Dependence of Energetic Electron Precipitation on the Geomagnetic Index Kp and Electron Energy

It has long been known that the magnetospheric particles can precipitate into the atmosphere of the Earth. In this paper we examine such precipitation of energetic electrons using the data obtained from low-altitude polar orbiting satellite observations. We analyze the precipitating electron flux da...
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Gespeichert in:

Autor*in:	Mi-Young Park [verfasserIn] Dae-Young Lee [verfasserIn] Dae-Kyu Shin [verfasserIn] Jung-Hee Cho [verfasserIn] Eun-Hee Lee [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2013

Schlagwörter:	energetic electrons particle precipitation radiation belts

Übergeordnetes Werk:	In: Journal of Astronomy and Space Sciences - Korean Space Science Society (KSSS), 2012, 30(2013), 4, Seite 247-253
Übergeordnetes Werk:	volume:30 ; year:2013 ; number:4 ; pages:247-253

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc Journal toc

DOI / URN:	10.5140/JASS.2013.30.4.247

Katalog-ID:	DOAJ054544831

Internformat


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520			\|a It has long been known that the magnetospheric particles can precipitate into the atmosphere of the Earth. In this paper we examine such precipitation of energetic electrons using the data obtained from low-altitude polar orbiting satellite observations. We analyze the precipitating electron flux data for many periods selected from a total of 84 storm events identified for 2001-2012. The analysis includes the dependence of precipitation on the Kp index and the electron energy, for which we use three energies E1 < 30 keV, E2 < 100 keV, E3 < 300 keV. We find that the precipitation is best correlated with Kp after a time delay of < 3 hours. Most importantly, the correlation with Kp is notably tighter for lower energy than for higher energy in the sense that the lower energy precipitation flux increases more rapidly with Kp than does the higher energy precipitation flux. Based on this we suggest that the Kp index reflects excitation of a wave that is responsible for scattering of preferably lower energy electrons. The role of waves of other types should become increasingly important for higher energy, for which we suggest to rely on other indicators than Kp if one can identify such an indicator.
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allfields	10.5140/JASS.2013.30.4.247 doi (DE-627)DOAJ054544831 (DE-599)DOAJ73a8d029db6440b2ad624b3a0be8af1b DE-627 ger DE-627 rakwb eng QB1-991 Mi-Young Park verfasserin aut Dependence of Energetic Electron Precipitation on the Geomagnetic Index Kp and Electron Energy 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier It has long been known that the magnetospheric particles can precipitate into the atmosphere of the Earth. In this paper we examine such precipitation of energetic electrons using the data obtained from low-altitude polar orbiting satellite observations. We analyze the precipitating electron flux data for many periods selected from a total of 84 storm events identified for 2001-2012. The analysis includes the dependence of precipitation on the Kp index and the electron energy, for which we use three energies E1 < 30 keV, E2 < 100 keV, E3 < 300 keV. We find that the precipitation is best correlated with Kp after a time delay of < 3 hours. Most importantly, the correlation with Kp is notably tighter for lower energy than for higher energy in the sense that the lower energy precipitation flux increases more rapidly with Kp than does the higher energy precipitation flux. Based on this we suggest that the Kp index reflects excitation of a wave that is responsible for scattering of preferably lower energy electrons. The role of waves of other types should become increasingly important for higher energy, for which we suggest to rely on other indicators than Kp if one can identify such an indicator. energetic electrons particle precipitation radiation belts Astronomy Dae-Young Lee verfasserin aut Dae-Kyu Shin verfasserin aut Jung-Hee Cho verfasserin aut Eun-Hee Lee verfasserin aut In Journal of Astronomy and Space Sciences Korean Space Science Society (KSSS), 2012 30(2013), 4, Seite 247-253 (DE-627)62761471X (DE-600)2557343-3 20931409 nnns volume:30 year:2013 number:4 pages:247-253 https://doi.org/10.5140/JASS.2013.30.4.247 kostenfrei https://doaj.org/article/73a8d029db6440b2ad624b3a0be8af1b kostenfrei http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2013/v30n4/OJOOBS_2013_v30n4_247.pdf kostenfrei https://doaj.org/toc/2093-5587 Journal toc kostenfrei https://doaj.org/toc/2093-1409 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 30 2013 4 247-253
