E-region ionospheric storm on May 1–3, 2010: GSM TIP model representation and suggestions for IRI improvement
This paper presents the model simulation results of ionospheric E-region parameters during geomagnetic storm on May 2–3, 2010. For this investigation we used the Global Self-consistent Model of the Thermosphere, Ionosphere and Protonosphere (GSM TIP) developed in West Department of IZMIRAN. GSM TIP...
Gespeichert in:
Veröffentlicht in: | Advances in space research 2015-04, Vol.55 (8), p.2124-2130 |
---|---|
Hauptverfasser: | , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 2130 |
---|---|
container_issue | 8 |
container_start_page | 2124 |
container_title | Advances in space research |
container_volume | 55 |
creator | Bessarab, F.S. Korenkov, Yu.N. Klimenko, V.V. Klimenko, M.V. Zhang, Y. |
description | This paper presents the model simulation results of ionospheric E-region parameters during geomagnetic storm on May 2–3, 2010. For this investigation we used the Global Self-consistent Model of the Thermosphere, Ionosphere and Protonosphere (GSM TIP) developed in West Department of IZMIRAN. GSM TIP model simulations were performed using empirical model of high-energy electron precipitation. The temporal and spatial distributions of the lower ionosphere parameters and minor neutral species are presented. GSM TIP model results of E-region parameters are compared with IRI-2012 model. The differences between model results are discussed. |
doi_str_mv | 10.1016/j.asr.2014.08.003 |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1770276990</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><els_id>S0273117714004992</els_id><sourcerecordid>1770276990</sourcerecordid><originalsourceid>FETCH-LOGICAL-c536t-2cd4a07c18745aa486088fea61d6ba48066968024f6046893d4fa2c48eb607013</originalsourceid><addsrcrecordid>eNqNUctOwzAQtBBIlMIHcPORAwnrxDgOnBAqUKkIBOVsuc6muEriYKdI3PgH_pAvwVU5Iw6r1a5mZh9DyDGDlAETZ6tUB59mwHgKMgXId8iIyaJMWMnlLhlBVuQJY0WxTw5CWAGwrChgRNwk8bi0rqMxXOhf0VtDw-B8S2PzXn9Q9v35lZ_SqA0X9Pb5ns6nj7R1FTbUY-8xYDfoYSOhu4qG9XKJYVMGWjtPp09Tatveu3dsI_CQ7NW6CXj0m8fk5WYyv75LZg-30-urWWLOczEkmam4hsLEE_i51lwKkLJGLVglFrEEIUohIeO1AC5kmVe81pnhEhcCCmD5mJxsdePkt3VcSLU2GGwa3aFbBxU_EV8iyhL-Ac0zyQQTeYSyLdR4F4LHWvXettp_KAZq44NaqeiD2vigQKroQ-RcbjkYz3236FUwFjuDlfVoBlU5-wf7B8kujtM</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1732816163</pqid></control><display><type>article</type><title>E-region ionospheric storm on May 1–3, 2010: GSM TIP model representation and suggestions for IRI improvement</title><source>Elsevier ScienceDirect Journals</source><creator>Bessarab, F.S. ; Korenkov, Yu.N. ; Klimenko, V.V. ; Klimenko, M.V. ; Zhang, Y.</creator><creatorcontrib>Bessarab, F.S. ; Korenkov, Yu.N. ; Klimenko, V.V. ; Klimenko, M.V. ; Zhang, Y.</creatorcontrib><description>This paper presents the model simulation results of ionospheric E-region parameters during geomagnetic storm on May 2–3, 2010. For this investigation we used the Global Self-consistent Model of the Thermosphere, Ionosphere and Protonosphere (GSM TIP) developed in West Department of IZMIRAN. GSM TIP model simulations were performed using empirical model of high-energy electron precipitation. The temporal and spatial distributions of the lower ionosphere parameters and minor neutral species are presented. GSM TIP model results of E-region parameters are compared with IRI-2012 model. The differences between model results are discussed.