The Relativistic Proton Spectrometer (RPS) for the Radiation Belt Storm Probes Mission
Abstract The Relativistic Proton Spectrometer (RPS) on the Radiation Belt Storm Probes spacecraft is a particle spectrometer designed to measure the flux, angular distribution, and energy spectrum of protons from ∼60 MeV to ∼2000 MeV. RPS will investigate decades-old questions about the inner Van Al...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Mazur, J. [verfasserIn] Friesen, L. [verfasserIn] Lin, A. [verfasserIn] Mabry, D. [verfasserIn] Katz, N. [verfasserIn] Dotan, Y. [verfasserIn] George, J. [verfasserIn] Blake, J. B. [verfasserIn] Looper, M. [verfasserIn] Redding, M. [verfasserIn] O’Brien, T. P. [verfasserIn] Cha, J. [verfasserIn] Birkitt, A. [verfasserIn] Carranza, P. [verfasserIn] Lalic, M. [verfasserIn] Fuentes, F. [verfasserIn] Galvan, R. [verfasserIn] McNab, M. [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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| Übergeordnetes Werk: |
Enthalten in: Space science reviews - Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962, 179(2012), 1-4 vom: 30. Aug., Seite 221-261 |
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| Übergeordnetes Werk: |
volume:179 ; year:2012 ; number:1-4 ; day:30 ; month:08 ; pages:221-261 |
| Links: |
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| DOI / URN: |
10.1007/s11214-012-9926-9 |
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| Katalog-ID: |
SPR017813344 |
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| 245 | 1 | 4 | |a The Relativistic Proton Spectrometer (RPS) for the Radiation Belt Storm Probes Mission |
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| 520 | |a Abstract The Relativistic Proton Spectrometer (RPS) on the Radiation Belt Storm Probes spacecraft is a particle spectrometer designed to measure the flux, angular distribution, and energy spectrum of protons from ∼60 MeV to ∼2000 MeV. RPS will investigate decades-old questions about the inner Van Allen belt proton environment: a nearby region of space that is relatively unexplored because of the hazards of spacecraft operation there and the difficulties in obtaining accurate proton measurements in an intense penetrating background. RPS is designed to provide the accuracy needed to answer questions about the sources and losses of the inner belt protons and to obtain the measurements required for the next-generation models of trapped protons in the magnetosphere. In addition to detailed information for individual protons, RPS features count rates at a 1-second timescale, internal radiation dosimetry, and information about electrostatic discharge events on the RBSP spacecraft that together will provide new information about space environmental hazards in the Earth’s magnetosphere. | ||
| 650 | 4 | |a RBSP |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Inner radiation belt |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a CRAND |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Trapped protons |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Solar energetic protons |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Total ionizing dose |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Relativistic protons |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Friesen, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Lin, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Mabry, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Katz, N. |e verfasserin |4 aut | |
| 700 | 1 | |a Dotan, Y. |e verfasserin |4 aut | |
| 700 | 1 | |a George, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Blake, J. B. |e verfasserin |4 aut | |
| 700 | 1 | |a Looper, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Redding, M. |e verfasserin |4 aut | |
| 700 | 1 | |a O’Brien, T. P. |e verfasserin |4 aut | |
| 700 | 1 | |a Cha, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Birkitt, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Carranza, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Lalic, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Fuentes, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Galvan, R. |e verfasserin |4 aut | |
| 700 | 1 | |a McNab, M. |e verfasserin |4 aut | |
