PoS - Proceedings of Science
Volume 301 - 35th International Cosmic Ray Conference (ICRC2017) - Session Cosmic-Ray Direct. CRD- direct measurements
Effect of the Jupiter magnetosphere on the cosmic ray protons measured with the PAMELA experiment
M. Ricci*, G. Pizzella, M. Martucci, A. Bruno, V. Di Felice, N. Marcelli, O. Adriani, G. Barbarino, G.A. Bazilevskaya, R. Bellotti, M. Boezio, E.A. Bogomolov, M. Bongi, G. Bonvicini, F. Cafagna, D. Campana, P. Carlson, M. Casolino, G. Castellini, C. De Santis, A.M. Galper, A. Karelin, S. Koldashov, S. Koldobskiy, S.Y. Krutkov, A. Kvashnin, A. Leonov, V. Malakhov, L. Marcelli, A. Mayorov, A.G. Mayorov, M. Mergé, V. Mikhailov, E. Mocchiutti, A. Monaco, N. Mori, R. Munini, G. Osteria, B. Panico, P. Papini, M. Pearce, P. Picozza, S.B. Ricciarini, M. Simon, R. Sparvoli, P. Spillantini, Y. Stozhkov, A. Vacchi, E. Vannuccini, G. Vasilyev, S. Voronov, Y. Yurkin, G. Zampa and N. Zampaet al. (click to show)
Full text: pdf
Pre-published on: August 16, 2017
Published on: August 03, 2018
The very intense Jovian magnetic field produces a magnetosphere where high-energy charged
particles are trapped, allowing the possibility for acceleration mechanism that could inject those particles in the open space. In the last decades, accelerated electrons from the Jupiter magnetosphere have been detected and studied in the interplanetary space. This work investigated whether the proton data obtained by the PAMELA space-borne detector between July 9th, 2006 to August 31th, 2014 shows signatures that arise from Jupiter. In this proceeding the basis of the analysis of cosmic ray protons by PAMELA are described and results will be shown at the conference.
DOI: https://doi.org/10.22323/1.301.0178
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.