Global Magnetic Patterns of Chirality
During the past five years at least six manifestations of a global organization of solar magnetic fields have been recognized. The magnetic chirality (handedness) of the following features shows a hemispheric preference: filament channels, quiescent filaments, sunspot whorls, superpenumbral fibrils,...
Gespeichert in:
| Veröffentlicht in: | Solar physics 1997-09, Vol.175 (1), p.27-44 |
|---|---|
| Hauptverfasser: | , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 44 |
|---|---|
| container_issue | 1 |
| container_start_page | 27 |
| container_title | Solar physics |
| container_volume | 175 |
| creator | Zirker, J B Martin, S F Harvey, K Gaizauskas, V |
| description | During the past five years at least six manifestations of a global organization of solar magnetic fields have been recognized. The magnetic chirality (handedness) of the following features shows a hemispheric preference: filament channels, quiescent filaments, sunspot whorls, superpenumbral fibrils, coronal arcades, and interplanetary clouds associated with CMEs. Although the patterns are clear in the data, their interpretation and their possible connection to the dynamo is open to question. This paper reviews the observations of the patterns, corrects some misinterpretations, and offers a scenario for the origin of the most marked pattern, the chirality of filaments. We suggest the pattern arises from the reconnection of coronal loops, under the influence of supergranulation and differential rotation. Unlike alternative scenarios, ours relies only on observable surface motions and fields.[PUBLICATION ABSTRACT] |
| doi_str_mv | 10.1023/A:1004946303735 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_miscellaneous_954525759</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>954525759</sourcerecordid><originalsourceid>FETCH-LOGICAL-c258t-6ef08cb1acfccdd9bfddb99ca0f42b21008bf627fcdaf8c9f75bbc4bcc5ebba33</originalsourceid><addsrcrecordid>eNpdjkFLxDAUhIMoWFfPXosgnqqvSV7TeFuWdRVW9KDgrSSviXaJrTbpwX9vRU-eZg4f3wxjpyVclsDF1fK6BJBaVgKEErjHshKVKECLl32WAYj6p9eH7CjGHcAMK8zY-SYM1oT83rz2LnWUP5qU3NjHfPD56q0bTejS1zE78CZEd_KXC_Z8s35a3Rbbh83darktiGOdisp5qMmWhjxR22rr29ZqTQa85JbPk7X1FVeeWuNr0l6htSQtETprjRALdvHr_RiHz8nF1Lx3kVwIpnfDFBuNEjkq1DN59o_cDdPYz-caJWTFOSKKb3tdUMQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>734622555</pqid></control><display><type>article</type><title>Global Magnetic Patterns of Chirality</title><source>SpringerLink Journals - AutoHoldings</source><creator>Zirker, J B ; Martin, S F ; Harvey, K ; Gaizauskas, V</creator><creatorcontrib>Zirker, J B ; Martin, S F ; Harvey, K ; Gaizauskas, V</creatorcontrib><description>During the past five years at least six manifestations of a global organization of solar magnetic fields have been recognized. The magnetic chirality (handedness) of the following features shows a hemispheric preference: filament channels, quiescent filaments, sunspot whorls, superpenumbral fibrils, coronal arcades, and interplanetary clouds associated with CMEs. Although the patterns are clear in the data, their interpretation and their possible connection to the dynamo is open to question. This paper reviews the observations of the patterns, corrects some misinterpretations, and offers a scenario for the origin of the most marked pattern, the chirality of filaments. We suggest the pattern arises from the reconnection of coronal loops, under the influence of supergranulation and differential rotation. Unlike alternative scenarios, ours relies only on observable surface motions and fields.[PUBLICATION ABSTRACT]</description><identifier>ISSN: 0038-0938</identifier><identifier>EISSN: 1573-093X</identifier><identifier>DOI: 10.1023/A:1004946303735</identifier><language>eng</language><publisher>Dordrecht: Springer Nature B.V</publisher><subject>Magnetic fields ; Solar physics ; Studies</subject><ispartof>Solar physics, 1997-09, Vol.175 (1), p.27-44</ispartof><rights>Kluwer Academic Publishers 1997</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c258t-6ef08cb1acfccdd9bfddb99ca0f42b21008bf627fcdaf8c9f75bbc4bcc5ebba33</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27901,27902</link.rule.ids></links><search><creatorcontrib>Zirker, J B</creatorcontrib><creatorcontrib>Martin, S F</creatorcontrib><creatorcontrib>Harvey, K</creatorcontrib><creatorcontrib>Gaizauskas, V</creatorcontrib><title>Global Magnetic Patterns of Chirality</title><title>Solar physics</title><description>During the past five years at least six manifestations of a global organization of solar magnetic fields have been recognized. The magnetic chirality (handedness) of the following features shows a hemispheric preference: filament channels, quiescent filaments, sunspot whorls, superpenumbral fibrils, coronal arcades, and interplanetary clouds associated with CMEs. Although the patterns are clear in the data, their interpretation and their possible connection to the dynamo is open to question. This paper reviews the observations of the patterns, corrects some misinterpretations, and offers a scenario for the origin of the most marked pattern, the chirality of filaments. We suggest the pattern arises from the reconnection of coronal loops, under the influence of supergranulation and differential rotation. Unlike alternative scenarios, ours relies only on observable surface motions and fields.