Outer radiation belt of relativistic electrons during the minimum of the 23rd solar cycle
Abstract The data on fluxes of electrons with energy Ee > 1 MeV and on radiation doses under the Al shielding of about 2 g/$ cm^{2} $ measured on the GLONASS satellite (circular orbit with altitude 20000 km and inclination 65°) for the period from December 2006 through May 2010 are analyzed. The...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Tverskaya, L. V. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2012 |
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| Schlagwörter: |
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| Anmerkung: |
© Pleiades Publishing, Ltd. 2012 |
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| Übergeordnetes Werk: |
Enthalten in: Geomagnetism and aeronomy - Moscow : MAIK Nauka/Interperiodica Publ., 1996, 52(2012), 6 vom: Nov., Seite 740-745 |
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| Übergeordnetes Werk: |
volume:52 ; year:2012 ; number:6 ; month:11 ; pages:740-745 |
| Links: |
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| DOI / URN: |
10.1134/S0016793212060126 |
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| Katalog-ID: |
SPR019996411 |
|---|
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| 100 | 1 | |a Tverskaya, L. V. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Outer radiation belt of relativistic electrons during the minimum of the 23rd solar cycle |
| 264 | 1 | |c 2012 | |
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| 520 | |a Abstract The data on fluxes of electrons with energy Ee > 1 MeV and on radiation doses under the Al shielding of about 2 g/$ cm^{2} $ measured on the GLONASS satellite (circular orbit with altitude 20000 km and inclination 65°) for the period from December 2006 through May 2010 are analyzed. The minimum of the 23rd solar cycle turned out to be the longest for all over the space exploration age. Consequently, average semiannual electron fluxes and daily radiation doses are showing the decrease by more than an order of magnitude in comparison with the levels observed in 2007. We present an example of a diffusion wave of relativistic electrons; the wave develops in a period between magnetic storms. This process may result in a significant increase of the radiation dose measured in the orbit, even under the conditions of weak geomagnetic disturbances. The dynamics of variations in relativistic electron fluxes during the magnetic storm of April 5–6, 2010, is discussed so far as this is the first strong flux enhancement in the 24th solar cycle. | ||
| 650 | 4 | |a Solar Cycle |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Magnetic Storm |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Relativistic Electron |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Electron Flux |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Radiation Belt |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Balashov, S. V. |4 aut | |
| 700 | 1 | |a Veden’kin, N. N. |4 aut | |
| 700 | 1 | |a Ivanov, V. V. |4 aut | |
| 700 | 1 | |a Karpenko, D. S. |4 aut | |
| 700 | 1 | |a Kochura, S. G. |4 aut | |
| 700 | 1 | |a Maksimov, I. A. |4 aut | |
| 700 | 1 | |a Open’ko, S. I. |4 aut | |
| 700 | 1 | |a Pavlov, N. N. |4 aut | |
| 700 | 1 | |a Reizman, S. Ya. |4 aut | |
| 700 | 1 | |a Rubinshtein, I. A. |4 aut | |
| 700 | 1 | |a Sitnokova, N. N. |4 aut | |
| 700 | 1 | |a Tel’tsov, M. V. |4 aut | |
| 700 | 1 | |a Trofimchuk, D. A. |4 aut | |
| 700 | 1 | |a Tulupov, V. I. |4 aut | |
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| 773 | 1 | 8 | |g volume:52 |g year:2012 |g number:6 |g month:11 |g pages:740-745 |
