%0 Journal Article %1 Malakhov_2015 %A Malakhov, V V %A Koldashov, S V %A Mayorov, A G %A Mayorova, M A %A Mikhailov, V V %A Aleksandrin, S Yu %A Adriani, O %A Barbarino, G C %A Bazilevskaya, G A %A Boezio, M %A Bogomolov, E A %A Bongi, M %A Bonvicini, V %A Bottai, S %A Bruno, A %A Cafagna, F %A Campana, D %A Carlson, P %A Casolino, M %A Castellini, G %A Donato, C De %A Santis, C De %A Simone, N De %A Felice, V Di %A Formato, V %A Galper, A M %A Karelin, A V %A Krutkov, S Yu %A Kvashnin, A A %A Kvashnin, A N %A Leonov, A A %A Marcelli, L %A Martucci, M %A Menn, W %A Merge, M %A Mocchuuitti, E %A Monaco, A %A Mori, N %A Munini, R %A Osteria, G %A Palma, F %A Panico, B %A Papini, P %A Pearce, M %A Picozza, P %A Ricci, M %A Ricciarini, S B %A Sarkar, R %A Scotti, V %A Simon, M %A Sparvoli, R %A Spillantini, P %A Stozhkov, Yu I %A Vacci, A %A Vannuccini, E %A Vasilyev, G I %A Voronov, S A %A Yurkin, Yu T %A Zampa, G %A Zampa, N %D 2015 %I IOP Publishing %J Journal of Physics: Conference Series %K pamela_exp %P 012069 %R 10.1088/1742-6596/632/1/012069 %T Time variations of proton flux in Earth inner radiation belt during 23/24 solar cycles based on the PAMELA and the ARINA data %U https://doi.org/10.1088%2F1742-6596%2F632%2F1%2F012069 %V 632 %X The PAMELA and the ARINA experiments are carried out on the board of satellite RESURS-DK1 since 2006 up to now. Main goal of the PAMELA instrument is measurements of high energy antiparticles in cosmic rays while the ARINA instrument is intended studying high energy charged particle bursts in the magnetosphere. Both of these experiments have a possibility to study trapped particles in the inner radiation belt. Complex of these two instruments covers proton energy range from 30 MeV up to trapping limit (E= ∼2 GeV). Continuous measurements with the PAMELA and the ARINA spectrometers include falling and rising phases of 23/24 solar cycles and maximum of 24th one. In this report we present temporal profiles of proton flux in the inner zone of the radiation belt (1.11 < L < 1.18, 0.18 < B < 0.22G). Dependence of proton fluxes on a magnitude of the solar activity was studied for various phases of 23/24 solar cycles. At that it was shown that proton fluxes at the solar minimum are several times greater than at the solar maximum.

@article{Malakhov_2015, abstract = {The PAMELA and the ARINA experiments are carried out on the board of satellite RESURS-DK1 since 2006 up to now. Main goal of the PAMELA instrument is measurements of high energy antiparticles in cosmic rays while the ARINA instrument is intended studying high energy charged particle bursts in the magnetosphere. Both of these experiments have a possibility to study trapped particles in the inner radiation belt. Complex of these two instruments covers proton energy range from 30 MeV up to trapping limit (E= ∼2 GeV). Continuous measurements with the PAMELA and the ARINA spectrometers include falling and rising phases of 23/24 solar cycles and maximum of 24th one. In this report we present temporal profiles of proton flux in the inner zone of the radiation belt (1.11 < L < 1.18, 0.18 < B < 0.22G). Dependence of proton fluxes on a magnitude of the solar activity was studied for various phases of 23/24 solar cycles. At that it was shown that proton fluxes at the solar minimum are several times greater than at the solar maximum.}, added-at = {2019-08-08T14:23:36.000+0200}, author = {Malakhov, V V and Koldashov, S V and Mayorov, A G and Mayorova, M A and Mikhailov, V V and Aleksandrin, S Yu and Adriani, O and Barbarino, G C and Bazilevskaya, G A and Boezio, M and Bogomolov, E A and Bongi, M and Bonvicini, V and Bottai, S and Bruno, A and Cafagna, F and Campana, D and Carlson, P and Casolino, M and Castellini, G and Donato, C De and Santis, C De and Simone, N De and Felice, V Di and Formato, V and Galper, A M and Karelin, A V and Krutkov, S Yu and Kvashnin, A A and Kvashnin, A N and Leonov, A A and Marcelli, L and Martucci, M and Menn, W and Merge, M and Mocchuuitti, E and Monaco, A and Mori, N and Munini, R and Osteria, G and Palma, F and Panico, B and Papini, P and Pearce, M and Picozza, P and Ricci, M and Ricciarini, S B and Sarkar, R and Scotti, V and Simon, M and Sparvoli, R and Spillantini, P and Stozhkov, Yu I and Vacci, A and Vannuccini, E and Vasilyev, G I and Voronov, S A and Yurkin, Yu T and Zampa, G and Zampa, N}, biburl = {https://www.bibsonomy.org/bibtex/25f73d013dce122c4294f161bb4de0ce4/pamela_exp}, doi = {10.1088/1742-6596/632/1/012069}, interhash = {b996e54eee0bb616a7bc6f47b0741e51}, intrahash = {5f73d013dce122c4294f161bb4de0ce4}, journal = {Journal of Physics: Conference Series}, keywords = {pamela_exp}, month = aug, pages = 012069, publisher = {{IOP} Publishing}, timestamp = {2019-08-08T14:23:36.000+0200}, title = {Time variations of proton flux in Earth inner radiation belt during 23/24 solar cycles based on the {PAMELA} and the {ARINA} data}, url = {https://doi.org/10.1088%2F1742-6596%2F632%2F1%2F012069}, volume = 632, year = 2015 }