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...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Geophysical research letters 2000-07, Vol.27 (14), p.2161-2164
Hauptverfasser: Glover, Alexi, Ranns, Neale D. R., Harra, Louise K., Culhane, J. Leonard
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&amp;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 &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; 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