Secondary electron and positron fluxes in the near-Earth space observed in the ARINA and PAMELA experiments
Abstract Secondary electron and positron fluxes in the energy range from 3 MeV to 7 GeV were measured with the ARINA and PAMELA spectrometers onboard the Resurs-DK satellite launched on June 15, 2006 into an elliptical orbit with an inclination of 70.4° and an altitude of 350–600 km. It is shown tha...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Adriani, O. [verfasserIn] Bazilevskaya, G. A. [verfasserIn] Barbarino, G. C. [verfasserIn] Bellotti, T. R. [verfasserIn] Bzheumikhova, M. A. [verfasserIn] Bogomolov, E. A. [verfasserIn] Boezio, V. M. [verfasserIn] Bonvicini, V. [verfasserIn] Bongi, M. [verfasserIn] Bonechi, L. [verfasserIn] Bottai, S. [verfasserIn] Bruno, A. [verfasserIn] Vacchi, A. [verfasserIn] Vannuccini, E. [verfasserIn] Vasiliev, G. V. [verfasserIn] Voronov, S. A. [verfasserIn] Galper, A. M. [verfasserIn] Grishantseva, L. A. [verfasserIn] Zampa, G. [verfasserIn] Zampa, N. [verfasserIn] Zverev, V. G. [verfasserIn] Casolino, M. [verfasserIn] Campana, T. D. [verfasserIn] Carlson, P. [verfasserIn] Castellini, G. [verfasserIn] Cafagna, F. [verfasserIn] Kvashnin, A. N. [verfasserIn] Koldashov, S. V. [verfasserIn] Krutkov, S. Yu. [verfasserIn] Leonov, A. A. [verfasserIn] Malakhov, V. V. [verfasserIn] Malvezzi, V. [verfasserIn] Marcelli, L. [verfasserIn] Menn, W. [verfasserIn] Mikhailov, V. V. [verfasserIn] Mocchiutti, E. [verfasserIn] Orsi, S. [verfasserIn] Osteria, G. [verfasserIn] Papini, P. [verfasserIn] De Pascale, M. P. [verfasserIn] Picozza, T. P. [verfasserIn] Pearce, M. [verfasserIn] De Rosa, G. [verfasserIn] Ricci, M. [verfasserIn] Ricciarini, S. B. [verfasserIn] Simon, M. [verfasserIn] De Simone, N. [verfasserIn] Sparvoli, R. [verfasserIn] Spillantini, P. [verfasserIn] Stozhkov, Yu. I. [verfasserIn] Taddei, E. [verfasserIn] Di Felice, V. [verfasserIn] Fedele, D. [verfasserIn] Hofverberg, P. [verfasserIn] Yurkin, Yu. T. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2009 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Bulletin of the Russian Academy of Sciences - New York, NY : Allerton Press, 2007, 73(2009), 3 vom: März, Seite 364-366 |
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| Übergeordnetes Werk: |
volume:73 ; year:2009 ; number:3 ; month:03 ; pages:364-366 |
| Links: |
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| DOI / URN: |
10.3103/S1062873809030253 |
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| Katalog-ID: |
SPR023150785 |
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| 100 | 1 | |a Adriani, O. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Secondary electron and positron fluxes in the near-Earth space observed in the ARINA and PAMELA experiments |
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| 520 | |a Abstract Secondary electron and positron fluxes in the energy range from 3 MeV to 7 GeV were measured with the ARINA and PAMELA spectrometers onboard the Resurs-DK satellite launched on June 15, 2006 into an elliptical orbit with an inclination of 70.4° and an altitude of 350–600 km. It is shown that positrons dominate over electrons by a factor of up to 4–5 in the geomagnetic equator region (L < 1.2 and B > 0.25). | ||
| 650 | 4 | |a Magnetic Anomaly |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Experimental Data Analysis |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a PAMELA Experiment |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Positron Flux |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Good Statistical Accuracy |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Bazilevskaya, G. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Barbarino, G. C. |e verfasserin |4 aut | |
