Variations of the multi-component ring current energy spectra during the geomagnetic storms: “Gorizont-35” results
The geosynchronous satellite Gorizont-35 results of observations and analysis of the ring current H +, He 2+ and O + ion's energy spectra variations near midnight (23.30±01.30 LT) during substorms and storms 11–24 Mach 1992 are presented. Measurements were made in E=41 – 133 keV/e energy range...
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| Veröffentlicht in: | Advances in space research 1996, Vol.17 (2), p.179-182 |
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| container_title | Advances in space research |
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| creator | Kovtyukh, A.S Martinenko, G.B Sosnovets, E.N Panasyuk, M.I Goryainov, M.F Savin, B.I |
| description | The geosynchronous satellite Gorizont-35 results of observations and analysis of the ring current H
+, He
2+ and O
+ ion's energy spectra variations near midnight (23.30±01.30 LT) during substorms and storms 11–24 Mach 1992 are presented. Measurements were made in E=41 – 133 keV/e energy range in seven channals (
ΔE
E
≈0.1
). It was found that the O
+ ions are the main component of the ring current energy density during the period of the active Sun. The He
2+ ions is the most dynamic component of the ring current (especially for E |
| doi_str_mv | 10.1016/0273-1177(95)00533-K |
| format | Article |
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+, He
2+ and O
+ ion's energy spectra variations near midnight (23.30±01.30 LT) during substorms and storms 11–24 Mach 1992 are presented. Measurements were made in E=41 – 133 keV/e energy range in seven channals (
ΔE
E
≈0.1
). It was found that the O
+ ions are the main component of the ring current energy density during the period of the active Sun. The He
2+ ions is the most dynamic component of the ring current (especially for E<70 keV/e). The H
+, He
2+ and O
+ ions energy spectra are almost similar in the same energy per charge presentation form.</description><identifier>ISSN: 0273-1177</identifier><identifier>EISSN: 1879-1948</identifier><identifier>DOI: 10.1016/0273-1177(95)00533-K</identifier><language>eng</language><publisher>Elsevier Ltd</publisher><ispartof>Advances in space research, 1996, Vol.17 (2), p.179-182</ispartof><rights>1995</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c199t-23790d6dde8b5310e432674088b7167a0e7d594325a109b0d9f2a8ad91b153403</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/0273-1177(95)00533-K$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>309,310,314,777,781,786,787,3537,4010,23911,23912,25121,27904,27905,27906,45976</link.rule.ids></links><search><creatorcontrib>Kovtyukh, A.S</creatorcontrib><creatorcontrib>Martinenko, G.B</creatorcontrib><creatorcontrib>Sosnovets, E.N</creatorcontrib><creatorcontrib>Panasyuk, M.I</creatorcontrib><creatorcontrib>Goryainov, M.F</creatorcontrib><creatorcontrib>Savin, B.I</creatorcontrib><title>Variations of the multi-component ring current energy spectra during the geomagnetic storms: “Gorizont-35” results</title><title>Advances in space research</title><description>The geosynchronous satellite Gorizont-35 results of observations and analysis of the ring current H
+, He
2+ and O
+ ion's energy spectra variations near midnight (23.30±01.30 LT) during substorms and storms 11–24 Mach 1992 are presented. Measurements were made in E=41 – 133 keV/e energy range in seven channals (
ΔE
E
≈0.1
). It was found that the O
+ ions are the main component of the ring current energy density during the period of the active Sun. The He
2+ ions is the most dynamic component of the ring current (especially for E<70 keV/e). The H
+, He
2+ and O
+ ions energy spectra are almost similar in the same energy per charge presentation form.</description><issn>0273-1177</issn><issn>1879-1948</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1996</creationdate><recordtype>article</recordtype><recordid>eNp9kM1KAzEUhYMoWH_ewEVWoovRZDIzmbgQpGiVFtyo25AmtzXSSWqSKeiqD6Iv55M4Y8Wlq8u995wD50PoiJIzSmh1TnLOMko5PxHlKSElY9l4Cw1ozUVGRVFvo8GfZBftxfhCCM05JwO0elLBqmS9i9jPcHoG3LSLZDPtm6V34BIO1s2xbkPoF3AQ5m84LkGnoLBpf769bQ6-UXMHyWockw9NvMBf64-RD_bdu5Sx8mv9iQPELj4eoJ2ZWkQ4_J376PHm-mF4m03uR3fDq0mmqRApyxkXxFTGQD0tGSVQsLziBanrKacVVwS4KUV3LBUlYkqMmOWqVkbQKS1ZQdg-Ot7kLoN_bSEm2dioYbFQDnwbZV4VjOWi6oTFRqiDjzHATC6DbVR4k5TIHrLsCcqeoBSl_IEsx53tcmODrsTKQpBRW3AajA0dIWm8_T_gGyVAhpQ</recordid><startdate>1996</startdate><enddate>1996</enddate><creator>Kovtyukh, A.S</creator><creator>Martinenko, G.B</creator><creator>Sosnovets, E.N</creator><creator>Panasyuk, M.I</creator><creator>Goryainov, M.F</creator><creator>Savin, B.I</creator><general>Elsevier Ltd</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>1996</creationdate><title>Variations of the multi-component ring current energy spectra during the geomagnetic storms: “Gorizont-35” results</title><author>Kovtyukh, A.S ; Martinenko, G.B ; Sosnovets, E.N ; Panasyuk, M.I ; Goryainov, M.F ; Savin, B.I</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c199t-23790d6dde8b5310e432674088b7167a0e7d594325a109b0d9f2a8ad91b153403</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1996</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Kovtyukh, A.S</creatorcontrib><creatorcontrib>Martinenko, G.B</creatorcontrib><creatorcontrib>Sosnovets, E.N</creatorcontrib><creatorcontrib>Panasyuk, M.I</creatorcontrib><creatorcontrib>Goryainov, M.F</creatorcontrib><creatorcontrib>Savin, B.I</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Advances in space research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kovtyukh, A.S</au><au>Martinenko, G.B</au><au>Sosnovets, E.N</au><au>Panasyuk, M.I</au><au>Goryainov, M.F</au><au>Savin, B.I</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Variations of the multi-component ring current energy spectra during the geomagnetic storms: “Gorizont-35” results</atitle><jtitle>Advances in space research</jtitle><date>1996</date><risdate>1996</risdate><volume>17</volume><issue>2</issue><spage>179</spage><epage>182</epage><pages>179-182</pages><issn>0273-1177</issn><eissn>1879-1948</eissn><abstract>The geosynchronous satellite Gorizont-35 results of observations and analysis of the ring current H
+, He
2+ and O
+ ion's energy spectra variations near midnight (23.30±01.30 LT) during substorms and storms 11–24 Mach 1992 are presented. Measurements were made in E=41 – 133 keV/e energy range in seven channals (
ΔE
E
≈0.1
). It was found that the O
+ ions are the main component of the ring current energy density during the period of the active Sun. The He
2+ ions is the most dynamic component of the ring current (especially for E<70 keV/e). The H
+, He
2+ and O
+ ions energy spectra are almost similar in the same energy per charge presentation form.</abstract><pub>Elsevier Ltd</pub><doi>10.1016/0273-1177(95)00533-K</doi><tpages>4</tpages></addata></record> |
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| identifier | ISSN: 0273-1177 |
| ispartof | Advances in space research, 1996, Vol.17 (2), p.179-182 |
| issn | 0273-1177 1879-1948 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_26433296 |
| source | Elsevier ScienceDirect Journals |
| title | Variations of the multi-component ring current energy spectra during the geomagnetic storms: “Gorizont-35” results |
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