</description><identifier>ISSN: 0273-1177</identifier><identifier>EISSN: 1879-1948</identifier><identifier>DOI: 10.1016/j.asr.2014.08.003</identifier><language>eng</language><publisher>Elsevier Ltd</publisher><subject>Computer simulation ; E region ; Electric field ; Electron precipitation ; Geomagnetic storm ; Ionospheric modeling ; Ionospheric storms ; IRI-2012 ; Mathematical models ; Nitric oxide density ; Representations ; Spatial distribution ; Temporal logic</subject><ispartof>Advances in space research, 2015-04, Vol.55 (8), p.2124-2130</ispartof><rights>2014 COSPAR</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c536t-2cd4a07c18745aa486088fea61d6ba48066968024f6046893d4fa2c48eb607013</citedby><cites>FETCH-LOGICAL-c536t-2cd4a07c18745aa486088fea61d6ba48066968024f6046893d4fa2c48eb607013</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.sciencedirect.com/science/article/pii/S0273117714004992$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>314,776,780,3537,27901,27902,65306</link.rule.ids></links><search><creatorcontrib>Bessarab, F.S.</creatorcontrib><creatorcontrib>Korenkov, Yu.N.</creatorcontrib><creatorcontrib>Klimenko, V.V.</creatorcontrib><creatorcontrib>Klimenko, M.V.</creatorcontrib><creatorcontrib>Zhang, Y.</creatorcontrib><title>E-region ionospheric storm on May 1–3, 2010: GSM TIP model representation and suggestions for IRI improvement</title><title>Advances in space research</title><description>This paper presents the model simulation results of ionospheric E-region parameters during geomagnetic storm on May 2–3, 2010. For this investigation we used the Global Self-consistent Model of the Thermosphere, Ionosphere and Protonosphere (GSM TIP) developed in West Department of IZMIRAN. GSM TIP model simulations were performed using empirical model of high-energy electron precipitation. The temporal and spatial distributions of the lower ionosphere parameters and minor neutral species are presented. GSM TIP model results of E-region parameters are compared with IRI-2012 model. The differences between model results are discussed.</description><subject>Computer simulation</subject><subject>E region</subject><subject>Electric field</subject><subject>Electron precipitation</subject><subject>Geomagnetic storm</subject><subject>Ionospheric modeling</subject><subject>Ionospheric storms</subject><subject>IRI-2012</subject><subject>Mathematical models</subject><subject>Nitric oxide density</subject><subject>Representations</subject><subject>Spatial distribution</subject><subject>Temporal logic</subject><issn>0273-1177</issn><issn>1879-1948</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNqNUctOwzAQtBBIlMIHcPORAwnrxDgOnBAqUKkIBOVsuc6muEriYKdI3PgH_pAvwVU5Iw6r1a5mZh9DyDGDlAETZ6tUB59mwHgKMgXId8iIyaJMWMnlLhlBVuQJY0WxTw5CWAGwrChgRNwk8bi0rqMxXOhf0VtDw-B8S2PzXn9Q9v35lZ_SqA0X9Pb5ns6nj7R1FTbUY-8xYDfoYSOhu4qG9XKJYVMGWjtPp09Tatveu3dsI_CQ7NW6CXj0m8fk5WYyv75LZg-30-urWWLOczEkmam4hsLEE_i51lwKkLJGLVglFrEEIUohIeO1AC5kmVe81pnhEhcCCmD5mJxsdePkt3VcSLU2GGwa3aFbBxU_EV8iyhL-Ac0zyQQTeYSyLdR4F4LHWvXettp_KAZq44NaqeiD2vigQKroQ-RcbjkYz3236FUwFjuDlfVoBlU5-wf7B8kujtM</recordid><startdate>20150415</startdate><enddate>20150415</enddate><creator>Bessarab, F.S.</creator><creator>Korenkov, Yu.N.</creator><creator>Klimenko, V.V.</creator><creator>Klimenko, M.V.</creator><creator>Zhang, Y.</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>20150415</creationdate><title>E-region ionospheric storm on May 1–3, 2010: GSM TIP model representation and suggestions for IRI improvement</title><author>Bessarab, F.S. ; Korenkov, Yu.N. ; Klimenko, V.V. ; Klimenko, M.V. ; Zhang, Y.