spelling	10.5140/JASS.2013.30.4.247 doi (DE-627)DOAJ054544831 (DE-599)DOAJ73a8d029db6440b2ad624b3a0be8af1b DE-627 ger DE-627 rakwb eng QB1-991 Mi-Young Park verfasserin aut Dependence of Energetic Electron Precipitation on the Geomagnetic Index Kp and Electron Energy 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier It has long been known that the magnetospheric particles can precipitate into the atmosphere of the Earth. In this paper we examine such precipitation of energetic electrons using the data obtained from low-altitude polar orbiting satellite observations. We analyze the precipitating electron flux data for many periods selected from a total of 84 storm events identified for 2001-2012. The analysis includes the dependence of precipitation on the Kp index and the electron energy, for which we use three energies E1 < 30 keV, E2 < 100 keV, E3 < 300 keV. We find that the precipitation is best correlated with Kp after a time delay of < 3 hours. Most importantly, the correlation with Kp is notably tighter for lower energy than for higher energy in the sense that the lower energy precipitation flux increases more rapidly with Kp than does the higher energy precipitation flux. Based on this we suggest that the Kp index reflects excitation of a wave that is responsible for scattering of preferably lower energy electrons. The role of waves of other types should become increasingly important for higher energy, for which we suggest to rely on other indicators than Kp if one can identify such an indicator. energetic electrons particle precipitation radiation belts Astronomy Dae-Young Lee verfasserin aut Dae-Kyu Shin verfasserin aut Jung-Hee Cho verfasserin aut Eun-Hee Lee verfasserin aut In Journal of Astronomy and Space Sciences Korean Space Science Society (KSSS), 2012 30(2013), 4, Seite 247-253 (DE-627)62761471X (DE-600)2557343-3 20931409 nnns volume:30 year:2013 number:4 pages:247-253 https://doi.org/10.5140/JASS.2013.30.4.247 kostenfrei https://doaj.org/article/73a8d029db6440b2ad624b3a0be8af1b kostenfrei http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2013/v30n4/OJOOBS_2013_v30n4_247.pdf kostenfrei https://doaj.org/toc/2093-5587 Journal toc kostenfrei https://doaj.org/toc/2093-1409 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 30 2013 4 247-253
allfields_unstemmed	10.5140/JASS.2013.30.4.247 doi (DE-627)DOAJ054544831 (DE-599)DOAJ73a8d029db6440b2ad624b3a0be8af1b DE-627 ger DE-627 rakwb eng QB1-991 Mi-Young Park verfasserin aut Dependence of Energetic Electron Precipitation on the Geomagnetic Index Kp and Electron Energy 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier It has long been known that the magnetospheric particles can precipitate into the atmosphere of the Earth. In this paper we examine such precipitation of energetic electrons using the data obtained from low-altitude polar orbiting satellite observations. We analyze the precipitating electron flux data for many periods selected from a total of 84 storm events identified for 2001-2012. The analysis includes the dependence of precipitation on the Kp index and the electron energy, for which we use three energies E1 < 30 keV, E2 < 100 keV, E3 < 300 keV. We find that the precipitation is best correlated with Kp after a time delay of < 3 hours. Most importantly, the correlation with Kp is notably tighter for lower energy than for higher energy in the sense that the lower energy precipitation flux increases more rapidly with Kp than does the higher energy precipitation flux. Based on this we suggest that the Kp index reflects excitation of a wave that is responsible for scattering of preferably lower energy electrons. The role of waves of other types should become increasingly important for higher energy, for which we suggest to rely on other indicators than Kp if one can identify such an indicator. energetic electrons particle precipitation radiation belts Astronomy Dae-Young Lee verfasserin aut Dae-Kyu Shin verfasserin aut Jung-Hee Cho verfasserin aut Eun-Hee Lee verfasserin aut In Journal of Astronomy and Space Sciences Korean Space Science Society (KSSS), 2012 30(2013), 4, Seite 247-253 (DE-627)62761471X (DE-600)2557343-3 20931409 nnns volume:30 year:2013 number:4 pages:247-253 https://doi.org/10.5140/JASS.2013.30.4.247 kostenfrei https://doaj.org/article/73a8d029db6440b2ad624b3a0be8af1b kostenfrei http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2013/v30n4/OJOOBS_2013_v30n4_247.pdf kostenfrei https://doaj.org/toc/2093-5587 Journal toc kostenfrei https://doaj.org/toc/2093-1409 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 30 2013 4 247-253