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10.1007/s11214-012-9926-9 doi (DE-627)SPR017813344 (SPR)s11214-012-9926-9-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Mazur, J. verfasserin aut The Relativistic Proton Spectrometer (RPS) for the Radiation Belt Storm Probes Mission 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The Relativistic Proton Spectrometer (RPS) on the Radiation Belt Storm Probes spacecraft is a particle spectrometer designed to measure the flux, angular distribution, and energy spectrum of protons from ∼60 MeV to ∼2000 MeV. RPS will investigate decades-old questions about the inner Van Allen belt proton environment: a nearby region of space that is relatively unexplored because of the hazards of spacecraft operation there and the difficulties in obtaining accurate proton measurements in an intense penetrating background. RPS is designed to provide the accuracy needed to answer questions about the sources and losses of the inner belt protons and to obtain the measurements required for the next-generation models of trapped protons in the magnetosphere. In addition to detailed information for individual protons, RPS features count rates at a 1-second timescale, internal radiation dosimetry, and information about electrostatic discharge events on the RBSP spacecraft that together will provide new information about space environmental hazards in the Earth’s magnetosphere. RBSP (dpeaa)DE-He213 Inner radiation belt (dpeaa)DE-He213 CRAND (dpeaa)DE-He213 Trapped protons (dpeaa)DE-He213 Solar energetic protons (dpeaa)DE-He213 Total ionizing dose (dpeaa)DE-He213 Relativistic protons (dpeaa)DE-He213 Friesen, L. verfasserin aut Lin, A. verfasserin aut Mabry, D. verfasserin aut Katz, N. verfasserin aut Dotan, Y. verfasserin aut George, J. verfasserin aut Blake, J. B. verfasserin aut Looper, M. verfasserin aut Redding, M. verfasserin aut O’Brien, T. P. verfasserin aut Cha, J. verfasserin aut Birkitt, A. verfasserin aut Carranza, P. verfasserin aut Lalic, M. verfasserin aut Fuentes, F. verfasserin aut Galvan, R. verfasserin aut McNab, M. verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 179(2012), 1-4 vom: 30. Aug., Seite 221-261 (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:179 year:2012 number:1-4 day:30 month:08 pages:221-261 https://dx.doi.org/10.1007/s11214-012-9926-9 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE 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_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_206 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_2056 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 39.00 ASE AR 179 2012 1-4 30 08 221-261 |
| spelling |
10.1007/s11214-012-9926-9 doi (DE-627)SPR017813344 (SPR)s11214-012-9926-9-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Mazur, J. verfasserin aut The Relativistic Proton Spectrometer (RPS) for the Radiation Belt Storm Probes Mission 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The Relativistic Proton Spectrometer (RPS) on the Radiation Belt Storm Probes spacecraft is a particle spectrometer designed to measure the flux, angular distribution, and energy spectrum of protons from ∼60 MeV to ∼2000 MeV. RPS will investigate decades-old questions about the inner Van Allen belt proton environment: a nearby region of space that is relatively unexplored because of the hazards of spacecraft operation there and the difficulties in obtaining accurate proton measurements in an intense penetrating background. RPS is designed to provide the accuracy needed to answer questions about the sources and losses of the inner belt protons and to obtain the measurements required for the next-generation models of trapped protons in the magnetosphere. In addition to detailed information for individual protons, RPS features count rates at a 1-second timescale, internal radiation dosimetry, and information about electrostatic discharge events on the RBSP spacecraft that together will provide new information about space environmental hazards in the Earth’s magnetosphere. RBSP (dpeaa)DE-He213 Inner radiation belt (dpeaa)DE-He213 CRAND (dpeaa)DE-He213 Trapped protons (dpeaa)DE-He213 Solar energetic protons (dpeaa)DE-He213 Total ionizing dose (dpeaa)DE-He213 Relativistic protons (dpeaa)DE-He213 Friesen, L. verfasserin aut Lin, A. verfasserin aut Mabry, D. verfasserin aut Katz, N. verfasserin aut Dotan, Y. verfasserin aut George, J. verfasserin aut Blake, J. B. verfasserin aut Looper, M. verfasserin aut Redding, M. verfasserin aut O’Brien, T. P. verfasserin aut Cha, J. verfasserin aut Birkitt, A. verfasserin aut Carranza, P. verfasserin aut Lalic, M. verfasserin aut Fuentes, F. verfasserin aut Galvan, R. verfasserin aut McNab, M. verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 179(2012), 1-4 vom: 30. Aug., Seite 221-261 (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:179 year:2012 number:1-4 day:30 month:08 pages:221-261 https://dx.doi.org/10.1007/s11214-012-9926-9 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE 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_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_206 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_2056 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 39.00 ASE AR 179 2012 1-4 30 08 221-261 |
