Loading…
Magnetic reconnection in the auroral acceleration region
Evidence is presented for the operation of extreme guide field magnetic reconnection in the presence of sheared flows in a narrow current sheet through the auroral acceleration region. Using auroral imagery, magnetically conjugate particle measurements and a 3‐D reduced MHD simulation, vortical moti...
Saved in:
Published in: | Geophysical research letters 2015-03, Vol.42 (6), p.1646-1653 |
---|---|
Main Author: | |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | cdi_FETCH-LOGICAL-c5040-4aa2aa999d601e41bfdd5d217b8eb598e60074aaea431533ffdc9c66083e29ab3 |
---|---|
cites | cdi_FETCH-LOGICAL-c5040-4aa2aa999d601e41bfdd5d217b8eb598e60074aaea431533ffdc9c66083e29ab3 |
container_end_page | 1653 |
container_issue | 6 |
container_start_page | 1646 |
container_title | Geophysical research letters |
container_volume | 42 |
creator | Chaston, C. C. |
description | Evidence is presented for the operation of extreme guide field magnetic reconnection in the presence of sheared flows in a narrow current sheet through the auroral acceleration region. Using auroral imagery, magnetically conjugate particle measurements and a 3‐D reduced MHD simulation, vortical motions in a narrow, rapidly evolving auroral arc indicative of the operation of magnetic tearing are identified. An estimate of the contribution of this process to the observed rate of energy deposition at the ionosphere shows that while this contribution can be significant it remains a minor fraction of the total. These observations are placed in the context of low magnetic shear reconnection made possible in plasmas with low plasma beta.
Key Points
Magnetic reconnection occurs in narrow discrete auroral arcs
Magnetic reconnection can occur for extremely small magnetic shear
Magnetic reconnection contributes |
doi_str_mv | 10.1002/2015GL063164 |
format | article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1685801225</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1910861254</sourcerecordid><originalsourceid>FETCH-LOGICAL-c5040-4aa2aa999d601e41bfdd5d217b8eb598e60074aaea431533ffdc9c66083e29ab3</originalsourceid><addsrcrecordid>eNqN0U1Lw0AQBuBFFKwfN39AwIsHozP7ld2jFK1CRRA9h81mUlPSpG4SpP_e1XoQD8XTDMzDMMPL2BnCFQLwaw6oZnPQArXcYxO0UqYGINtnEwAbe57pQ3bU90sAECBwwsyjW7Q01D4J5Lu2JT_UXZvUbTK8UeLG0AXXJM57aii471mgRSwn7KByTU-nP_WYvd7dvkzv0_nT7GF6M0-9AgmpdI47Z60tNSBJLKqyVCXHrDBUKGtIx_siIicFKiGqqvTWaw1GELeuEMfsYrt3Hbr3kfohX9V9vKZxLXVjn6M2ygByrv5DhVBSch3p-R-67MbQxkdytAhGI1dyp9KZMIiG86gut8qHru8DVfk61CsXNjlC_pVL_juXyPmWf9QNbXbafPY8VzyLWX0CY0KLQg</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1673811822</pqid></control><display><type>article</type><title>Magnetic reconnection in the auroral acceleration region</title><source>Wiley-Blackwell AGU Digital Archive</source><creator>Chaston, C. C.</creator><creatorcontrib>Chaston, C. C.</creatorcontrib><description>Evidence is presented for the operation of extreme guide field magnetic reconnection in the presence of sheared flows in a narrow current sheet through the auroral acceleration region. Using auroral imagery, magnetically conjugate particle measurements and a 3‐D reduced MHD simulation, vortical motions in a narrow, rapidly evolving auroral arc indicative of the operation of magnetic tearing are identified. An estimate of the contribution of this process to the observed rate of energy deposition at the ionosphere shows that while this contribution can be significant it remains a minor fraction of the total. These observations are placed in the context of low magnetic shear reconnection made possible in plasmas with low plasma beta.