| 700 | 1 | |a Bellotti, T. R. |e verfasserin |4 aut | |
| 700 | 1 | |a Bzheumikhova, M. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Bogomolov, E. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Boezio, V. M. |e verfasserin |4 aut | |
| 700 | 1 | |a Bonvicini, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Bongi, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Bonechi, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Bottai, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Bruno, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Vacchi, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Vannuccini, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Vasiliev, G. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Voronov, S. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Galper, A. M. |e verfasserin |4 aut | |
| 700 | 1 | |a Grishantseva, L. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Zampa, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Zampa, N. |e verfasserin |4 aut | |
| 700 | 1 | |a Zverev, V. G. |e verfasserin |4 aut | |
| 700 | 1 | |a Casolino, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Campana, T. D. |e verfasserin |4 aut | |
| 700 | 1 | |a Carlson, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Castellini, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Cafagna, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Kvashnin, A. N. |e verfasserin |4 aut | |
| 700 | 1 | |a Koldashov, S. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Krutkov, S. Yu. |e verfasserin |4 aut | |
| 700 | 1 | |a Leonov, A. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Malakhov, V. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Malvezzi, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Marcelli, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Menn, W. |e verfasserin |4 aut | |
| 700 | 1 | |a Mikhailov, V. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Mocchiutti, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Orsi, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Osteria, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Papini, P. |e verfasserin |4 aut | |
| 700 | 1 | |a De Pascale, M. P. |e verfasserin |4 aut | |
| 700 | 1 | |a Picozza, T. P. |e verfasserin |4 aut | |
| 700 | 1 | |a Pearce, M. |e verfasserin |4 aut | |
| 700 | 1 | |a De Rosa, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Ricci, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Ricciarini, S. B. |e verfasserin |4 aut | |
| 700 | 1 | |a Simon, M. |e verfasserin |4 aut | |
| 700 | 1 | |a De Simone, N. |e verfasserin |4 aut | |
| 700 | 1 | |a Sparvoli, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Spillantini, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Stozhkov, Yu. I. |e verfasserin |4 aut | |
| 700 | 1 | |a Taddei, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Di Felice, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Fedele, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Hofverberg, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Yurkin, Yu. T. |e verfasserin |4 aut | |
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10.3103/S1062873809030253 doi (DE-627)SPR023150785 (SPR)S1062873809030253-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Adriani, O. verfasserin aut Secondary electron and positron fluxes in the near-Earth space observed in the ARINA and PAMELA experiments 2009 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Secondary electron and positron fluxes in the energy range from 3 MeV to 7 GeV were measured with the ARINA and PAMELA spectrometers onboard the Resurs-DK satellite launched on June 15, 2006 into an elliptical orbit with an inclination of 70.4° and an altitude of 350–600 km. It is shown that positrons dominate