Quasi-trapped electron fluxes ( [formula omitted]) under the radiation belts: analysis of their connection with geomagnetic indices
Fluxes of energetic electrons ( >0.5 MeV ) at altitudes of about 500 km were measured onboard CORONAS-I, launched in March 1994. We found certain L-shells (2.1,1.6,1.3), where quasi-trapped electrons were observed practically permanently during March–June 1994. Distributions of the anomalous elec...
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Veröffentlicht in: | Journal of atmospheric and solar-terrestrial physics 2002-03, Vol.64 (5), p.601-605 |
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container_title | Journal of atmospheric and solar-terrestrial physics |
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creator | Kuznetsov, S.N. Myagkova, I.N. |
description | Fluxes of energetic electrons (
>0.5
MeV
) at altitudes of about
500
km
were measured onboard CORONAS-I, launched in March 1994. We found certain
L-shells (2.1,1.6,1.3), where quasi-trapped electrons were observed practically permanently during March–June 1994. Distributions of the anomalous electron flux have been determined versus
L, local time and universal time for Northern and Southern hemispheres. The occurrence frequencies of the peaks of electron fluxes have been correlated with geomagnetic indices variations. |
doi_str_mv | 10.1016/S1364-6826(02)00019-6 |
format | Article |
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>0.5
MeV
) at altitudes of about
500
km
were measured onboard CORONAS-I, launched in March 1994. We found certain
L-shells (2.1,1.6,1.3), where quasi-trapped electrons were observed practically permanently during March–June 1994. Distributions of the anomalous electron flux have been determined versus
L, local time and universal time for Northern and Southern hemispheres. The occurrence frequencies of the peaks of electron fluxes have been correlated with geomagnetic indices variations.</description><identifier>ISSN: 1364-6826</identifier><identifier>EISSN: 1879-1824</identifier><identifier>DOI: 10.1016/S1364-6826(02)00019-6</identifier><language>eng</language><publisher>Elsevier Ltd</publisher><subject>Kp-index ; Quasi-trapped electrons ; Radiation belts ; Thunderstorms</subject><ispartof>Journal of atmospheric and solar-terrestrial physics, 2002-03, Vol.64 (5), p.601-605</ispartof><rights>2002</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c369t-13dffdae1c83816d7f721e84a7e6325687c86c953c9a4a46cc6255837d3502453</citedby><cites>FETCH-LOGICAL-c369t-13dffdae1c83816d7f721e84a7e6325687c86c953c9a4a46cc6255837d3502453</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/S1364-6826(02)00019-6$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>315,781,785,3551,27929,27930,46000</link.rule.ids></links><search><creatorcontrib>Kuznetsov, S.N.</creatorcontrib><creatorcontrib>Myagkova, I.N.</creatorcontrib><title>Quasi-trapped electron fluxes ( [formula omitted]) under the radiation belts: analysis of their connection with geomagnetic indices</title><title>Journal of atmospheric and solar-terrestrial physics</title><description>Fluxes of energetic electrons (
>0.5
MeV
) at altitudes of about
500
km
were measured onboard CORONAS-I, launched in March 1994. We found certain
L-shells (2.1,1.6,1.3), where quasi-trapped electrons were observed practically permanently during March–June 1994. Distributions of the anomalous electron flux have been determined versus
L, local time and universal time for Northern and Southern hemispheres. The occurrence frequencies of the peaks of electron fluxes have been correlated with geomagnetic indices variations.</description><subject>Kp-index</subject><subject>Quasi-trapped electrons</subject><subject>Radiation belts</subject><subject>Thunderstorms</subject><issn>1364-6826</issn><issn>1879-1824</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2002</creationdate><recordtype>article</recordtype><recordid>eNqF0U2rEzEUBuBBFKzVnyBkJe1irvmYfIwbkXK9CgURdSUSYnKmjcwkY5K52rV_3JlW113lLJ7zQs5bVc8JviGYiJefCBNNLRQVG0y3GGPS1uJBtSJKtjVRtHk4z__J4-pJzj9mJKkSq-rPx8lkX5dkxhEcgh5sSTGgrp9-Q0Yb9LWLaZh6g-LgSwH3bYum4CChcgSUjPOm-Nl_h77kV8gE05-yzyh2C_AJ2RjCnLmYX74c0QHiYA4BirfIB-ct5KfVo870GZ79e9fVl7e3n3fv6v2Hu_e7N_vaMtGWmjDXdc4AsYopIpzsJCWgGiNBMMqFklYJ23JmW9OYRlgrKOeKScc4pg1n6-rFJXdM8ecEuejBZwt9bwLEKWsqBVOc4quQKC6FVHKG_AJtijkn6PSY_GDSSROsl270uRu9HF5jqs_daDHvvb7swfzdew9JZ-shWHA-zcfSLvorCX8BoACX7w</recordid><startdate>20020301</startdate><enddate>20020301</enddate><creator>Kuznetsov, S.N.</creator><creator>Myagkova, I.N.</creator><general>Elsevier Ltd</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20020301</creationdate><title>Quasi-trapped electron fluxes ( [formula omitted]) under the radiation belts: analysis of their connection with geomagnetic indices</title><author>Kuznetsov, S.N. ; Myagkova, I.N.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c369t-13dffdae1c83816d7f721e84a7e6325687c86c953c9a4a46cc6255837d3502453</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2002</creationdate><topic>Kp-index</topic><topic>Quasi-trapped electrons</topic><topic>Radiation belts</topic><topic>Thunderstorms</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Kuznetsov, S.N.</creatorcontrib><creatorcontrib>Myagkova, I.N.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Journal of atmospheric and solar-terrestrial physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kuznetsov, S.N.</au><au>Myagkova, I.N.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Quasi-trapped electron fluxes ( [formula omitted]) under the radiation belts: analysis of their connection with geomagnetic indices</atitle><jtitle>Journal of atmospheric and solar-terrestrial physics</jtitle><date>2002-03-01</date><risdate>2002</risdate><volume>64</volume><issue>5</issue><spage>601</spage><epage>605</epage><pages>601-605</pages><issn>1364-6826</issn><eissn>1879-1824</eissn><abstract>Fluxes of energetic electrons (
>0.5
MeV
) at altitudes of about
500
km
were measured onboard CORONAS-I, launched in March 1994. We found certain
L-shells (2.1,1.6,1.3), where quasi-trapped electrons were observed practically permanently during March–June 1994. Distributions of the anomalous electron flux have been determined versus
L, local time and universal time for Northern and Southern hemispheres. The occurrence frequencies of the peaks of electron fluxes have been correlated with geomagnetic indices variations.</abstract><pub>Elsevier Ltd</pub><doi>10.1016/S1364-6826(02)00019-6</doi><tpages>5</tpages></addata></record> |
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language | eng |
recordid | cdi_proquest_miscellaneous_27638520 |
source | ScienceDirect Journals (5 years ago - present) |
subjects | Kp-index Quasi-trapped electrons Radiation belts Thunderstorms |
title | Quasi-trapped electron fluxes ( [formula omitted]) under the radiation belts: analysis of their connection with geomagnetic indices |
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