allfieldsGer	10.5140/JASS.2013.30.4.247 doi (DE-627)DOAJ054544831 (DE-599)DOAJ73a8d029db6440b2ad624b3a0be8af1b DE-627 ger DE-627 rakwb eng QB1-991 Mi-Young Park verfasserin aut Dependence of Energetic Electron Precipitation on the Geomagnetic Index Kp and Electron Energy 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier It has long been known that the magnetospheric particles can precipitate into the atmosphere of the Earth. In this paper we examine such precipitation of energetic electrons using the data obtained from low-altitude polar orbiting satellite observations. We analyze the precipitating electron flux data for many periods selected from a total of 84 storm events identified for 2001-2012. The analysis includes the dependence of precipitation on the Kp index and the electron energy, for which we use three energies E1 < 30 keV, E2 < 100 keV, E3 < 300 keV. We find that the precipitation is best correlated with Kp after a time delay of < 3 hours. Most importantly, the correlation with Kp is notably tighter for lower energy than for higher energy in the sense that the lower energy precipitation flux increases more rapidly with Kp than does the higher energy precipitation flux. Based on this we suggest that the Kp index reflects excitation of a wave that is responsible for scattering of preferably lower energy electrons. The role of waves of other types should become increasingly important for higher energy, for which we suggest to rely on other indicators than Kp if one can identify such an indicator. energetic electrons particle precipitation radiation belts Astronomy Dae-Young Lee verfasserin aut Dae-Kyu Shin verfasserin aut Jung-Hee Cho verfasserin aut Eun-Hee Lee verfasserin aut In Journal of Astronomy and Space Sciences Korean Space Science Society (KSSS), 2012 30(2013), 4, Seite 247-253 (DE-627)62761471X (DE-600)2557343-3 20931409 nnns volume:30 year:2013 number:4 pages:247-253 https://doi.org/10.5140/JASS.2013.30.4.247 kostenfrei https://doaj.org/article/73a8d029db6440b2ad624b3a0be8af1b kostenfrei http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2013/v30n4/OJOOBS_2013_v30n4_247.pdf kostenfrei https://doaj.org/toc/2093-5587 Journal toc kostenfrei https://doaj.org/toc/2093-1409 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 30 2013 4 247-253
allfieldsSound	10.5140/JASS.2013.30.4.247 doi (DE-627)DOAJ054544831 (DE-599)DOAJ73a8d029db6440b2ad624b3a0be8af1b DE-627 ger DE-627 rakwb eng QB1-991 Mi-Young Park verfasserin aut Dependence of Energetic Electron Precipitation on the Geomagnetic Index Kp and Electron Energy 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier It has long been known that the magnetospheric particles can precipitate into the atmosphere of the Earth. In this paper we examine such precipitation of energetic electrons using the data obtained from low-altitude polar orbiting satellite observations. We analyze the precipitating electron flux data for many periods selected from a total of 84 storm events identified for 2001-2012. The analysis includes the dependence of precipitation on the Kp index and the electron energy, for which we use three energies E1 < 30 keV, E2 < 100 keV, E3 < 300 keV. We find that the precipitation is best correlated with Kp after a time delay of < 3 hours. Most importantly, the correlation with Kp is notably tighter for lower energy than for higher energy in the sense that the lower energy precipitation flux increases more rapidly with Kp than does the higher energy precipitation flux. Based on this we suggest that the Kp index reflects excitation of a wave that is responsible for scattering of preferably lower energy electrons. The role of waves of other types should become increasingly important for higher energy, for which we suggest to rely on other indicators than Kp if one can identify such an indicator. energetic electrons particle precipitation radiation belts Astronomy Dae-Young Lee verfasserin aut Dae-Kyu Shin verfasserin aut Jung-Hee Cho verfasserin aut Eun-Hee Lee verfasserin aut In Journal of Astronomy and Space Sciences Korean Space Science Society (KSSS), 2012 30(2013), 4, Seite 247-253 (DE-627)62761471X (DE-600)2557343-3 20931409 nnns volume:30 year:2013 number:4 pages:247-253 https://doi.org/10.5140/JASS.2013.30.4.247 kostenfrei https://doaj.org/article/73a8d029db6440b2ad624b3a0be8af1b kostenfrei http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2013/v30n4/OJOOBS_2013_v30n4_247.pdf kostenfrei https://doaj.org/toc/2093-5587 Journal toc kostenfrei https://doaj.org/toc/2093-1409 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 30 2013 4 247-253
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source	In Journal of Astronomy and Space Sciences 30(2013), 4, Seite 247-253 volume:30 year:2013 number:4 pages:247-253
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callnumber-first	Q - Science
author	Mi-Young Park
spellingShingle	Mi-Young Park misc QB1-991 misc energetic electrons misc particle precipitation misc radiation belts misc Astronomy Dependence of Energetic Electron Precipitation on the Geomagnetic Index Kp and Electron Energy
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topic_title	QB1-991 Dependence of Energetic Electron Precipitation on the Geomagnetic Index Kp and Electron Energy energetic electrons particle precipitation radiation belts
topic	misc QB1-991 misc energetic electrons misc particle precipitation misc radiation belts misc Astronomy
topic_unstemmed	misc QB1-991 misc energetic electrons misc particle precipitation misc radiation belts misc Astronomy
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title	Dependence of Energetic Electron Precipitation on the Geomagnetic Index Kp and Electron Energy