over electrons by a factor of up to 4–5 in the geomagnetic equator region (L < 1.2 and B > 0.25). Magnetic Anomaly (dpeaa)DE-He213 Experimental Data Analysis (dpeaa)DE-He213 PAMELA Experiment (dpeaa)DE-He213 Positron Flux (dpeaa)DE-He213 Good Statistical Accuracy (dpeaa)DE-He213 Bazilevskaya, G. A. verfasserin aut Barbarino, G. C. verfasserin aut Bellotti, T. R. verfasserin aut Bzheumikhova, M. A. verfasserin aut Bogomolov, E. A. verfasserin aut Boezio, V. M. verfasserin aut Bonvicini, V. verfasserin aut Bongi, M. verfasserin aut Bonechi, L. verfasserin aut Bottai, S. verfasserin aut Bruno, A. verfasserin aut Vacchi, A. verfasserin aut Vannuccini, E. verfasserin aut Vasiliev, G. V. verfasserin aut Voronov, S. A. verfasserin aut Galper, A. M. verfasserin aut Grishantseva, L. A. verfasserin aut Zampa, G. verfasserin aut Zampa, N. verfasserin aut Zverev, V. G. verfasserin aut Casolino, M. verfasserin aut Campana, T. D. verfasserin aut Carlson, P. verfasserin aut Castellini, G. verfasserin aut Cafagna, F. verfasserin aut Kvashnin, A. N. verfasserin aut Koldashov, S. V. verfasserin aut Krutkov, S. Yu. verfasserin aut Leonov, A. A. verfasserin aut Malakhov, V. V. verfasserin aut Malvezzi, V. verfasserin aut Marcelli, L. verfasserin aut Menn, W. verfasserin aut Mikhailov, V. V. verfasserin aut Mocchiutti, E. verfasserin aut Orsi, S. verfasserin aut Osteria, G. verfasserin aut Papini, P. verfasserin aut De Pascale, M. P. verfasserin aut Picozza, T. P. verfasserin aut Pearce, M. verfasserin aut De Rosa, G. verfasserin aut Ricci, M. verfasserin aut Ricciarini, S. B. verfasserin aut Simon, M. verfasserin aut De Simone, N. verfasserin aut Sparvoli, R. verfasserin aut Spillantini, P. verfasserin aut Stozhkov, Yu. I. verfasserin aut Taddei, E. verfasserin aut Di Felice, V. verfasserin aut Fedele, D. verfasserin aut Hofverberg, P. verfasserin aut Yurkin, Yu. T. verfasserin aut Enthalten in Bulletin of the Russian Academy of Sciences New York, NY : Allerton Press, 2007 73(2009), 3 vom: März, Seite 364-366 (DE-627)556723872 (DE-600)2403169-0 1934-9432 nnns volume:73 year:2009 number:3 month:03 pages:364-366 https://dx.doi.org/10.3103/S1062873809030253 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 73 2009 3 03 364-366 |
| spelling |
10.3103/S1062873809030253 doi (DE-627)SPR023150785 (SPR)S1062873809030253-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Adriani, O. verfasserin aut Secondary electron and positron fluxes in the near-Earth space observed in the ARINA and PAMELA experiments 2009 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Secondary electron and positron fluxes in the energy range from 3 MeV to 7 GeV were measured with the ARINA and PAMELA spectrometers onboard the Resurs-DK satellite launched on June 15, 2006 into an elliptical orbit with an inclination of 70.4° and an altitude of 350–600 km. It is shown that positrons dominate over electrons by a factor of up to 4–5 in the geomagnetic equator region (L < 1.2 and B > 0.25). Magnetic Anomaly (dpeaa)DE-He213 Experimental Data Analysis (dpeaa)DE-He213 PAMELA Experiment (dpeaa)DE-He213 Positron Flux (dpeaa)DE-He213 Good Statistical Accuracy (dpeaa)DE-He213 Bazilevskaya, G. A. verfasserin aut Barbarino, G. C. verfasserin aut Bellotti, T. R. verfasserin aut Bzheumikhova, M. A. verfasserin aut Bogomolov, E. A. verfasserin aut Boezio, V. M. verfasserin aut Bonvicini, V. verfasserin aut Bongi, M. verfasserin aut Bonechi, L. verfasserin aut Bottai, S. verfasserin aut Bruno, A. verfasserin aut Vacchi, A. verfasserin aut Vannuccini, E. verfasserin aut Vasiliev, G. V. verfasserin aut Voronov, S. A. verfasserin aut Galper, A. M. verfasserin aut Grishantseva, L. A. verfasserin aut Zampa, G. verfasserin aut Zampa, N. verfasserin aut Zverev, V. G. verfasserin aut