Review of electron fluxes within the local drift loss cone: Measurements on CORONAS-I

R. Bučík; K. Kudela; A. V. Dmitriev; S. N. Kuznetsov; I. N. Myagkova; S. P. Ryumin

doi:10.1016/j.asr.2003.03.077

Review of electron fluxes within the local drift loss cone: Measurements on CORONAS-I

R. Bučík, K. Kudela, A. V. Dmitriev, S. N. Kuznetsov, I. N. Myagkova, S. P. Ryumin

太空科學與工程學系

研究成果: 雜誌貢獻 › 期刊論文 › 同行評審

6 引文斯高帕斯（Scopus）

摘要

Measurements of relativistic electrons (500 keV to 12 MeV) within the drift loss cone during geomagnetic storms in the spring of 1994, obtained with MKL instrument aboard the low-altitude (∼500 km) polar-orbiting satellite, CORONAS-I, are reviewed. CORONAS-I satellite observed two more pronounced electron enhancements during the period studied (March-April 1994). Time profile of Dst index indicates that these events occurred after magnetic storms on March 6-8, 1994 (Dst = -109 nT) and April 2-4, 1994 (Dst = -111 nT). Both time and L shell variations of the precipitating electron fluxes over the wide L shell range of 1-9 are presented and discussed. On the average, these fluxes had a maximum value at L = 3.8-4.6 observed during the storm recovery phases.

原文	???core.languages.en_GB???
頁（從 - 到）	1979-1983
頁數	5
期刊	Advances in Space Research
卷	36
發行號	10
DOIs	https://doi.org/10.1016/j.asr.2003.03.077
出版狀態	已出版 - 2005

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10.1016/j.asr.2003.03.077

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@article{9d880ce9f25a4a228de49f78bb6a0ba5,

title = "Review of electron fluxes within the local drift loss cone: Measurements on CORONAS-I",

abstract = "Measurements of relativistic electrons (500 keV to 12 MeV) within the drift loss cone during geomagnetic storms in the spring of 1994, obtained with MKL instrument aboard the low-altitude (∼500 km) polar-orbiting satellite, CORONAS-I, are reviewed. CORONAS-I satellite observed two more pronounced electron enhancements during the period studied (March-April 1994). Time profile of Dst index indicates that these events occurred after magnetic storms on March 6-8, 1994 (Dst = -109 nT) and April 2-4, 1994 (Dst = -111 nT). Both time and L shell variations of the precipitating electron fluxes over the wide L shell range of 1-9 are presented and discussed. On the average, these fluxes had a maximum value at L = 3.8-4.6 observed during the storm recovery phases.",

keywords = "Drift loss cone, Outer radiation belt, Relativistic electrons",

author = "R. Bu{\v c}{\'i}k and K. Kudela and Dmitriev, {A. V.} and Kuznetsov, {S. N.} and Myagkova, {I. N.} and Ryumin, {S. P.}",

note = "Funding Information: This work was supported by Slovak Scientific Grant Agency VEGA under Grant 2/4064. Dst indices were obtained from the World Data Center, Kyoto website.",

year = "2005",

doi = "10.1016/j.asr.2003.03.077",

language = "???core.languages.en_GB???",

volume = "36",

pages = "1979--1983",

journal = "Advances in Space Research",

issn = "0273-1177",

number = "10",

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TY - JOUR

T1 - Review of electron fluxes within the local drift loss cone

T2 - Measurements on CORONAS-I

AU - Bučík, R.

AU - Kudela, K.

AU - Dmitriev, A. V.

AU - Kuznetsov, S. N.

AU - Myagkova, I. N.

AU - Ryumin, S. P.

N1 - Funding Information: This work was supported by Slovak Scientific Grant Agency VEGA under Grant 2/4064. Dst indices were obtained from the World Data Center, Kyoto website.

PY - 2005

Y1 - 2005

N2 - Measurements of relativistic electrons (500 keV to 12 MeV) within the drift loss cone during geomagnetic storms in the spring of 1994, obtained with MKL instrument aboard the low-altitude (∼500 km) polar-orbiting satellite, CORONAS-I, are reviewed. CORONAS-I satellite observed two more pronounced electron enhancements during the period studied (March-April 1994). Time profile of Dst index indicates that these events occurred after magnetic storms on March 6-8, 1994 (Dst = -109 nT) and April 2-4, 1994 (Dst = -111 nT). Both time and L shell variations of the precipitating electron fluxes over the wide L shell range of 1-9 are presented and discussed. On the average, these fluxes had a maximum value at L = 3.8-4.6 observed during the storm recovery phases.

AB - Measurements of relativistic electrons (500 keV to 12 MeV) within the drift loss cone during geomagnetic storms in the spring of 1994, obtained with MKL instrument aboard the low-altitude (∼500 km) polar-orbiting satellite, CORONAS-I, are reviewed. CORONAS-I satellite observed two more pronounced electron enhancements during the period studied (March-April 1994). Time profile of Dst index indicates that these events occurred after magnetic storms on March 6-8, 1994 (Dst = -109 nT) and April 2-4, 1994 (Dst = -111 nT). Both time and L shell variations of the precipitating electron fluxes over the wide L shell range of 1-9 are presented and discussed. On the average, these fluxes had a maximum value at L = 3.8-4.6 observed during the storm recovery phases.

KW - Drift loss cone

KW - Outer radiation belt

KW - Relativistic electrons

UR - http://www.scopus.com/inward/record.url?scp=27844589900&partnerID=8YFLogxK

U2 - 10.1016/j.asr.2003.03.077

DO - 10.1016/j.asr.2003.03.077

M3 - 期刊論文

AN - SCOPUS:27844589900

SN - 0273-1177

VL - 36

SP - 1979

EP - 1983

JO - Advances in Space Research

JF - Advances in Space Research

IS - 10

ER -

Review of electron fluxes within the local drift loss cone: Measurements on CORONAS-I

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