obtained by neutron monitors and other detectors. Our measurements show a spectral behavior different from those derived from the neutron monitor network. No satisfactory analytical fitting was found for the energy spectra. During the first hours of the December 13 event, solar energetic particles spectra were close to the exponential form, demonstrating rather significant temporal evolution. Solar He with energy up to 1 GeV n-1 was recorded on December 13. For the December 14 event, energy of solar protons reached 600 MeV, whereas the maximum energy of He was below 100 MeV n-1 . The spectra were slightly bent in the lower energy range and preserved their form during the second event. Differences in the particle flux appearance and temporal evolution of these two events may argue for special conditions leading to the acceleration of solar particles up to relativistic energies. [ABSTRACT FROM AUTHOR]- Published
- 2011
- Full Text
- View/download PDF
45. The Cosmic-Ray Antiproton Flux between 3 and 49 GeV.
- Author
-
Boezio, M., Bonvicini, V., Schiavon, P., Vacchi, A., Zampa, N., Bergström, D., Carlson, P., Francke, T., Grinstein, S., Suffert, M., Hof, M., Kremer, J., Menn, W., Simon, M., Stephens, S. A., Ambriola, M., Bellotti, R., Cafagna, F., Ciacio, F., and Circella, M.
- Published
- 2001
- Full Text
- View/download PDF
46. TRAPPED PROTON FLUXES AT LOW EARTH ORBITS MEASURED BY THE PAMELA EXPERIMENT.
- Author
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Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., De Donato, C., De Santis, C., De Simone, N., and Felice, V. Di
- Published
- 2015
- Full Text
- View/download PDF
47. MEASUREMENT OF BORON AND CARBON FLUXES IN COSMIC RAYS WITH THE PAMELA EXPERIMENT.
- Author
-
Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., Danilchenko, I. A., Donato, C. De, Santis, C. De, and Simone, N. De
- Subjects
COSMIC rays ,GALAXIES ,BORON ,FLUX (Energy) ,CARBON ,KINETIC energy - Abstract
The propagation of cosmic rays inside our galaxy plays a fundamental role in shaping their injection spectra into those observed at Earth. One of the best tools to investigate this issue is the ratio of fluxes for secondary and primary species. The boron-to-carbon (B/C) ratio, in particular, is a sensitive probe to investigate propagation mechanisms. This paper presents new measurements of the absolute fluxes of boron and carbon nuclei as well as the B/C ratio from the PAMELA space experiment. The results span the range 0.44-129 GeV/n in kinetic energy for data taken in the period 2006 July to 2008 March. [ABSTRACT FROM AUTHOR]
- Published
- 2014
- Full Text
- View/download PDF
48. High-Energy Deuteron Measurement with the CAPRICE98 Experiment.
- Author
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Papini, P., Piccardi, S., Spillantini, P., Vannuccini, E., Ambriola, M., Bellotti, R., Cafagna, F., Ciacio, F., Circella, M., De Marzo, C. N., Bartalucci, S., Ricci, M., Bergström, D., Carlson, P., Francke, T., Hansen, P., Mocchiutti, E., Boezio, M., Bonvicini, V., and Schiavon, P.
- Published
- 2004
- Full Text
- View/download PDF
49. In-Orbit Performance of the Space Telescope NINA and Galactic Cosmic-Ray Flux Measurements.
- Author
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Bidoli, V., Canestro, A., Casolino, M., De Pascale, M. P., Furano, G., Iannucci, A., Morselli, A., Picozza, P., Reali, E., Sparvoli, R., Bakaldin, A., Galper, A., Koldashov, S., Korotkov, M., Leonov, A., Mikhailov, V., Murashov, A., Voronov, S., Boezio, M., and Bonvicini, V.
- Published
- 2001
- Full Text
- View/download PDF
50. First Mass-resolved Measurement of High-Energy Cosmic-Ray Antiprotons.
- Author
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Bergström, D., Boezio, M., Carlson, P., Francke, T., Grinstein, S., Khalchukov, F., Suffert, M., Hof, M., Kremer, J., Menn, W., Simon, M., Stephens, S. A., Ambriola, M. L., Bellotti, R., Cafagna, F., Ciacio, F., Circella, M., De Marzo, C., Finetti, N., and Papini, P.
- Published
- 2000
- Full Text
- View/download PDF
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