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c536t-2cd4a07c18745aa486088fea61d6ba48066968024f6046893d4fa2c48eb607013</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Computer simulation</topic><topic>E region</topic><topic>Electric field</topic><topic>Electron precipitation</topic><topic>Geomagnetic storm</topic><topic>Ionospheric modeling</topic><topic>Ionospheric storms</topic><topic>IRI-2012</topic><topic>Mathematical models</topic><topic>Nitric oxide density</topic><topic>Representations</topic><topic>Spatial distribution</topic><topic>Temporal logic</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Bessarab, F.S.</creatorcontrib><creatorcontrib>Korenkov, Yu.N.</creatorcontrib><creatorcontrib>Klimenko, V.V.</creatorcontrib><creatorcontrib>Klimenko, M.V.</creatorcontrib><creatorcontrib>Zhang, Y.</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>Advances in space research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Bessarab, F.S.</au><au>Korenkov, Yu.N.</au><au>Klimenko, V.V.</au><au>Klimenko, M.V.</au><au>Zhang, Y.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>E-region ionospheric storm on May 1–3, 2010: GSM TIP model representation and suggestions for IRI improvement</atitle><jtitle>Advances in space research</jtitle><date>2015-04-15</date><risdate>2015</risdate><volume>55</volume><issue>8</issue><spage>2124</spage><epage>2130</epage><pages>2124-2130</pages><issn>0273-1177</issn><eissn>1879-1948</eissn><abstract>This paper presents the model simulation results of ionospheric E-region parameters during geomagnetic storm on May 2–3, 2010. For this investigation we used the Global Self-consistent Model of the Thermosphere, Ionosphere and Protonosphere (GSM TIP) developed in West Department of IZMIRAN. GSM TIP model simulations were performed using empirical model of high-energy electron precipitation. The temporal and spatial distributions of the lower ionosphere parameters and minor neutral species are presented. GSM TIP model results of E-region parameters are compared with IRI-2012 model. The differences between model results are discussed.</abstract><pub>Elsevier Ltd</pub><doi>10.1016/j.asr.2014.08.003</doi><tpages>7</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0273-1177 |
ispartof | Advances in space research, 2015-04, Vol.55 (8), p.2124-2130 |
issn | 0273-1177 1879-1948 |
language | eng |
recordid | cdi_proquest_miscellaneous_1770276990 |
source | Elsevier ScienceDirect Journals |
subjects | Computer simulation E region Electric field Electron precipitation Geomagnetic storm Ionospheric modeling Ionospheric storms IRI-2012 Mathematical models Nitric oxide density Representations Spatial distribution Temporal logic |
title | E-region ionospheric storm on May 1–3, 2010: GSM TIP model representation and suggestions for IRI improvement |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-11T07%3A49%3A35IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=E-region%20ionospheric%20storm%20on%20May%201%E2%80%933,%202010:%20GSM%20TIP%20model%20representation%20and%20suggestions%20for%20IRI%20improvement&rft.jtitle=Advances%20in%20space%20research&rft.au=Bessarab,%20F.S.&rft.date=2015-04-15&rft.volume=55&rft.issue=8&rft.spage=2124&rft.epage=2130&rft.pages=2124-2130&rft.issn=0273-1177&rft.eissn=1879-1948&rft_id=info:doi/10.1016/j.asr.2014.08.003&rft_dat=%3Cproquest_cross%3E1770276990%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1732816163&rft_id=info:pmid/&rft_els_id=S0273117714004992&rfr_iscdi=true |