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10.1134/S0016793212060126 doi (DE-627)SPR019996411 (SPR)S0016793212060126-e DE-627 ger DE-627 rakwb eng Tverskaya, L. V. verfasserin aut Outer radiation belt of relativistic electrons during the minimum of the 23rd solar cycle 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2012 Abstract The data on fluxes of electrons with energy Ee > 1 MeV and on radiation doses under the Al shielding of about 2 g/$ cm^{2} $ measured on the GLONASS satellite (circular orbit with altitude 20000 km and inclination 65°) for the period from December 2006 through May 2010 are analyzed. The minimum of the 23rd solar cycle turned out to be the longest for all over the space exploration age. Consequently, average semiannual electron fluxes and daily radiation doses are showing the decrease by more than an order of magnitude in comparison with the levels observed in 2007. We present an example of a diffusion wave of relativistic electrons; the wave develops in a period between magnetic storms. This process may result in a significant increase of the radiation dose measured in the orbit, even under the conditions of weak geomagnetic disturbances. The dynamics of variations in relativistic electron fluxes during the magnetic storm of April 5–6, 2010, is discussed so far as this is the first strong flux enhancement in the 24th solar cycle. Solar Cycle (dpeaa)DE-He213 Magnetic Storm (dpeaa)DE-He213 Relativistic Electron (dpeaa)DE-He213 Electron Flux (dpeaa)DE-He213 Radiation Belt (dpeaa)DE-He213 Balashov, S. V. aut Veden’kin, N. N. aut Ivanov, V. V. aut Karpenko, D. S. aut Kochura, S. G. aut Maksimov, I. A. aut Open’ko, S. I. aut Pavlov, N. N. aut Reizman, S. Ya. aut Rubinshtein, I. A. aut Sitnokova, N. N. aut Tel’tsov, M. V. aut Trofimchuk, D. A. aut Tulupov, V. I. aut Enthalten in Geomagnetism and aeronomy Moscow : MAIK Nauka/Interperiodica Publ., 1996 52(2012), 6 vom: Nov., Seite 740-745 (DE-627)342320920 (DE-600)2071667-9 1555-645X nnns volume:52 year:2012 number:6 month:11 pages:740-745 https://dx.doi.org/10.1134/S0016793212060126 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_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 AR 52 2012 6 11 740-745 |
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10.1134/S0016793212060126 doi (DE-627)SPR019996411 (SPR)S0016793212060126-e DE-627 ger DE-627 rakwb eng Tverskaya, L. V. verfasserin aut Outer radiation belt of relativistic electrons during the minimum of the 23rd solar cycle 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2012 Abstract The data on fluxes of electrons with energy Ee > 1 MeV and on radiation doses under the Al shielding of about 2 g/$ cm^{2} $ measured on the GLONASS satellite (circular orbit with altitude 20000 km and inclination 65°) for the period from December 2006 through May 2010 are analyzed. The minimum of the 23rd solar cycle turned out to be the longest for all over the space exploration age. Consequently, average semiannual electron fluxes and daily radiation doses are showing the decrease by more than an order of magnitude in comparison with the levels observed in 2007. We present an example of a diffusion wave of relativistic electrons; the wave develops in a period between magnetic storms. This process may result in a significant increase of the radiation dose measured in the orbit, even under the conditions of weak geomagnetic disturbances. The dynamics of variations in relativistic electron fluxes during the magnetic storm of April 5–6, 2010, is discussed so far as this is the first strong flux enhancement in the 24th solar cycle. Solar Cycle (dpeaa)DE-He213 Magnetic Storm (dpeaa)DE-He213 Relativistic Electron (dpeaa)DE-He213 Electron Flux (dpeaa)DE-He213 Radiation Belt (dpeaa)DE-He213 Balashov, S. V. aut Veden’kin, N. N. aut Ivanov, V. V. aut Karpenko, D. S. aut Kochura, S. G. aut Maksimov, I. A. aut Open’ko, S. I. aut Pavlov, N. N. aut Reizman, S. Ya. aut Rubinshtein, I. A. aut Sitnokova, N. N. aut Tel’tsov, M. V. aut Trofimchuk, D. A. aut Tulupov, V. I. aut Enthalten in Geomagnetism and aeronomy Moscow : MAIK Nauka/Interperiodica Publ., 1996 52(2012), 6 vom: Nov., Seite 740-745 (DE-627)342320920 (DE-600)2071667-9 1555-645X nnns volume:52 year:2012 number:6 month:11 pages:740-745 https://dx.doi.org/10.1134/S0016793212060126 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_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 AR 52 2012 6 11 740-745 |
