The onset and association of CMEs with sigmoidal active regions
Previous studies of active regions characterised by Soft X‐ray S or inverse‐S morphology [Canfield et al., 1999], have found these regions to possess a higher probability of eruption. In such cases, CME launch has been inferred using X‐ray proxies to indicate eruption. Active regions observed during...
Gespeichert in:
Veröffentlicht in: | Geophysical research letters 2000-07, Vol.27 (14), p.2161-2164 |
---|---|
Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 2164 |
---|---|
container_issue | 14 |
container_start_page | 2161 |
container_title | Geophysical research letters |
container_volume | 27 |
creator | Glover, Alexi Ranns, Neale D. R. Harra, Louise K. Culhane, J. Leonard |
description | Previous studies of active regions characterised by Soft X‐ray S or inverse‐S morphology [Canfield et al., 1999], have found these regions to possess a higher probability of eruption. In such cases, CME launch has been inferred using X‐ray proxies to indicate eruption. Active regions observed during 1997, previously categorised as both sigmoidal and eruptive [Canfield, 1999], have been selected for further study, incorporating SoHO‐LASCO, SoHO‐EIT and ground based H‐alpha data. Our results allow re‐classification into three main categories; sigmoidal, non‐sigmoidal and active regions appearing sigmoidal due to the projection of many loops. Although the reduced dataset size prevents a statistical measure of significance, we note that regions comprising a single S (or inverse‐S) shaped structure are more frequently associated with a CME than those classed as non‐sigmoidal. This motivates the study of a larger dataset and highlights the need for a quantitative observational definition of the term “sigmoid”. |
doi_str_mv | 10.1029/2000GL000018 |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_21480806</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>21480806</sourcerecordid><originalsourceid>FETCH-LOGICAL-c4126-ccb30182557191b4be9a0562cf37d9d0f083ec24d55469a9e4034af8f7871263</originalsourceid><addsrcrecordid>eNp9kE1Lw0AQhhdRsFZv_oA9iCejsx_5OomGmgpRUQr1tmw3m3Y1TWomtfbfm1pRT15m5vA8L8NLyDGDcwY8vuAAkGbdABbtkB6LpfQigHCX9ADi7uZhsE8OEF86RIBgPXI5mllaV2hbqqucasTaON26uqJ1QZO7AdKVa2cU3XReu1yXVJvWvVva2GkH4SHZK3SJ9uh798noZjBKhl72kN4mV5lnJOOBZ8xEdE9x3w9ZzCZyYmMNfsBNIcI8zqGASFjDZe77Moh1bCUIqYuoCKOw80WfnG5jF039trTYqrlDY8tSV7ZeouJMRhDBBjzbgqapERtbqEXj5rpZKwZqU5L6W1KHn3znajS6LBpdGYe_juTAI9lhfIutXGnX_0aq9CljQn797G0lh639-JF086qCUIS-Gt-nCrKEjR-vh-pZfAIdU4Gq</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>21480806</pqid></control><display><type>article</type><title>The onset and association of CMEs with sigmoidal active regions</title><source>Wiley Journals</source><source>Wiley-Blackwell AGU Digital Library</source><source>EZB-FREE-00999 freely available EZB journals</source><source>Wiley Online Library (Open Access Collection)</source><creator>Glover, Alexi ; Ranns, Neale D. R. ; Harra, Louise K. ; Culhane, J. Leonard</creator><creatorcontrib>Glover, Alexi ; Ranns, Neale D. R. ; Harra, Louise K. ; Culhane, J. Leonard</creatorcontrib><description>Previous studies of active regions characterised by Soft X‐ray S or inverse‐S morphology [Canfield et al., 1999], have found these regions to possess a higher probability of eruption. In such cases, CME launch has been inferred using X‐ray proxies to indicate eruption. Active regions observed during 1997, previously categorised as both sigmoidal and eruptive [Canfield, 1999], have been selected for further study, incorporating SoHO‐LASCO, SoHO‐EIT and ground based H‐alpha data. Our results allow re‐classification into three main categories; sigmoidal, non‐sigmoidal and active regions appearing sigmoidal due to the projection of many loops. Although the reduced dataset size prevents a statistical measure of significance, we note that regions comprising a single S (or inverse‐S) shaped structure are more frequently associated with a CME than those classed as non‐sigmoidal. This motivates the study of a larger dataset and highlights the need for a quantitative observational definition of the term “sigmoid”.