The May 17, 2012 solar event: Back-tracing analysis and flux reconstruction with PAMELA
| Autor: | Sergey Koldashov, Yu. T. Yurkin, V. V. Mikhailov, G. A. Bazilevskaya, R. Sparvoli, S. Y. Krutkov, M. Bongi, V. Di Felice, Yuri Stozhkov, Ulisse Bravar, P. Picozza, V. V. Malakhov, Mark Pearce, S. B. Ricciarini, Roberto Bellotti, R. Carbone, Steven Stochaj, N. De Simone, A. M. Galper, Sergey Koldobskiy, F. Cafagna, P. Papini, G. C. Barbarino, E. Vannuccini, A. G. Mayorov, Alfonso Monaco, E. Mocchiutti, E. C. Christian, A. V. Karelin, N. Zampa, M. Merge, S. A. Voronov, Per Carlson, C. De Santis, D. Campana, James M. Ryan, E. A. Bogomolov, V. G. Zverev, A. N. Kvashnin, G. Osteria, Marco Casolino, C. De Donato, M. Simon, V. Bonvicini, L. Marcelli, Maria Teresa Ricci, A. Vacchi, Valerio Formato, A. Bruno, G. I. Vasilyev, Nicola Mori, Matteo Martucci, G. A. de Nolfo, G. Castellini, Alexey Leonov, Ritabrata Sarkar, S. Bottai, Riccardo Munini, G. Zampa, Beatrice Panico, P. Spillantini, M. A. Lee, O. Adriani, W. Menn, F. Palma, Valentina Scotti, Mirko Boezio |
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| Přispěvatelé: | Bruno, A., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bravar, U., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., Christian, E. C., De Donato, C., De Nolfo, G. A., De Santis, C., De Simone, N., Felice, V. D., Formato, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Krutkov, S. Y., Kvashnin, A. N., Lee, M., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Mergè, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Ryan, J. M., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stochaj, S., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., Zverev, V. G. |
| Jazyk: | angličtina |
| Rok vydání: | 2016 |
| Předmět: |
Physics
Settore FIS/01 History Solar energetic particles Spacecraft business.industry Magnetosphere Direction of arrival Astrophysics Tracing Solar physics 01 natural sciences Computer Science Applications Education Computational physics Physics and Astronomy (all) 0103 physical sciences Physics::Space Physics Neutron Interplanetary magnetic field 010306 general physics business Angular distribution Cosmology Earth (planet) Low power electronics Orbits Solar system 010303 astronomy & astrophysics |
| Zdroj: | International Conference on Particle Physics and Astrophysics, ICPPA 2015, Moscow; Russian Federation, 05/10/2015, 10/10/2015 info:cnr-pdr/source/autori:Bruno A.; Adriani O.; Barbarino G.C.; Bazilevskaya G.A.; Bellotti R.; Boezio M.; Bogomolov E.A.; Bongi M.; Bonvicini V.; Bottai S.; Bravar U.; Cafagna F.; Campana D.; Carbone R.; Carlson P.; Casolino M.; Castellini G.; Christian E.C.; De Donato C.; De Nolfo G.A.; De Santis C.; De Simone N.; Felice V.D.; Formato V.; Galper A.M.; Karelin A.V.; Koldashov S.V.; Koldobskiy S.; Krutkov S.Y.; Kvashnin A.N.; Lee M.; Leonov A.; Malakhov V.; Marcelli L.; Martucci M.; Mayorov A.G.; Menn W.; Merge M.; Mikhailov V.V.; Mocchiutti E.; Monaco A.; Mori N.; Munini R.; Osteria G.; Palma F.; Panico B.; Papini P.; Pearce M.; Picozza P.; Ricci M.; Ricciarini S.B.; Ryan J.M.; Sarkar R.; Scotti V.; Simon M.; Sparvoli R.; Spillantini P.; Stochaj S.; Stozhkov Y.I.; Vacchi A.; Vannuccini E.; Vasilyev G.I.; Voronov S.A.; Yurkin Y.T.; Zampa G.; Zampa N.; Zverev V.G./congresso_nome:International Conference on Particle Physics and Astrophysics, ICPPA 2015/congresso_luogo:Moscow; Russian Federation/congresso_data:05%2F10%2F2015, 10%2F10%2F2015/anno:2016/pagina_da:/pagina_a:/intervallo_pagine |
| Popis: | The PAMELA space experiment is providing first direct observations of Solar Energetic Particles (SEPs) with energies from about 80 MeV to several GeV in near-Earth orbit, bridging the low energy measurements by other spacecrafts and the Ground Level Enhancement (GLE) data by the worldwide network of neutron monitors. Its unique observational capabilities include the possibility of measuring the flux angular distribution and thus investigating possible anisotropies associated to SEP events. The analysis is supported by an accurate back-tracing simulation based on a realistic description of the Earth's magnetosphere, which is exploited to estimate the SEP energy spectra as a function of the asymptotic direction of arrival with respect to the Interplanetary Magnetic Field (IMF). In this work we report the results for the May 17, 2012 event. |
| Databáze: | OpenAIRE |
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