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10.1007/s11214-012-9926-9 doi (DE-627)SPR017813344 (SPR)s11214-012-9926-9-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Mazur, J. verfasserin aut The Relativistic Proton Spectrometer (RPS) for the Radiation Belt Storm Probes Mission 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The Relativistic Proton Spectrometer (RPS) on the Radiation Belt Storm Probes spacecraft is a particle spectrometer designed to measure the flux, angular distribution, and energy spectrum of protons from ∼60 MeV to ∼2000 MeV. RPS will investigate decades-old questions about the inner Van Allen belt proton environment: a nearby region of space that is relatively unexplored because of the hazards of spacecraft operation there and the difficulties in obtaining accurate proton measurements in an intense penetrating background. RPS is designed to provide the accuracy needed to answer questions about the sources and losses of the inner belt protons and to obtain the measurements required for the next-generation models of trapped protons in the magnetosphere. In addition to detailed information for individual protons, RPS features count rates at a 1-second timescale, internal radiation dosimetry, and information about electrostatic discharge events on the RBSP spacecraft that together will provide new information about space environmental hazards in the Earth’s magnetosphere. RBSP (dpeaa)DE-He213 Inner radiation belt (dpeaa)DE-He213 CRAND (dpeaa)DE-He213 Trapped protons (dpeaa)DE-He213 Solar energetic protons (dpeaa)DE-He213 Total ionizing dose (dpeaa)DE-He213 Relativistic protons (dpeaa)DE-He213 Friesen, L. verfasserin aut Lin, A. verfasserin aut Mabry, D. verfasserin aut Katz, N. verfasserin aut Dotan, Y. verfasserin aut George, J. verfasserin aut Blake, J. B. verfasserin aut Looper, M. verfasserin aut Redding, M. verfasserin aut O’Brien, T. P. verfasserin aut Cha, J. verfasserin aut Birkitt, A. verfasserin aut Carranza, P. verfasserin aut Lalic, M. verfasserin aut Fuentes, F. verfasserin aut Galvan, R. verfasserin aut McNab, M. verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 179(2012), 1-4 vom: 30. Aug., Seite 221-261 (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:179 year:2012 number:1-4 day:30 month:08 pages:221-261 https://dx.doi.org/10.1007/s11214-012-9926-9 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE 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_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_206 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_2056 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 39.00 ASE AR 179 2012 1-4 30 08 221-261 |
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10.1007/s11214-012-9926-9 doi (DE-627)SPR017813344 (SPR)s11214-012-9926-9-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Mazur, J. verfasserin aut The Relativistic Proton Spectrometer (RPS) for the Radiation Belt Storm Probes Mission 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The Relativistic Proton Spectrometer (RPS) on the Radiation Belt Storm Probes spacecraft is a particle spectrometer designed to measure the flux, angular distribution, and energy spectrum of protons from ∼60 MeV to ∼2000 MeV. RPS will investigate decades-old questions about the inner Van Allen belt proton environment: a nearby region of space that is relatively unexplored because of the hazards of spacecraft operation there and the difficulties in obtaining accurate proton measurements in an intense penetrating background. RPS is designed to provide the accuracy needed to answer questions about the sources and losses of the inner belt protons and to obtain the measurements required for the next-generation models of trapped protons in the magnetosphere. In addition to detailed information for individual protons, RPS features count rates at a 1-second timescale, internal radiation dosimetry, and information about electrostatic discharge events on the RBSP spacecraft that together will provide new information about space environmental hazards in the Earth’s magnetosphere. RBSP (dpeaa)DE-He213 Inner radiation belt (dpeaa)DE-He213 CRAND (dpeaa)DE-He213 Trapped protons (dpeaa)DE-He213 Solar energetic protons (dpeaa)DE-He213 Total ionizing dose (dpeaa)DE-He213 Relativistic protons (dpeaa)DE-He213 Friesen, L. verfasserin aut Lin, A. verfasserin aut Mabry, D. verfasserin aut Katz, N. verfasserin aut Dotan, Y. verfasserin aut George, J. verfasserin aut Blake, J. B. verfasserin aut Looper, M. verfasserin aut Redding, M. verfasserin aut O’Brien, T. P. verfasserin aut Cha, J. verfasserin aut Birkitt, A. verfasserin aut Carranza, P. verfasserin aut Lalic, M. verfasserin aut Fuentes, F. verfasserin aut Galvan, R. verfasserin aut McNab, M. verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 179(2012), 1-4 vom: 30. Aug., Seite 221-261 (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:179 year:2012 number:1-4 day:30 month:08 pages:221-261 https://dx.doi.org/10.1007/s11214-012-9926-9 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE 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_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_206 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_2056 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 39.00 ASE AR 179 2012 1-4 30 08 221-261 |