Casolino, M. verfasserin aut Campana, T. D. verfasserin aut Carlson, P. verfasserin aut Castellini, G. verfasserin aut Cafagna, F. verfasserin aut Kvashnin, A. N. verfasserin aut Koldashov, S. V. verfasserin aut Krutkov, S. Yu. verfasserin aut Leonov, A. A. verfasserin aut Malakhov, V. V. verfasserin aut Malvezzi, V. verfasserin aut Marcelli, L. verfasserin aut Menn, W. verfasserin aut Mikhailov, V. V. verfasserin aut Mocchiutti, E. verfasserin aut Orsi, S. verfasserin aut Osteria, G. verfasserin aut Papini, P. verfasserin aut De Pascale, M. P. verfasserin aut Picozza, T. P. verfasserin aut Pearce, M. verfasserin aut De Rosa, G. verfasserin aut Ricci, M. verfasserin aut Ricciarini, S. B. verfasserin aut Simon, M. verfasserin aut De Simone, N. verfasserin aut Sparvoli, R. verfasserin aut Spillantini, P. verfasserin aut Stozhkov, Yu. I. verfasserin aut Taddei, E. verfasserin aut Di Felice, V. verfasserin aut Fedele, D. verfasserin aut Hofverberg, P. verfasserin aut Yurkin, Yu. T. verfasserin aut Enthalten in Bulletin of the Russian Academy of Sciences New York, NY : Allerton Press, 2007 73(2009), 3 vom: März, Seite 364-366 (DE-627)556723872 (DE-600)2403169-0 1934-9432 nnns volume:73 year:2009 number:3 month:03 pages:364-366 https://dx.doi.org/10.3103/S1062873809030253 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 73 2009 3 03 364-366 |
| allfields_unstemmed |
10.3103/S1062873809030253 doi (DE-627)SPR023150785 (SPR)S1062873809030253-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Adriani, O. verfasserin aut Secondary electron and positron fluxes in the near-Earth space observed in the ARINA and PAMELA experiments 2009 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Secondary electron and positron fluxes in the energy range from 3 MeV to 7 GeV were measured with the ARINA and PAMELA spectrometers onboard the Resurs-DK satellite launched on June 15, 2006 into an elliptical orbit with an inclination of 70.4° and an altitude of 350–600 km. It is shown that positrons dominate over electrons by a factor of up to 4–5 in the geomagnetic equator region (L < 1.2 and B > 0.25). Magnetic Anomaly (dpeaa)DE-He213 Experimental Data Analysis (dpeaa)DE-He213 PAMELA Experiment (dpeaa)DE-He213 Positron Flux (dpeaa)DE-He213 Good Statistical Accuracy (dpeaa)DE-He213 Bazilevskaya, G. A. verfasserin aut Barbarino, G. C. verfasserin aut Bellotti, T. R. verfasserin aut Bzheumikhova, M. A. verfasserin aut Bogomolov, E. A. verfasserin aut Boezio, V. M. verfasserin aut Bonvicini, V. verfasserin aut Bongi, M. verfasserin aut Bonechi, L. verfasserin aut Bottai, S. verfasserin aut Bruno, A. verfasserin aut Vacchi, A. verfasserin aut Vannuccini, E. verfasserin aut Vasiliev, G. V. verfasserin aut Voronov, S. A. verfasserin aut Galper, A. M. verfasserin aut Grishantseva, L. A. verfasserin aut Zampa, G. verfasserin aut Zampa, N. verfasserin aut Zverev, V. G. verfasserin aut Casolino, M. verfasserin aut Campana, T. D. verfasserin aut Carlson, P. verfasserin aut Castellini, G. verfasserin aut Cafagna, F. verfasserin aut Kvashnin, A. N. verfasserin aut Koldashov, S. V. verfasserin aut Krutkov, S. Yu. verfasserin aut Leonov, A. A. verfasserin aut Malakhov, V. V. verfasserin aut Malvezzi, V. verfasserin aut Marcelli, L. verfasserin aut Menn, W. verfasserin aut Mikhailov, V. V. verfasserin aut Mocchiutti, E. verfasserin aut Orsi, S. verfasserin aut Osteria, G. verfasserin aut Papini, P. verfasserin aut De Pascale, M. P. verfasserin aut Picozza, T. P. verfasserin aut Pearce, M. verfasserin aut De Rosa, G. verfasserin aut Ricci, M. verfasserin aut Ricciarini, S. B. verfasserin aut Simon, M. verfasserin aut De Simone, N. verfasserin aut Sparvoli, R. verfasserin aut Spillantini, P. verfasserin aut Stozhkov, Yu. I. verfasserin aut Taddei, E. verfasserin aut Di Felice, V. verfasserin aut Fedele, D. verfasserin aut Hofverberg, P. verfasserin aut Yurkin, Yu. T. verfasserin aut Enthalten in Bulletin of the Russian Academy of Sciences New York, NY : Allerton Press, 2007 73(2009), 3 vom: März, Seite 364-366 (DE-627)556723872 (DE-600)2403169-0 1934-9432 nnns volume:73 year:2009 number:3 month:03 pages:364-366 https://dx.doi.org/10.3103/S1062873809030253 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 73 2009 3 03 364-366 |