[PUBLICATION ABSTRACT]</description><subject>Magnetic fields</subject><subject>Solar physics</subject><subject>Studies</subject><issn>0038-0938</issn><issn>1573-093X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1997</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNpdjkFLxDAUhIMoWFfPXosgnqqvSV7TeFuWdRVW9KDgrSSviXaJrTbpwX9vRU-eZg4f3wxjpyVclsDF1fK6BJBaVgKEErjHshKVKECLl32WAYj6p9eH7CjGHcAMK8zY-SYM1oT83rz2LnWUP5qU3NjHfPD56q0bTejS1zE78CZEd_KXC_Z8s35a3Rbbh83darktiGOdisp5qMmWhjxR22rr29ZqTQa85JbPk7X1FVeeWuNr0l6htSQtETprjRALdvHr_RiHz8nF1Lx3kVwIpnfDFBuNEjkq1DN59o_cDdPYz-caJWTFOSKKb3tdUMQ</recordid><startdate>19970901</startdate><enddate>19970901</enddate><creator>Zirker, J B</creator><creator>Martin, S F</creator><creator>Harvey, K</creator><creator>Gaizauskas, V</creator><general>Springer Nature B.V</general><scope>3V.</scope><scope>7TG</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AEUYN</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>KL.</scope><scope>L7M</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope></search><sort><creationdate>19970901</creationdate><title>Global Magnetic Patterns of Chirality</title><author>Zirker, J B ; Martin, S F ; Harvey, K ; Gaizauskas, V</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c258t-6ef08cb1acfccdd9bfddb99ca0f42b21008bf627fcdaf8c9f75bbc4bcc5ebba33</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1997</creationdate><topic>Magnetic fields</topic><topic>Solar physics</topic><topic>Studies</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Zirker, J B</creatorcontrib><creatorcontrib>Martin, S F</creatorcontrib><creatorcontrib>Harvey, K</creatorcontrib><creatorcontrib>Gaizauskas, V</creatorcontrib><collection>ProQuest Central (Corporate)</collection><collection>Meteorological & Geoastrophysical Abstracts</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 One Sustainability</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & 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>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Science Database</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & 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 Basic</collection><jtitle>Solar physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Zirker, J B</au><au>Martin, S F</au><au>Harvey, K</au><au>Gaizauskas, V</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Global Magnetic Patterns of Chirality</atitle><jtitle>Solar physics</jtitle><date>1997-09-01</date><risdate>1997</risdate><volume>175</volume><issue>1</issue><spage>27</spage><epage>44</epage><pages>27-44</pages><issn>0038-0938</issn><eissn>1573-093X</eissn><abstract>During the past five years at least six manifestations of a global organization of solar magnetic fields have been recognized. The magnetic chirality (handedness) of the following features shows a hemispheric preference: filament channels, quiescent filaments, sunspot whorls, superpenumbral fibrils, coronal arcades, and interplanetary clouds associated with CMEs. Although the patterns are clear in the data, their interpretation and their possible connection to the dynamo is open to question. This paper reviews the observations of the patterns, corrects some misinterpretations, and offers a scenario for the origin of the most marked pattern, the chirality of filaments. We suggest the pattern arises from the reconnection of coronal loops, under the influence of supergranulation and differential rotation. Unlike alternative scenarios, ours relies only on observable surface motions and fields.[PUBLICATION ABSTRACT]</abstract><cop>Dordrecht</cop><pub>Springer Nature B.V</pub><doi>10.1023/A:1004946303735</doi><tpages>18</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0038-0938 |
| ispartof | Solar physics, 1997-09, Vol.175 (1), p.27-44 |
| issn | 0038-0938 1573-093X |
| language | eng |
| recordid | cdi_proquest_miscellaneous_954525759 |
| source | SpringerLink Journals - AutoHoldings |
| subjects | Magnetic fields Solar physics Studies |
| title | Global Magnetic Patterns of Chirality |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-03T14%3A39%3A15IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Global%20Magnetic%20Patterns%20of%20Chirality&rft.jtitle=Solar%20physics&rft.au=Zirker,%20J%20B&rft.date=1997-09-01&rft.volume=175&rft.issue=1&rft.spage=27&rft.epage=44&rft.pages=27-44&rft.issn=0038-0938&rft.eissn=1573-093X&rft_id=info:doi/10.1023/A:1004946303735&rft_dat=%3Cproquest%3E954525759%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=734622555&rft_id=info:pmid/&rfr_iscdi=true |