WFRF:(De Felice M.)
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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 04554naa a2201021 4500 | |
| 001 | oai:DiVA.org:kth-175945 | |
| 003 | SwePub | |
| 008 | 151026s2015 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-1759452 URI |
| 024 | 7 | a https://doi.org/10.1088/1742-6596/632/1/0120692 DOI |
| 040 | a (SwePub)kth | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a kon2 swepub-publicationtype |
| 100 | 1 | a Malakhov, V. V.4 aut |
| 245 | 1 0 | a Time variations of proton flux in Earth inner radiation belt during 23/24 solar cycles based on the PAMELA and the ARINA data. |
| 264 | c 2015-08-13 | |
| 264 | 1 | b IOP Publishing,c 2015 |
| 338 | a print2 rdacarrier | |
| 500 | a QC 20151102 | |
| 520 | a 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= similar to 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. | |
| 650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
| 700 | 1 | a Koldashov, S. V.4 aut |
| 700 | 1 | a Mayorov, A. G.4 aut |
| 700 | 1 | a Mayorova, M. A.4 aut |
| 700 | 1 | a Mikhailov, V. V.4 aut |
| 700 | 1 | a Aleksandrin, S. Yu4 aut |
| 700 | 1 | a Adriani, O.4 aut |
| 700 | 1 | a Barbarino, G. C.4 aut |
| 700 | 1 | a Bazilevskaya, G. A.4 aut |
| 700 | 1 | a Boezio, M.4 aut |
| 700 | 1 | a Bogomolov, E. A.4 aut |
| 700 | 1 | a Bongi, M.4 aut |
| 700 | 1 | a Bonvicini, V.4 aut |
| 700 | 1 | a Bottai, S.4 aut |
| 700 | 1 | a Bruno, A.4 aut |
| 700 | 1 | a Cafagna, F.4 aut |
| 700 | 1 | a Campana, D.4 aut |
| 700 | 1 | a Carlson, Peru KTH,Partikel- och astropartikelfysik,Oskar Klein Centre for Cosmoparticle Physics, Sweden4 aut0 (Swepub:kth)u1ua4u32 |
| 700 | 1 | a Casolino, M.4 aut |
| 700 | 1 | a Castellini, G.4 aut |
| 700 | 1 | a De Donato, C.4 aut |
| 700 | 1 | a De Santis, C.4 aut |
| 700 | 1 | a De Simone, N.4 aut |
| 700 | 1 | a Di Felice, V.4 aut |
| 700 | 1 | a Formato, V.4 aut |
| 700 | 1 | a Galper, A. M.4 aut |
| 700 | 1 | a Karelin, A. V.4 aut |
| 700 | 1 | a Krutkov, S. Yu4 aut |
| 700 | 1 | a Kvashnin, A. A.4 aut |
| 700 | 1 | a Kvashnin, A. N.4 aut |
| 700 | 1 | a Leonov, A. A.4 aut |
| 700 | 1 | a Marcelli, L.4 aut |
| 700 | 1 | a Martucci, M.4 aut |
| 700 | 1 | a Menn, W.4 aut |
| 700 | 1 | a Merge, M.4 aut |
| 700 | 1 | a Mocchuuitti, E.4 aut |
| 700 | 1 | a Monaco, A.4 aut |
| 700 | 1 | a Mori, N.4 aut |
| 700 | 1 | a Munini, R.4 aut |
| 700 | 1 | a Osteria, G.4 aut |
| 700 | 1 | a Palma, F.4 aut |
| 700 | 1 | a Panico, B.4 aut |
| 700 | 1 | a Papini, P.4 aut |
| 700 | 1 | a Pearce, Marku KTH,Partikel- och astropartikelfysik,Oskar Klein Centre for Cosmoparticle Physics, Sweden4 aut0 (Swepub:kth)u17jptna |
| 700 | 1 | a Picozza, P.4 aut |
| 700 | 1 | a Ricci, M.4 aut |
| 700 | 1 | a Ricciarini, S. B.4 aut |
| 700 | 1 | a Sarkar, R.4 aut |
| 700 | 1 | a Scotti, V.4 aut |
| 700 | 1 | a Simon, M.4 aut |
| 700 | 1 | a Sparvoli, R.4 aut |
| 700 | 1 | a Spillantini, P.4 aut |
| 700 | 1 | a Stozhkov, Yu I.4 aut |
| 700 | 1 | a Vacci, A.4 aut |
| 700 | 1 | a Vannuccini, E.4 aut |
| 700 | 1 | a Vasilyev, G. I.4 aut |
| 700 | 1 | a Voronov, S. A.4 aut |
| 700 | 1 | a Yurkin, Yu T.4 aut |
| 700 | 1 | a Zampa, G.4 aut |
| 700 | 1 | a Zampa, N.4 aut |
| 710 | 2 | a KTHb Partikel- och astropartikelfysik4 org |
| 773 | 0 | t 24TH EUROPEAN COSMIC RAY SYMPOSIUM (ECRS)d : IOP Publishing |
| 856 | 4 | u http://iopscience.iop.org/article/10.1088/1742-6596/632/1/012069/pdf |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-175945 |
| 856 | 4 8 | u https://doi.org/10.1088/1742-6596/632/1/012069 |
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- Malakhov, V. V.
- Koldashov, S. V.
- Mayorov, A. G.
- Mayorova, M. A.
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- Adriani, O.
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- Bottai, S.
- Bruno, A.
- Cafagna, F.
- Campana, D.
- Carlson, Per
- Casolino, M.
- Castellini, G.
- De Donato, C.
- De Santis, C.
- De Simone, N.
- Di Felice, V.
- Formato, V.
- Galper, A. M.
- Karelin, A. V.
- Krutkov, S. Yu
- Kvashnin, A. A.
- Kvashnin, A. N.
- Leonov, A. A.
- Marcelli, L.
- Martucci, M.
- Menn, W.
- Merge, M.
- Mocchuuitti, E.
- Monaco, A.
- Mori, N.
- Munini, R.
- Osteria, G.
- Palma, F.
- Panico, B.
- Papini, P.
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- Scotti, V.
- Simon, M.
- Sparvoli, R.
- Spillantini, P.
- Stozhkov, Yu I.
- Vacci, A.
- Vannuccini, E.
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- Voronov, S. A.
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