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10.1134/S0016793212060126 doi (DE-627)SPR019996411 (SPR)S0016793212060126-e DE-627 ger DE-627 rakwb eng Tverskaya, L. V. verfasserin aut Outer radiation belt of relativistic electrons during the minimum of the 23rd solar cycle 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2012 Abstract The data on fluxes of electrons with energy Ee > 1 MeV and on radiation doses under the Al shielding of about 2 g/$ cm^{2} $ measured on the GLONASS satellite (circular orbit with altitude 20000 km and inclination 65°) for the period from December 2006 through May 2010 are analyzed. The minimum of the 23rd solar cycle turned out to be the longest for all over the space exploration age. Consequently, average semiannual electron fluxes and daily radiation doses are showing the decrease by more than an order of magnitude in comparison with the levels observed in 2007. We present an example of a diffusion wave of relativistic electrons; the wave develops in a period between magnetic storms. This process may result in a significant increase of the radiation dose measured in the orbit, even under the conditions of weak geomagnetic disturbances. The dynamics of variations in relativistic electron fluxes during the magnetic storm of April 5–6, 2010, is discussed so far as this is the first strong flux enhancement in the 24th solar cycle. Solar Cycle (dpeaa)DE-He213 Magnetic Storm (dpeaa)DE-He213 Relativistic Electron (dpeaa)DE-He213 Electron Flux (dpeaa)DE-He213 Radiation Belt (dpeaa)DE-He213 Balashov, S. V. aut Veden’kin, N. N. aut Ivanov, V. V. aut Karpenko, D. S. aut Kochura, S. G. aut Maksimov, I. A. aut Open’ko, S. I. aut Pavlov, N. N. aut Reizman, S. Ya. aut Rubinshtein, I. A. aut Sitnokova, N. N. aut Tel’tsov, M. V. aut Trofimchuk, D. A. aut Tulupov, V. I. aut Enthalten in Geomagnetism and aeronomy Moscow : MAIK Nauka/Interperiodica Publ., 1996 52(2012), 6 vom: Nov., Seite 740-745 (DE-627)342320920 (DE-600)2071667-9 1555-645X nnns volume:52 year:2012 number:6 month:11 pages:740-745 https://dx.doi.org/10.1134/S0016793212060126 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_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 AR 52 2012 6 11 740-745 |
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10.1134/S0016793212060126 doi (DE-627)SPR019996411 (SPR)S0016793212060126-e DE-627 ger DE-627 rakwb eng Tverskaya, L. V. verfasserin aut Outer radiation belt of relativistic electrons during the minimum of the 23rd solar cycle 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2012 Abstract The data on fluxes of electrons with energy Ee > 1 MeV and on radiation doses under the Al shielding of about 2 g/$ cm^{2} $ measured on the GLONASS satellite (circular orbit with altitude 20000 km and inclination 65°) for the period from December 2006 through May 2010 are analyzed. The minimum of the 23rd solar cycle turned out to be the longest for all over the space exploration age. Consequently, average semiannual electron fluxes and daily radiation doses are showing the decrease by more than an order of magnitude in comparison with the levels observed in 2007. We present an example of a diffusion wave of relativistic electrons; the wave develops in a period between magnetic storms. This process may result in a significant increase of the radiation dose measured in the orbit, even under the conditions of weak geomagnetic disturbances. The dynamics of variations in relativistic electron fluxes during the magnetic storm of April 5–6, 2010, is discussed so far as this is the first strong flux enhancement in the 24th solar cycle. Solar Cycle (dpeaa)DE-He213 Magnetic Storm (dpeaa)DE-He213 Relativistic Electron (dpeaa)DE-He213 Electron Flux (dpeaa)DE-He213 Radiation Belt (dpeaa)DE-He213 Balashov, S. V. aut Veden’kin, N. N. aut Ivanov, V. V. aut Karpenko, D. S. aut Kochura, S. G. aut Maksimov, I. A. aut Open’ko, S. I. aut Pavlov, N. N. aut Reizman, S. Ya. aut Rubinshtein, I. A. aut Sitnokova, N. N. aut Tel’tsov, M. V. aut Trofimchuk, D. A. aut Tulupov, V. I. aut Enthalten in Geomagnetism and aeronomy Moscow : MAIK Nauka/Interperiodica Publ., 1996 52(2012), 6 vom: Nov., Seite 740-745 (DE-627)342320920 (DE-600)2071667-9 1555-645X nnns volume:52 year:2012 number:6 month:11 pages:740-745 https://dx.doi.org/10.1134/S0016793212060126 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_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 AR 52 2012 6 11 740-745 |
