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Titel |
The large-scale anisotropy with the PAMELA calorimeter |
VerfasserIn |
A. Karelin, O. Adriani, G. Barbarino, G. Bazilevskaya, R. Bellotti, M. Boezio, E. Bogomolov, M. Bongi, V. Bonvicini, S. Bottai, A. Bruno, F. Cafagna, D. Campana, R. Carbone, P. Carlson, M. Casolino, G. Castellini, C. De Donato, C. De Santis, N. De Simone, V. Di Felice, V. Formato, A. Galper, S. Koldashov, S. Koldobskiy, S. Krut'kov, A. Kvashnin, A. Leonov, V. Malakhov, L. Marcelli, M. Martucci, A. Mayorov, W. Menn, M. Mergé, V. Mikhailov, E. Mocchiutti, A. Monaco, N. Mori, R. Munini, G. Osteria, F. Palma, B. Panico, P. Papini, M. Pearce, P. Picozza, M. Ricci, S. Ricciarini, R. Sarkar, M. Simon, V. Scotti, R. Sparvoli, P. Spillantini, Y. Stozhkov, A. Vacchi, E. Vannuccini, G. Vasilyev, S. Voronov, Y. Yurkin, G. Zampa, N. Zampa |
Medientyp |
Artikel
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Sprache |
Englisch
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ISSN |
2199-3955
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Digitales Dokument |
URL |
Erschienen |
In: ASTRA Proceedings ; 2, no. 2 ; Nr. 2, no. 2 (2015-10-02), S.35-37 |
Datensatznummer |
250115169
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Publikation (Nr.) |
copernicus.org/ap-2-35-2015.pdf |
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Zusammenfassung |
The large-scale anisotropy (or the so-called star-diurnal wave) has been
studied using the calorimeter of the space-born experiment PAMELA. The cosmic
ray anisotropy has been obtained for the Southern and Northern hemispheres
simultaneously in the equatorial coordinate system for the time period
2006–2014. The dipole amplitude and phase have been measured for energies
1–20 TeV n-1. |
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