A Trans-equatorial Filament and the Bastille Day Flare/CME Event

The Bastille Day Event on July 14 2000, a major solar flare and a global coronal mass ejection (CME), is not a phenomenon of a single active region. Activation and eruption of a huge trans-equatorial filament is seen to precede the simultaneous filament eruption and flare in the source active region...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Proceedings of the International Astronomical Union 2004-09, Vol.2004 (IAUS226), p.135-136
Hauptverfasser: Wang, Jingxiu, Zhou, Guiping, Wen, Yayuan, Zhang, Yuzong, Zhang, Jun, Wang, Huaning, Deng, Yuanyong
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 136
container_issue IAUS226
container_start_page 135
container_title Proceedings of the International Astronomical Union
container_volume 2004
creator Wang, Jingxiu
Zhou, Guiping
Wen, Yayuan
Zhang, Yuzong
Zhang, Jun
Wang, Huaning
Deng, Yuanyong
description The Bastille Day Event on July 14 2000, a major solar flare and a global coronal mass ejection (CME), is not a phenomenon of a single active region. Activation and eruption of a huge trans-equatorial filament is seen to precede the simultaneous filament eruption and flare in the source active region, AR9077, and the full halo-CME in the high corona. Evidence of reconfiguration of large-scale structures, manifested by SOHO EIT and Yohkoh SXT observations, is clearly seen. The large-scale magnetic composition related to the trans-equatorial filament and its sheared magnetic arcades appears to be the essential part of the CME parent magnetic structure. Estimations show that the filament-arcade system has enough magnetic helicityto account for the helicity carried by the related CMEs.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html
doi_str_mv 10.1017/S1743921305000360
format Article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_19654198</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><cupid>10_1017_S1743921305000360</cupid><sourcerecordid>1401573121</sourcerecordid><originalsourceid>FETCH-LOGICAL-c272t-ae06a449cda09c24c822ddddfbb6b3075f772a76487a013db70aa8b1577ff61b3</originalsourceid><addsrcrecordid>eNp1kEFLw0AQhRdRsFZ_gLfFg7fY2d3sbnKz1lSFigfrOUySjaZsknY3EfrvTWlRUJzLDMP3Ho9HyCWDGwZMT16ZDkXMmQAJAELBERntXkHMOTv-vpk4JWferwBCFQk5IrdTunTY-MBseuxaV6Gl88pibZqOYlPQ7sPQO_RdZa2h97ilc4vOTGbPCU0-B-icnJRovbk47DF5myfL2WOweHl4mk0XQc417wI0oDAM47xAiHMe5hHnxTBllqlMgJal1hy1CiONwESRaUCMMia1LkvFMjEm13vftWs3vfFdWlc-N9ZiY9repyxWMmRxNIBXv8BV27tmyJZyLjkA13KA2B7KXeu9M2W6dlWNbpsySHeFpn8KHTTioME6c1Xxbn6c_1d9Abw_dTo</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>225200275</pqid></control><display><type>article</type><title>A Trans-equatorial Filament and the Bastille Day Flare/CME Event</title><source>Cambridge Journals</source><creator>Wang, Jingxiu ; Zhou, Guiping ; Wen, Yayuan ; Zhang, Yuzong ; Zhang, Jun ; Wang, Huaning ; Deng, Yuanyong</creator><creatorcontrib>Wang, Jingxiu ; Zhou, Guiping ; Wen, Yayuan ; Zhang, Yuzong ; Zhang, Jun ; Wang, Huaning ; Deng, Yuanyong</creatorcontrib><description>The Bastille Day Event on July 14 2000, a major solar flare and a global coronal mass ejection (CME), is not a phenomenon of a single active region. Activation and eruption of a huge trans-equatorial filament is seen to precede the simultaneous filament eruption and flare in the source active region, AR9077, and the full halo-CME in the high corona. Evidence of reconfiguration of large-scale structures, manifested by SOHO EIT and Yohkoh SXT observations, is clearly seen. The large-scale magnetic composition related to the trans-equatorial filament and its sheared magnetic arcades appears to be the essential part of the CME parent magnetic structure. Estimations show that the filament-arcade system has enough magnetic helicityto account for the helicity carried by the related CMEs.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html</description><identifier>ISSN: 1743-9213</identifier><identifier>EISSN: 1743-9221</identifier><identifier>DOI: 10.1017/S1743921305000360</identifier><language>eng</language><publisher>Cambridge, UK: Cambridge University Press</publisher><subject>Astronomy ; Contributed Papers</subject><ispartof>Proceedings of the International Astronomical Union, 2004-09, Vol.2004 (IAUS226), p.135-136</ispartof><rights>2005 International Astronomical Union</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.cambridge.org/core/product/identifier/S1743921305000360/type/journal_article$$EHTML$$P50$$Gcambridge$$H</linktohtml><link.rule.ids>164,314,780,784,27924,27925,55628</link.rule.ids></links><search><creatorcontrib>Wang, Jingxiu</creatorcontrib><creatorcontrib>Zhou, Guiping</creatorcontrib><creatorcontrib>Wen, Yayuan</creatorcontrib><creatorcontrib>Zhang, Yuzong</creatorcontrib><creatorcontrib>Zhang, Jun</creatorcontrib><creatorcontrib>Wang, Huaning</creatorcontrib><creatorcontrib>Deng, Yuanyong</creatorcontrib><title>A Trans-equatorial Filament and the Bastille Day Flare/CME Event</title><title>Proceedings of the International Astronomical Union</title><addtitle>Proc. IAU</addtitle><description>The Bastille Day Event on July 14 2000, a major solar flare and a global coronal mass ejection (CME), is not a phenomenon of a single active region. Activation and eruption of a huge trans-equatorial filament is seen to precede the simultaneous filament eruption and flare in the source active region, AR9077, and the full halo-CME in the high corona. Evidence of reconfiguration of large-scale structures, manifested by SOHO EIT and Yohkoh SXT observations, is clearly seen. The large-scale magnetic composition related to the trans-equatorial filament and its sheared magnetic arcades appears to be the essential part of the CME parent magnetic structure. Estimations show that the filament-arcade system has enough magnetic helicityto account for the helicity carried by the related CMEs.