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10.1134/S0016793212060126 doi (DE-627)SPR019996411 (SPR)S0016793212060126-e DE-627 ger DE-627 rakwb eng Tverskaya, L. V. verfasserin aut Outer radiation belt of relativistic electrons during the minimum of the 23rd solar cycle 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2012 Abstract The data on fluxes of electrons with energy Ee > 1 MeV and on radiation doses under the Al shielding of about 2 g/$ cm^{2} $ measured on the GLONASS satellite (circular orbit with altitude 20000 km and inclination 65°) for the period from December 2006 through May 2010 are analyzed. The minimum of the 23rd solar cycle turned out to be the longest for all over the space exploration age. Consequently, average semiannual electron fluxes and daily radiation doses are showing the decrease by more than an order of magnitude in comparison with the levels observed in 2007. We present an example of a diffusion wave of relativistic electrons; the wave develops in a period between magnetic storms. This process may result in a significant increase of the radiation dose measured in the orbit, even under the conditions of weak geomagnetic disturbances. The dynamics of variations in relativistic electron fluxes during the magnetic storm of April 5–6, 2010, is discussed so far as this is the first strong flux enhancement in the 24th solar cycle. Solar Cycle (dpeaa)DE-He213 Magnetic Storm (dpeaa)DE-He213 Relativistic Electron (dpeaa)DE-He213 Electron Flux (dpeaa)DE-He213 Radiation Belt (dpeaa)DE-He213 Balashov, S. V. aut Veden’kin, N. N. aut Ivanov, V. V. aut Karpenko, D. S. aut Kochura, S. G. aut Maksimov, I. A. aut Open’ko, S. I. aut Pavlov, N. N. aut Reizman, S. Ya. aut Rubinshtein, I. A. aut Sitnokova, N. N. aut Tel’tsov, M. V. aut Trofimchuk, D. A. aut Tulupov, V. I. aut Enthalten in Geomagnetism and aeronomy Moscow : MAIK Nauka/Interperiodica Publ., 1996 52(2012), 6 vom: Nov., Seite 740-745 (DE-627)342320920 (DE-600)2071667-9 1555-645X nnns volume:52 year:2012 number:6 month:11 pages:740-745 https://dx.doi.org/10.1134/S0016793212060126 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_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 AR 52 2012 6 11 740-745 |
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Enthalten in Geomagnetism and aeronomy 52(2012), 6 vom: Nov., Seite 740-745 volume:52 year:2012 number:6 month:11 pages:740-745 |
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Enthalten in Geomagnetism and aeronomy 52(2012), 6 vom: Nov., Seite 740-745 volume:52 year:2012 number:6 month:11 pages:740-745 |
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Tverskaya, L. V. @@aut@@ Balashov, S. V. @@aut@@ Veden’kin, N. N. @@aut@@ Ivanov, V. V. @@aut@@ Karpenko, D. S. @@aut@@ Kochura, S. G. @@aut@@ Maksimov, I. A. @@aut@@ Open’ko, S. I. @@aut@@ Pavlov, N. N. @@aut@@ Reizman, S. Ya. @@aut@@ Rubinshtein, I. A. @@aut@@ Sitnokova, N. N. @@aut@@ Tel’tsov, M. V. @@aut@@ Trofimchuk, D. A. @@aut@@ Tulupov, V. I. @@aut@@ |
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Tverskaya, L. V. |
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Tverskaya, L. V. misc Solar Cycle misc Magnetic Storm misc Relativistic Electron misc Electron Flux misc Radiation Belt Outer radiation belt of relativistic electrons during the minimum of the 23rd solar cycle |
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Outer radiation belt of relativistic electrons during the minimum of the 23rd solar cycle Solar Cycle (dpeaa)DE-He213 Magnetic Storm (dpeaa)DE-He213 Relativistic Electron (dpeaa)DE-He213 Electron Flux (dpeaa)DE-He213 Radiation Belt (dpeaa)DE-He213 |
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Outer radiation belt of relativistic electrons during the minimum of the 23rd solar cycle |
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Tverskaya, L. V. |
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Geomagnetism and aeronomy |
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Tverskaya, L. V. Balashov, S. V. Veden’kin, N. N. Ivanov, V. V. Karpenko, D. S. Kochura, S. G. Maksimov, I. A. Open’ko, S. I. Pavlov, N. N. Reizman, S. Ya. Rubinshtein, I. A. Sitnokova, N. N. Tel’tsov, M. V. Trofimchuk, D. A. Tulupov, V. I. |
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Elektronische Aufsätze |
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Tverskaya, L. V. |
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10.1134/S0016793212060126 |
| title_sort |
outer radiation belt of relativistic electrons during the minimum of the 23rd solar cycle |
| title_auth |
Outer radiation belt of relativistic electrons during the minimum of the 23rd solar cycle |
| abstract |