Key Points
Magnetic reconnection occurs in narrow discrete auroral arcs
Magnetic reconnection can occur for extremely small magnetic shear
Magnetic reconnection contributes <20% to the auroral acceleration energy budget</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1002/2015GL063164</identifier><language>eng</language><publisher>Washington: John Wiley & Sons, Inc</publisher><subject>Acceleration ; aurora ; Auroral arcs ; Auroral zones ; Auroras ; Current sheets ; Deposition ; electric fields ; Energy ; Energy budgets ; Geophysics ; Identification ; Imagery ; Ionosphere ; Magnetic fields ; Magnetic reconnection ; Magnetohydrodynamics ; particle acceleration ; Plasmas ; Plasmas (physics) ; reconnection ; Shear ; Simulation ; Tearing ; tearing instability ; Three dimensional ; vorticity</subject><ispartof>Geophysical research letters, 2015-03, Vol.42 (6), p.1646-1653</ispartof><rights>2015. American Geophysical Union. All Rights Reserved.</rights><rights>Copyright Blackwell Publishing Ltd. Mar 2015</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c5040-4aa2aa999d601e41bfdd5d217b8eb598e60074aaea431533ffdc9c66083e29ab3</citedby><cites>FETCH-LOGICAL-c5040-4aa2aa999d601e41bfdd5d217b8eb598e60074aaea431533ffdc9c66083e29ab3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1002%2F2015GL063164$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1002%2F2015GL063164$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,776,780,11490,27898,27899,46440,46864</link.rule.ids></links><search><creatorcontrib>Chaston, C. C.</creatorcontrib><title>Magnetic reconnection in the auroral acceleration region</title><title>Geophysical research letters</title><description>Evidence is presented for the operation of extreme guide field magnetic reconnection in the presence of sheared flows in a narrow current sheet through the auroral acceleration region. Using auroral imagery, magnetically conjugate particle measurements and a 3‐D reduced MHD simulation, vortical motions in a narrow, rapidly evolving auroral arc indicative of the operation of magnetic tearing are identified. An estimate of the contribution of this process to the observed rate of energy deposition at the ionosphere shows that while this contribution can be significant it remains a minor fraction of the total. These observations are placed in the context of low magnetic shear reconnection made possible in plasmas with low plasma beta.
Key Points
Magnetic reconnection occurs in narrow discrete auroral arcs
Magnetic reconnection can occur for extremely small magnetic shear
Magnetic reconnection contributes <20% to the auroral acceleration energy budget</description><subject>Acceleration</subject><subject>aurora</subject><subject>Auroral arcs</subject><subject>Auroral zones</subject><subject>Auroras</subject><subject>Current sheets</subject><subject>Deposition</subject><subject>electric fields</subject><subject>Energy</subject><subject>Energy budgets</subject><subject>Geophysics</subject><subject>Identification</subject><subject>Imagery</subject><subject>Ionosphere</subject><subject>Magnetic fields</subject><subject>Magnetic reconnection</subject><subject>Magnetohydrodynamics</subject><subject>particle acceleration</subject><subject>Plasmas</subject><subject>Plasmas (physics)</subject><subject>reconnection</subject><subject>Shear</subject><subject>Simulation</subject><subject>Tearing</subject><subject>tearing instability</subject><subject>Three dimensional</subject><subject>vorticity</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNqN0U1Lw0AQBuBFFKwfN39AwIsHozP7ld2jFK1CRRA9h81mUlPSpG4SpP_e1XoQD8XTDMzDMMPL2BnCFQLwaw6oZnPQArXcYxO0UqYGINtnEwAbe57pQ3bU90sAECBwwsyjW7Q01D4J5Lu2JT_UXZvUbTK8UeLG0AXXJM57aii471mgRSwn7KByTU-nP_WYvd7dvkzv0_nT7GF6M0-9AgmpdI47Z60tNSBJLKqyVCXHrDBUKGtIx_siIicFKiGqqvTWaw1GELeuEMfsYrt3Hbr3kfohX9V9vKZxLXVjn6M2ygByrv5DhVBSch3p-R-67MbQxkdytAhGI1dyp9KZMIiG86gut8qHru8DVfk61CsXNjlC_pVL_juXyPmWf9QNbXbafPY8VzyLWX0CY0KLQg</recordid><startdate>20150328</startdate><enddate>20150328</enddate><creator>Chaston, C. C.</creator><general>John Wiley & Sons, Inc</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>7TN</scope><scope>8FD</scope><scope>F1W</scope><scope>FR3</scope><scope>H8D</scope><scope>H96</scope><scope>KL.