</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1029/2000GL000018</identifier><identifier>CODEN: GPRLAJ</identifier><language>eng</language><publisher>Washington, DC: Blackwell Publishing Ltd</publisher><subject>Astronomy ; Coronal mass ejection ; Earth, ocean, space ; Exact sciences and technology ; Solar physics ; Solar system</subject><ispartof>Geophysical research letters, 2000-07, Vol.27 (14), p.2161-2164</ispartof><rights>Copyright 2000 by the American Geophysical Union.</rights><rights>2000 INIST-CNRS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c4126-ccb30182557191b4be9a0562cf37d9d0f083ec24d55469a9e4034af8f7871263</citedby><cites>FETCH-LOGICAL-c4126-ccb30182557191b4be9a0562cf37d9d0f083ec24d55469a9e4034af8f7871263</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1029%2F2000GL000018$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F2000GL000018$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,780,784,1417,1433,11514,27924,27925,45574,45575,46409,46468,46833,46892</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=1420284$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Glover, Alexi</creatorcontrib><creatorcontrib>Ranns, Neale D. R.</creatorcontrib><creatorcontrib>Harra, Louise K.</creatorcontrib><creatorcontrib>Culhane, J. Leonard</creatorcontrib><title>The onset and association of CMEs with sigmoidal active regions</title><title>Geophysical research letters</title><addtitle>Geophys. Res. Lett</addtitle><description>Previous studies of active regions characterised by Soft X‐ray S or inverse‐S morphology [Canfield et al., 1999], have found these regions to possess a higher probability of eruption. In such cases, CME launch has been inferred using X‐ray proxies to indicate eruption. Active regions observed during 1997, previously categorised as both sigmoidal and eruptive [Canfield, 1999], have been selected for further study, incorporating SoHO‐LASCO, SoHO‐EIT and ground based H‐alpha data. Our results allow re‐classification into three main categories; sigmoidal, non‐sigmoidal and active regions appearing sigmoidal due to the projection of many loops. Although the reduced dataset size prevents a statistical measure of significance, we note that regions comprising a single S (or inverse‐S) shaped structure are more frequently associated with a CME than those classed as non‐sigmoidal. This motivates the study of a larger dataset and highlights the need for a quantitative observational definition of the term “sigmoid”.</description><subject>Astronomy</subject><subject>Coronal mass ejection</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Solar physics</subject><subject>Solar system</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2000</creationdate><recordtype>article</recordtype><recordid>eNp9kE1Lw0AQhhdRsFZv_oA9iCejsx_5OomGmgpRUQr1tmw3m3Y1TWomtfbfm1pRT15m5vA8L8NLyDGDcwY8vuAAkGbdABbtkB6LpfQigHCX9ADi7uZhsE8OEF86RIBgPXI5mllaV2hbqqucasTaON26uqJ1QZO7AdKVa2cU3XReu1yXVJvWvVva2GkH4SHZK3SJ9uh798noZjBKhl72kN4mV5lnJOOBZ8xEdE9x3w9ZzCZyYmMNfsBNIcI8zqGASFjDZe77Moh1bCUIqYuoCKOw80WfnG5jF039trTYqrlDY8tSV7ZeouJMRhDBBjzbgqapERtbqEXj5rpZKwZqU5L6W1KHn3znajS6LBpdGYe_juTAI9lhfIutXGnX_0aq9CljQn797G0lh639-JF086qCUIS-Gt-nCrKEjR-vh-pZfAIdU4Gq</recordid><startdate>20000715</startdate><enddate>20000715</enddate><creator>Glover, Alexi</creator><creator>Ranns, Neale D. R.</creator><creator>Harra, Louise K.