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title_full	Dependence of Energetic Electron Precipitation on the Geomagnetic Index Kp and Electron Energy
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author_browse	Mi-Young Park Dae-Young Lee Dae-Kyu Shin Jung-Hee Cho Eun-Hee Lee
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author-letter	Mi-Young Park
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title_sort	dependence of energetic electron precipitation on the geomagnetic index kp and electron energy
callnumber	QB1-991
title_auth	Dependence of Energetic Electron Precipitation on the Geomagnetic Index Kp and Electron Energy
abstract	It has long been known that the magnetospheric particles can precipitate into the atmosphere of the Earth. In this paper we examine such precipitation of energetic electrons using the data obtained from low-altitude polar orbiting satellite observations. We analyze the precipitating electron flux data for many periods selected from a total of 84 storm events identified for 2001-2012. The analysis includes the dependence of precipitation on the Kp index and the electron energy, for which we use three energies E1 < 30 keV, E2 < 100 keV, E3 < 300 keV. We find that the precipitation is best correlated with Kp after a time delay of < 3 hours. Most importantly, the correlation with Kp is notably tighter for lower energy than for higher energy in the sense that the lower energy precipitation flux increases more rapidly with Kp than does the higher energy precipitation flux. Based on this we suggest that the Kp index reflects excitation of a wave that is responsible for scattering of preferably lower energy electrons. The role of waves of other types should become increasingly important for higher energy, for which we suggest to rely on other indicators than Kp if one can identify such an indicator.
abstractGer	It has long been known that the magnetospheric particles can precipitate into the atmosphere of the Earth. In this paper we examine such precipitation of energetic electrons using the data obtained from low-altitude polar orbiting satellite observations. We analyze the precipitating electron flux data for many periods selected from a total of 84 storm events identified for 2001-2012. The analysis includes the dependence of precipitation on the Kp index and the electron energy, for which we use three energies E1 < 30 keV, E2 < 100 keV, E3 < 300 keV. We find that the precipitation is best correlated with Kp after a time delay of < 3 hours. Most importantly, the correlation with Kp is notably tighter for lower energy than for higher energy in the sense that the lower energy precipitation flux increases more rapidly with Kp than does the higher energy precipitation flux. Based on this we suggest that the Kp index reflects excitation of a wave that is responsible for scattering of preferably lower energy electrons. The role of waves of other types should become increasingly important for higher energy, for which we suggest to rely on other indicators than Kp if one can identify such an indicator.
abstract_unstemmed	It has long been known that the magnetospheric particles can precipitate into the atmosphere of the Earth. In this paper we examine such precipitation of energetic electrons using the data obtained from low-altitude polar orbiting satellite observations. We analyze the precipitating electron flux data for many periods selected from a total of 84 storm events identified for 2001-2012. The analysis includes the dependence of precipitation on the Kp index and the electron energy, for which we use three energies E1 < 30 keV, E2 < 100 keV, E3 < 300 keV. We find that the precipitation is best correlated with Kp after a time delay of < 3 hours. Most importantly, the correlation with Kp is notably tighter for lower energy than for higher energy in the sense that the lower energy precipitation flux increases more rapidly with Kp than does the higher energy precipitation flux. Based on this we suggest that the Kp index reflects excitation of a wave that is responsible for scattering of preferably lower energy electrons. The role of waves of other types should become increasingly important for higher energy, for which we suggest to rely on other indicators than Kp if one can identify such an indicator.
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title_short	Dependence of Energetic Electron Precipitation on the Geomagnetic Index Kp and Electron Energy
url	https://doi.org/10.5140/JASS.2013.30.4.247 https://doaj.org/article/73a8d029db6440b2ad624b3a0be8af1b http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2013/v30n4/OJOOBS_2013_v30n4_247.pdf https://doaj.org/toc/2093-5587 https://doaj.org/toc/2093-1409
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author2	Dae-Young Lee Dae-Kyu Shin Jung-Hee Cho Eun-Hee Lee
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up_date	2024-07-03T23:36:50.277Z
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