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10.3103/S1062873809030253 doi (DE-627)SPR023150785 (SPR)S1062873809030253-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Adriani, O. verfasserin aut Secondary electron and positron fluxes in the near-Earth space observed in the ARINA and PAMELA experiments 2009 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Secondary electron and positron fluxes in the energy range from 3 MeV to 7 GeV were measured with the ARINA and PAMELA spectrometers onboard the Resurs-DK satellite launched on June 15, 2006 into an elliptical orbit with an inclination of 70.4° and an altitude of 350–600 km. It is shown that positrons dominate over electrons by a factor of up to 4–5 in the geomagnetic equator region (L < 1.2 and B > 0.25). Magnetic Anomaly (dpeaa)DE-He213 Experimental Data Analysis (dpeaa)DE-He213 PAMELA Experiment (dpeaa)DE-He213 Positron Flux (dpeaa)DE-He213 Good Statistical Accuracy (dpeaa)DE-He213 Bazilevskaya, G. A. verfasserin aut Barbarino, G. C. verfasserin aut Bellotti, T. R. verfasserin aut Bzheumikhova, M. A. verfasserin aut Bogomolov, E. A. verfasserin aut Boezio, V. M. verfasserin aut Bonvicini, V. verfasserin aut Bongi, M. verfasserin aut Bonechi, L. verfasserin aut Bottai, S. verfasserin aut Bruno, A. verfasserin aut Vacchi, A. verfasserin aut Vannuccini, E. verfasserin aut Vasiliev, G. V. verfasserin aut Voronov, S. A. verfasserin aut Galper, A. M. verfasserin aut Grishantseva, L. A. verfasserin aut Zampa, G. verfasserin aut Zampa, N. verfasserin aut Zverev, V. G. verfasserin aut Casolino, M. verfasserin aut Campana, T. D. verfasserin aut Carlson, P. verfasserin aut Castellini, G. verfasserin aut Cafagna, F. verfasserin aut Kvashnin, A. N. verfasserin aut Koldashov, S. V. verfasserin aut Krutkov, S. Yu. verfasserin aut Leonov, A. A. verfasserin aut Malakhov, V. V. verfasserin aut Malvezzi, V. verfasserin aut Marcelli, L. verfasserin aut Menn, W. verfasserin aut Mikhailov, V. V. verfasserin aut Mocchiutti, E. verfasserin aut Orsi, S. verfasserin aut Osteria, G. verfasserin aut Papini, P. verfasserin aut De Pascale, M. P. verfasserin aut Picozza, T. P. verfasserin aut Pearce, M. verfasserin aut De Rosa, G. verfasserin aut Ricci, M. verfasserin aut Ricciarini, S. B. verfasserin aut Simon, M. verfasserin aut De Simone, N. verfasserin aut Sparvoli, R. verfasserin aut Spillantini, P. verfasserin aut Stozhkov, Yu. I. verfasserin aut Taddei, E. verfasserin aut Di Felice, V. verfasserin aut Fedele, D. verfasserin aut Hofverberg, P. verfasserin aut Yurkin, Yu. T. verfasserin aut Enthalten in Bulletin of the Russian Academy of Sciences New York, NY : Allerton Press, 2007 73(2009), 3 vom: März, Seite 364-366 (DE-627)556723872 (DE-600)2403169-0 1934-9432 nnns volume:73 year:2009 number:3 month:03 pages:364-366 https://dx.doi.org/10.3103/S1062873809030253 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 73 2009 3 03 364-366 |