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10.1007/s11214-012-9926-9 doi (DE-627)SPR017813344 (SPR)s11214-012-9926-9-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Mazur, J. verfasserin aut The Relativistic Proton Spectrometer (RPS) for the Radiation Belt Storm Probes Mission 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The Relativistic Proton Spectrometer (RPS) on the Radiation Belt Storm Probes spacecraft is a particle spectrometer designed to measure the flux, angular distribution, and energy spectrum of protons from ∼60 MeV to ∼2000 MeV. RPS will investigate decades-old questions about the inner Van Allen belt proton environment: a nearby region of space that is relatively unexplored because of the hazards of spacecraft operation there and the difficulties in obtaining accurate proton measurements in an intense penetrating background. RPS is designed to provide the accuracy needed to answer questions about the sources and losses of the inner belt protons and to obtain the measurements required for the next-generation models of trapped protons in the magnetosphere. In addition to detailed information for individual protons, RPS features count rates at a 1-second timescale, internal radiation dosimetry, and information about electrostatic discharge events on the RBSP spacecraft that together will provide new information about space environmental hazards in the Earth’s magnetosphere. RBSP (dpeaa)DE-He213 Inner radiation belt (dpeaa)DE-He213 CRAND (dpeaa)DE-He213 Trapped protons (dpeaa)DE-He213 Solar energetic protons (dpeaa)DE-He213 Total ionizing dose (dpeaa)DE-He213 Relativistic protons (dpeaa)DE-He213 Friesen, L. verfasserin aut Lin, A. verfasserin aut Mabry, D. verfasserin aut Katz, N. verfasserin aut Dotan, Y. verfasserin aut George, J. verfasserin aut Blake, J. B. verfasserin aut Looper, M. verfasserin aut Redding, M. verfasserin aut O’Brien, T. P. verfasserin aut Cha, J. verfasserin aut Birkitt, A. verfasserin aut Carranza, P. verfasserin aut Lalic, M. verfasserin aut Fuentes, F. verfasserin aut Galvan, R. verfasserin aut McNab, M. verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 179(2012), 1-4 vom: 30. Aug., Seite 221-261 (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:179 year:2012 number:1-4 day:30 month:08 pages:221-261 https://dx.doi.org/10.1007/s11214-012-9926-9 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE 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_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_206 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_2056 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 39.00 ASE AR 179 2012 1-4 30 08 221-261 |
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Enthalten in Space science reviews 179(2012), 1-4 vom: 30. Aug., Seite 221-261 volume:179 year:2012 number:1-4 day:30 month:08 pages:221-261 |
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RBSP Inner radiation belt CRAND Trapped protons Solar energetic protons Total ionizing dose Relativistic protons |
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Mazur, J. @@aut@@ Friesen, L. @@aut@@ Lin, A. @@aut@@ Mabry, D. @@aut@@ Katz, N. @@aut@@ Dotan, Y. @@aut@@ George, J. @@aut@@ Blake, J. B. @@aut@@ Looper, M. @@aut@@ Redding, M. @@aut@@ O’Brien, T. P. @@aut@@ Cha, J. @@aut@@ Birkitt, A. @@aut@@ Carranza, P. @@aut@@ Lalic, M. @@aut@@ Fuentes, F. @@aut@@ Galvan, R. @@aut@@ McNab, M. @@aut@@ |
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RPS will investigate decades-old questions about the inner Van Allen belt proton environment: a nearby region of space that is relatively unexplored because of the hazards of spacecraft operation there and the difficulties in obtaining accurate proton measurements in an intense penetrating background. RPS is designed to provide the accuracy needed to answer questions about the sources and losses of the inner belt protons and to obtain the measurements required for the next-generation models of trapped protons in the magnetosphere. 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|
| author |
Mazur, J. |
| spellingShingle |
Mazur, J. ddc 600 bkl 39.00 misc RBSP misc Inner radiation belt misc CRAND misc Trapped protons misc Solar energetic protons misc Total ionizing dose misc Relativistic protons The Relativistic Proton Spectrometer (RPS) for the Radiation Belt Storm Probes Mission |
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Mazur, J. |