Abstract The data on fluxes of electrons with energy Ee > 1 MeV and on radiation doses under the Al shielding of about 2 g/$ cm^{2} $ measured on the GLONASS satellite (circular orbit with altitude 20000 km and inclination 65°) for the period from December 2006 through May 2010 are analyzed. The minimum of the 23rd solar cycle turned out to be the longest for all over the space exploration age. Consequently, average semiannual electron fluxes and daily radiation doses are showing the decrease by more than an order of magnitude in comparison with the levels observed in 2007. We present an example of a diffusion wave of relativistic electrons; the wave develops in a period between magnetic storms. This process may result in a significant increase of the radiation dose measured in the orbit, even under the conditions of weak geomagnetic disturbances. The dynamics of variations in relativistic electron fluxes during the magnetic storm of April 5–6, 2010, is discussed so far as this is the first strong flux enhancement in the 24th solar cycle. © Pleiades Publishing, Ltd. 2012 |
| abstractGer |
Abstract The data on fluxes of electrons with energy Ee > 1 MeV and on radiation doses under the Al shielding of about 2 g/$ cm^{2} $ measured on the GLONASS satellite (circular orbit with altitude 20000 km and inclination 65°) for the period from December 2006 through May 2010 are analyzed. The minimum of the 23rd solar cycle turned out to be the longest for all over the space exploration age. Consequently, average semiannual electron fluxes and daily radiation doses are showing the decrease by more than an order of magnitude in comparison with the levels observed in 2007. We present an example of a diffusion wave of relativistic electrons; the wave develops in a period between magnetic storms. This process may result in a significant increase of the radiation dose measured in the orbit, even under the conditions of weak geomagnetic disturbances. The dynamics of variations in relativistic electron fluxes during the magnetic storm of April 5–6, 2010, is discussed so far as this is the first strong flux enhancement in the 24th solar cycle. © Pleiades Publishing, Ltd. 2012 |
| abstract_unstemmed |
Abstract The data on fluxes of electrons with energy Ee > 1 MeV and on radiation doses under the Al shielding of about 2 g/$ cm^{2} $ measured on the GLONASS satellite (circular orbit with altitude 20000 km and inclination 65°) for the period from December 2006 through May 2010 are analyzed. The minimum of the 23rd solar cycle turned out to be the longest for all over the space exploration age. Consequently, average semiannual electron fluxes and daily radiation doses are showing the decrease by more than an order of magnitude in comparison with the levels observed in 2007. We present an example of a diffusion wave of relativistic electrons; the wave develops in a period between magnetic storms. This process may result in a significant increase of the radiation dose measured in the orbit, even under the conditions of weak geomagnetic disturbances. The dynamics of variations in relativistic electron fluxes during the magnetic storm of April 5–6, 2010, is discussed so far as this is the first strong flux enhancement in the 24th solar cycle. © Pleiades Publishing, Ltd. 2012 |
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6 |
| title_short |
Outer radiation belt of relativistic electrons during the minimum of the 23rd solar cycle |
| url |
https://dx.doi.org/10.1134/S0016793212060126 |
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| author2 |
Balashov, S. V. Veden’kin, N. N. Ivanov, V. V. Karpenko, D. S. Kochura, S. G. Maksimov, I. A. Open’ko, S. I. Pavlov, N. N. Reizman, S. Ya Rubinshtein, I. A. Sitnokova, N. N. Tel’tsov, M. V. Trofimchuk, D. A. Tulupov, V. I. |
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Balashov, S. V. Veden’kin, N. N. Ivanov, V. V. Karpenko, D. S. Kochura, S. G. Maksimov, I. A. Open’ko, S. I. Pavlov, N. N. Reizman, S. Ya Rubinshtein, I. A. Sitnokova, N. N. Tel’tsov, M. V. Trofimchuk, D. A. Tulupov, V. I. |
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10.1134/S0016793212060126 |
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2024-07-04T03:35:48.923Z |
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| score |
7.398264 |