</creator><creator>Culhane, J. Leonard</creator><general>Blackwell Publishing Ltd</general><general>American Geophysical Union</general><scope>BSCLL</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20000715</creationdate><title>The onset and association of CMEs with sigmoidal active regions</title><author>Glover, Alexi ; Ranns, Neale D. R. ; Harra, Louise K. ; Culhane, J. Leonard</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c4126-ccb30182557191b4be9a0562cf37d9d0f083ec24d55469a9e4034af8f7871263</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2000</creationdate><topic>Astronomy</topic><topic>Coronal mass ejection</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Solar physics</topic><topic>Solar system</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Glover, Alexi</creatorcontrib><creatorcontrib>Ranns, Neale D. R.</creatorcontrib><creatorcontrib>Harra, Louise K.</creatorcontrib><creatorcontrib>Culhane, J. Leonard</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>Geophysical research letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Glover, Alexi</au><au>Ranns, Neale D. R.</au><au>Harra, Louise K.</au><au>Culhane, J. Leonard</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The onset and association of CMEs with sigmoidal active regions</atitle><jtitle>Geophysical research letters</jtitle><addtitle>Geophys. Res. Lett</addtitle><date>2000-07-15</date><risdate>2000</risdate><volume>27</volume><issue>14</issue><spage>2161</spage><epage>2164</epage><pages>2161-2164</pages><issn>0094-8276</issn><eissn>1944-8007</eissn><coden>GPRLAJ</coden><abstract>Previous studies of active regions characterised by Soft X‐ray S or inverse‐S morphology [Canfield et al., 1999], have found these regions to possess a higher probability of eruption. In such cases, CME launch has been inferred using X‐ray proxies to indicate eruption. Active regions observed during 1997, previously categorised as both sigmoidal and eruptive [Canfield, 1999], have been selected for further study, incorporating SoHO‐LASCO, SoHO‐EIT and ground based H‐alpha data. Our results allow re‐classification into three main categories; sigmoidal, non‐sigmoidal and active regions appearing sigmoidal due to the projection of many loops. Although the reduced dataset size prevents a statistical measure of significance, we note that regions comprising a single S (or inverse‐S) shaped structure are more frequently associated with a CME than those classed as non‐sigmoidal. This motivates the study of a larger dataset and highlights the need for a quantitative observational definition of the term “sigmoid”.</abstract><cop>Washington, DC</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/2000GL000018</doi><tpages>4</tpages><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0094-8276 |
ispartof | Geophysical research letters, 2000-07, Vol.27 (14), p.2161-2164 |
issn | 0094-8276 1944-8007 |
language | eng |
recordid | cdi_proquest_miscellaneous_21480806 |
source | Wiley Journals; Wiley-Blackwell AGU Digital Library; EZB-FREE-00999 freely available EZB journals; Wiley Online Library (Open Access Collection) |
subjects | Astronomy Coronal mass ejection Earth, ocean, space Exact sciences and technology Solar physics Solar system |
title | The onset and association of CMEs with sigmoidal active regions |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-02T13%3A18%3A22IST&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=The%20onset%20and%20association%20of%20CMEs%20with%20sigmoidal%20active%20regions&rft.jtitle=Geophysical%20research%20letters&rft.au=Glover,%20Alexi&rft.date=2000-07-15&rft.volume=27&rft.issue=14&rft.spage=2161&rft.epage=2164&rft.pages=2161-2164&rft.issn=0094-8276&rft.eissn=1944-8007&rft.coden=GPRLAJ&rft_id=info:doi/10.1029/2000GL000018&rft_dat=%3Cproquest_cross%3E21480806%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=21480806&rft_id=info:pmid/&rfr_iscdi=true |