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Adriani, O. @@aut@@ Bazilevskaya, G. A. @@aut@@ Barbarino, G. C. @@aut@@ Bellotti, T. R. @@aut@@ Bzheumikhova, M. A. @@aut@@ Bogomolov, E. A. @@aut@@ Boezio, V. M. @@aut@@ Bonvicini, V. @@aut@@ Bongi, M. @@aut@@ Bonechi, L. @@aut@@ Bottai, S. @@aut@@ Bruno, A. @@aut@@ Vacchi, A. @@aut@@ Vannuccini, E. @@aut@@ Vasiliev, G. V. @@aut@@ Voronov, S. A. @@aut@@ Galper, A. M. @@aut@@ Grishantseva, L. A. @@aut@@ Zampa, G. @@aut@@ Zampa, N. @@aut@@ Zverev, V. G. @@aut@@ Casolino, M. @@aut@@ Campana, T. D. @@aut@@ Carlson, P. @@aut@@ Castellini, G. @@aut@@ Cafagna, F. @@aut@@ Kvashnin, A. N. @@aut@@ Koldashov, S. V. @@aut@@ Krutkov, S. Yu. @@aut@@ Leonov, A. A. @@aut@@ Malakhov, V. V. @@aut@@ Malvezzi, V. @@aut@@ Marcelli, L. @@aut@@ Menn, W. @@aut@@ Mikhailov, V. V. @@aut@@ Mocchiutti, E. @@aut@@ Orsi, S. @@aut@@ Osteria, G. @@aut@@ Papini, P. @@aut@@ De Pascale, M. P. @@aut@@ Picozza, T. P. @@aut@@ Pearce, M. @@aut@@ De Rosa, G. @@aut@@ Ricci, M. @@aut@@ Ricciarini, S. B. @@aut@@ Simon, M. @@aut@@ De Simone, N. @@aut@@ Sparvoli, R. @@aut@@ Spillantini, P. @@aut@@ Stozhkov, Yu. I. @@aut@@ Taddei, E. @@aut@@ Di Felice, V. @@aut@@ Fedele, D. @@aut@@ Hofverberg, P. @@aut@@ Yurkin, Yu. T. @@aut@@ |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">SPR023150785</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20220111100823.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">201006s2009 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.3103/S1062873809030253</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR023150785</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)S1062873809030253-e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">ASE</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">33.00</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Adriani, O.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Secondary electron and positron fluxes in the near-Earth space observed in the ARINA and PAMELA experiments</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2009</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Secondary electron and positron fluxes in the energy range from 3 MeV to 7 GeV were measured with the ARINA and PAMELA spectrometers onboard the Resurs-DK satellite launched on June 15, 2006 into an elliptical orbit with an inclination of 70.4° and an altitude of 350–600 km. It is shown that positrons dominate over electrons by a factor of up to 4–5 in the geomagnetic equator region (L < 1.2 and B > 0.25).</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Magnetic Anomaly</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Experimental Data Analysis</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">PAMELA Experiment</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Positron Flux</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Good Statistical Accuracy</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bazilevskaya, G. A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Barbarino, G. C.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bellotti, T. R.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bzheumikhova, M. A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bogomolov, E. A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Boezio, V. 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Adriani, O. ddc 530 bkl 33.00 misc Magnetic Anomaly misc Experimental Data Analysis misc PAMELA Experiment misc Positron Flux misc Good Statistical Accuracy Secondary electron and positron fluxes in the near-Earth space observed in the ARINA and PAMELA experiments |
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530 ASE 33.00 bkl Secondary electron and positron fluxes in the near-Earth space observed in the ARINA and PAMELA experiments Magnetic Anomaly (dpeaa)DE-He213 Experimental Data Analysis (dpeaa)DE-He213 PAMELA Experiment (dpeaa)DE-He213 Positron Flux (dpeaa)DE-He213 Good Statistical Accuracy (dpeaa)DE-He213 |
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Secondary electron and positron fluxes in the near-Earth space observed in the ARINA and PAMELA experiments |