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html</description><subject>Astronomy</subject><subject>Contributed Papers</subject><issn>1743-9213</issn><issn>1743-9221</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2004</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><recordid>eNp1kEFLw0AQhRdRsFZ_gLfFg7fY2d3sbnKz1lSFigfrOUySjaZsknY3EfrvTWlRUJzLDMP3Ho9HyCWDGwZMT16ZDkXMmQAJAELBERntXkHMOTv-vpk4JWferwBCFQk5IrdTunTY-MBseuxaV6Gl88pibZqOYlPQ7sPQO_RdZa2h97ilc4vOTGbPCU0-B-icnJRovbk47DF5myfL2WOweHl4mk0XQc417wI0oDAM47xAiHMe5hHnxTBllqlMgJal1hy1CiONwESRaUCMMia1LkvFMjEm13vftWs3vfFdWlc-N9ZiY9repyxWMmRxNIBXv8BV27tmyJZyLjkA13KA2B7KXeu9M2W6dlWNbpsySHeFpn8KHTTioME6c1Xxbn6c_1d9Abw_dTo</recordid><startdate>20040901</startdate><enddate>20040901</enddate><creator>Wang, Jingxiu</creator><creator>Zhou, Guiping</creator><creator>Wen, Yayuan</creator><creator>Zhang, Yuzong</creator><creator>Zhang, Jun</creator><creator>Wang, Huaning</creator><creator>Deng, Yuanyong</creator><general>Cambridge University Press</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>Q9U</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20040901</creationdate><title>A Trans-equatorial Filament and the Bastille Day Flare/CME Event</title><author>Wang, Jingxiu ; Zhou, Guiping ; Wen, Yayuan ; Zhang, Yuzong ; Zhang, Jun ; Wang, Huaning ; Deng, Yuanyong</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c272t-ae06a449cda09c24c822ddddfbb6b3075f772a76487a013db70aa8b1577ff61b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2004</creationdate><topic>Astronomy</topic><topic>Contributed Papers</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Wang, Jingxiu</creatorcontrib><creatorcontrib>Zhou, Guiping</creatorcontrib><creatorcontrib>Wen, Yayuan</creatorcontrib><creatorcontrib>Zhang, Yuzong</creatorcontrib><creatorcontrib>Zhang, Jun</creatorcontrib><creatorcontrib>Wang, Huaning</creatorcontrib><creatorcontrib>Deng, Yuanyong</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies &amp; Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ProQuest Central Student</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Science Database</collection><collection>Advanced Technologies &amp; Aerospace Database</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Collection</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>ProQuest Central Basic</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><jtitle>Proceedings of the International Astronomical Union</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Wang, Jingxiu</au><au>Zhou, Guiping</au><au>Wen, Yayuan</au><au>Zhang, Yuzong</au><au>Zhang, Jun</au><au>Wang, Huaning</au><au>Deng, Yuanyong</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A Trans-equatorial Filament and the Bastille Day Flare/CME Event</atitle><jtitle>Proceedings of the International Astronomical Union</jtitle><addtitle>Proc. IAU</addtitle><date>2004-09-01</date><risdate>2004</risdate><volume>2004</volume><issue>IAUS226</issue><spage>135</spage><epage>136</epage><pages>135-136</pages><issn>1743-9213</issn><eissn>1743-9221</eissn><abstract>The Bastille Day Event on July 14 2000, a major solar flare and a global coronal mass ejection (CME), is not a phenomenon of a single active region. Activation and eruption of a huge trans-equatorial filament is seen to precede the simultaneous filament eruption and flare in the source active region, AR9077, and the full halo-CME in the high corona. Evidence of reconfiguration of large-scale structures, manifested by SOHO EIT and Yohkoh SXT observations, is clearly seen. The large-scale magnetic composition related to the trans-equatorial filament and its sheared magnetic arcades appears to be the essential part of the CME parent magnetic structure. Estimations show that the filament-arcade system has enough magnetic helicityto account for the helicity carried by the related CMEs.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html</abstract><cop>Cambridge, UK</cop><pub>Cambridge University Press</pub><doi>10.1017/S1743921305000360</doi><tpages>2</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 1743-9213
ispartof Proceedings of the International Astronomical Union, 2004-09, Vol.2004 (IAUS226), p.135-136
issn 1743-9213
1743-9221
language eng
recordid cdi_proquest_miscellaneous_19654198
source Cambridge Journals
subjects Astronomy
Contributed Papers
title A Trans-equatorial Filament and the Bastille Day Flare/CME Event
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-04T23%3A08%3A28IST&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=A%20Trans-equatorial%20Filament%20and%20the%20Bastille%20Day%20Flare/CME%20Event&rft.jtitle=Proceedings%20of%20the%20International%20Astronomical%20Union&rft.au=Wang,%20Jingxiu&rft.date=2004-09-01&rft.volume=2004&rft.issue=IAUS226&rft.spage=135&rft.epage=136&rft.pages=135-136&rft.issn=1743-9213&rft.eissn=1743-9221&rft_id=info:doi/10.1017/S1743921305000360&rft_dat=%3Cproquest_cross%3E1401573121%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=225200275&rft_id=info:pmid/&rft_cupid=10_1017_S1743921305000360&rfr_iscdi=true