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electronic Article |
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600 - Technology |
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keep |
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aut aut aut aut aut aut aut aut aut aut aut aut aut aut aut aut aut aut |
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springer |
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true |
| illustrated |
Not Illustrated |
| issn |
1572-9672 |
| topic_title |
600 ASE 39.00 bkl The Relativistic Proton Spectrometer (RPS) for the Radiation Belt Storm Probes Mission RBSP (dpeaa)DE-He213 Inner radiation belt (dpeaa)DE-He213 CRAND (dpeaa)DE-He213 Trapped protons (dpeaa)DE-He213 Solar energetic protons (dpeaa)DE-He213 Total ionizing dose (dpeaa)DE-He213 Relativistic protons (dpeaa)DE-He213 |
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The Relativistic Proton Spectrometer (RPS) for the Radiation Belt Storm Probes Mission |
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Mazur, J. Friesen, L. Lin, A. Mabry, D. Katz, N. Dotan, Y. George, J. Blake, J. B. Looper, M. Redding, M. O’Brien, T. P. Cha, J. Birkitt, A. Carranza, P. Lalic, M. Fuentes, F. Galvan, R. McNab, M. |
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The Relativistic Proton Spectrometer (RPS) for the Radiation Belt Storm Probes Mission |
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Abstract The Relativistic Proton Spectrometer (RPS) on the Radiation Belt Storm Probes spacecraft is a particle spectrometer designed to measure the flux, angular distribution, and energy spectrum of protons from ∼60 MeV to ∼2000 MeV. RPS will investigate decades-old questions about the inner Van Allen belt proton environment: a nearby region of space that is relatively unexplored because of the hazards of spacecraft operation there and the difficulties in obtaining accurate proton measurements in an intense penetrating background. RPS is designed to provide the accuracy needed to answer questions about the sources and losses of the inner belt protons and to obtain the measurements required for the next-generation models of trapped protons in the magnetosphere. In addition to detailed information for individual protons, RPS features count rates at a 1-second timescale, internal radiation dosimetry, and information about electrostatic discharge events on the RBSP spacecraft that together will provide new information about space environmental hazards in the Earth’s magnetosphere. |
| abstractGer |
Abstract The Relativistic Proton Spectrometer (RPS) on the Radiation Belt Storm Probes spacecraft is a particle spectrometer designed to measure the flux, angular distribution, and energy spectrum of protons from ∼60 MeV to ∼2000 MeV. RPS will investigate decades-old questions about the inner Van Allen belt proton environment: a nearby region of space that is relatively unexplored because of the hazards of spacecraft operation there and the difficulties in obtaining accurate proton measurements in an intense penetrating background. RPS is designed to provide the accuracy needed to answer questions about the sources and losses of the inner belt protons and to obtain the measurements required for the next-generation models of trapped protons in the magnetosphere. In addition to detailed information for individual protons, RPS features count rates at a 1-second timescale, internal radiation dosimetry, and information about electrostatic discharge events on the RBSP spacecraft that together will provide new information about space environmental hazards in the Earth’s magnetosphere. |
| abstract_unstemmed |
Abstract The Relativistic Proton Spectrometer (RPS) on the Radiation Belt Storm Probes spacecraft is a particle spectrometer designed to measure the flux, angular distribution, and energy spectrum of protons from ∼60 MeV to ∼2000 MeV. RPS will investigate decades-old questions about the inner Van Allen belt proton environment: a nearby region of space that is relatively unexplored because of the hazards of spacecraft operation there and the difficulties in obtaining accurate proton measurements in an intense penetrating background. RPS is designed to provide the accuracy needed to answer questions about the sources and losses of the inner belt protons and to obtain the measurements required for the next-generation models of trapped protons in the magnetosphere. In addition to detailed information for individual protons, RPS features count rates at a 1-second timescale, internal radiation dosimetry, and information about electrostatic discharge events on the RBSP spacecraft that together will provide new information about space environmental hazards in the Earth’s magnetosphere. |
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| score |
7.401865 |