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Secondary electron and positron fluxes in the near-Earth space observed in the ARINA and PAMELA experiments |
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Adriani, O. Bazilevskaya, G. A. Barbarino, G. C. Bellotti, T. R. Bzheumikhova, M. A. Bogomolov, E. A. Boezio, V. M. Bonvicini, V. Bongi, M. Bonechi, L. Bottai, S. Bruno, A. Vacchi, A. Vannuccini, E. Vasiliev, G. V. Voronov, S. A. Galper, A. M. Grishantseva, L. A. Zampa, G. Zampa, N. Zverev, V. G. Casolino, M. Campana, T. D. Carlson, P. Castellini, G. Cafagna, F. Kvashnin, A. N. Koldashov, S. V. Krutkov, S. Yu. Leonov, A. A. Malakhov, V. V. Malvezzi, V. Marcelli, L. Menn, W. Mikhailov, V. V. Mocchiutti, E. Orsi, S. Osteria, G. Papini, P. De Pascale, M. P. Picozza, T. P. Pearce, M. De Rosa, G. Ricci, M. Ricciarini, S. B. Simon, M. De Simone, N. Sparvoli, R. Spillantini, P. Stozhkov, Yu. I. Taddei, E. Di Felice, V. Fedele, D. Hofverberg, P. Yurkin, Yu. T. |
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secondary electron and positron fluxes in the near-earth space observed in the arina and pamela experiments |
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Secondary electron and positron fluxes in the near-Earth space observed in the ARINA and PAMELA experiments |
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Abstract Secondary electron and positron fluxes in the energy range from 3 MeV to 7 GeV were measured with the ARINA and PAMELA spectrometers onboard the Resurs-DK satellite launched on June 15, 2006 into an elliptical orbit with an inclination of 70.4° and an altitude of 350–600 km. It is shown that positrons dominate over electrons by a factor of up to 4–5 in the geomagnetic equator region (L < 1.2 and B > 0.25). |
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Abstract Secondary electron and positron fluxes in the energy range from 3 MeV to 7 GeV were measured with the ARINA and PAMELA spectrometers onboard the Resurs-DK satellite launched on June 15, 2006 into an elliptical orbit with an inclination of 70.4° and an altitude of 350–600 km. It is shown that positrons dominate over electrons by a factor of up to 4–5 in the geomagnetic equator region (L < 1.2 and B > 0.25). |
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Abstract Secondary electron and positron fluxes in the energy range from 3 MeV to 7 GeV were measured with the ARINA and PAMELA spectrometers onboard the Resurs-DK satellite launched on June 15, 2006 into an elliptical orbit with an inclination of 70.4° and an altitude of 350–600 km. It is shown that positrons dominate over electrons by a factor of up to 4–5 in the geomagnetic equator region (L < 1.2 and B > 0.25). |
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Secondary electron and positron fluxes in the near-Earth space observed in the ARINA and PAMELA experiments |
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Bazilevskaya, G. A. Barbarino, G. C. Bellotti, T. R. Bzheumikhova, M. A. Bogomolov, E. A. Boezio, V. M. Bonvicini, V. Bongi, M. Bonechi, L. Bottai, S. Bruno, A. Vacchi, A. Vannuccini, E. Vasiliev, G. V. Voronov, S. A. Galper, A. M. Grishantseva, L. A. Zampa, G. Zampa, N. Zverev, V. G. Casolino, M. Campana, T. D. Carlson, P. Castellini, G. Cafagna, F. Kvashnin, A. N. Koldashov, S. V. Krutkov, S. Yu Leonov, A. A. Malakhov, V. V. Malvezzi, V. Marcelli, L. Menn, W. Mikhailov, V. V. Mocchiutti, E. Orsi, S. Osteria, G. Papini, P. De Pascale, M. P. Picozza, T. P. Pearce, M. De Rosa, G. Ricci, M. Ricciarini, S. B. Simon, M. De Simone, N. Sparvoli, R. Spillantini, P. Stozhkov, Yu. I. Taddei, E. Di Felice, V. Fedele, D. Hofverberg, P. Yurkin, Yu. T. |
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| score |
7.3998604 |