</scope><scope>KR7</scope><scope>L.G</scope><scope>L7M</scope><scope>7UA</scope><scope>C1K</scope><scope>7SU</scope></search><sort><creationdate>20150328</creationdate><title>Magnetic reconnection in the auroral acceleration region</title><author>Chaston, C. C.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c5040-4aa2aa999d601e41bfdd5d217b8eb598e60074aaea431533ffdc9c66083e29ab3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Acceleration</topic><topic>aurora</topic><topic>Auroral arcs</topic><topic>Auroral zones</topic><topic>Auroras</topic><topic>Current sheets</topic><topic>Deposition</topic><topic>electric fields</topic><topic>Energy</topic><topic>Energy budgets</topic><topic>Geophysics</topic><topic>Identification</topic><topic>Imagery</topic><topic>Ionosphere</topic><topic>Magnetic fields</topic><topic>Magnetic reconnection</topic><topic>Magnetohydrodynamics</topic><topic>particle acceleration</topic><topic>Plasmas</topic><topic>Plasmas (physics)</topic><topic>reconnection</topic><topic>Shear</topic><topic>Simulation</topic><topic>Tearing</topic><topic>tearing instability</topic><topic>Three dimensional</topic><topic>vorticity</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Chaston, C. C.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Oceanic Abstracts</collection><collection>Technology Research Database</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Civil Engineering Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Water Resources Abstracts</collection><collection>Environmental Sciences and Pollution Management</collection><collection>Environmental Engineering Abstracts</collection><jtitle>Geophysical research letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Chaston, C. C.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Magnetic reconnection in the auroral acceleration region</atitle><jtitle>Geophysical research letters</jtitle><date>2015-03-28</date><risdate>2015</risdate><volume>42</volume><issue>6</issue><spage>1646</spage><epage>1653</epage><pages>1646-1653</pages><issn>0094-8276</issn><eissn>1944-8007</eissn><abstract>Evidence is presented for the operation of extreme guide field magnetic reconnection in the presence of sheared flows in a narrow current sheet through the auroral acceleration region. Using auroral imagery, magnetically conjugate particle measurements and a 3‐D reduced MHD simulation, vortical motions in a narrow, rapidly evolving auroral arc indicative of the operation of magnetic tearing are identified. An estimate of the contribution of this process to the observed rate of energy deposition at the ionosphere shows that while this contribution can be significant it remains a minor fraction of the total. These observations are placed in the context of low magnetic shear reconnection made possible in plasmas with low plasma beta.
Key Points
Magnetic reconnection occurs in narrow discrete auroral arcs
Magnetic reconnection can occur for extremely small magnetic shear
Magnetic reconnection contributes <20% to the auroral acceleration energy budget</abstract><cop>Washington</cop><pub>John Wiley & Sons, Inc</pub><doi>10.1002/2015GL063164</doi><tpages>8</tpages><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0094-8276 |
ispartof | Geophysical research letters, 2015-03, Vol.42 (6), p.1646-1653 |
issn | 0094-8276 1944-8007 |
language | eng |
recordid | cdi_proquest_miscellaneous_1685801225 |
source | Wiley-Blackwell AGU Digital Archive |
subjects | Acceleration aurora Auroral arcs Auroral zones Auroras Current sheets Deposition electric fields Energy Energy budgets Geophysics Identification Imagery Ionosphere Magnetic fields Magnetic reconnection Magnetohydrodynamics particle acceleration Plasmas Plasmas (physics) reconnection Shear Simulation Tearing tearing instability Three dimensional vorticity |
title | Magnetic reconnection in the auroral acceleration region |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-03-04T22%3A03%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=Magnetic%20reconnection%20in%20the%20auroral%20acceleration%20region&rft.jtitle=Geophysical%20research%20letters&rft.au=Chaston,%20C.%20C.&rft.date=2015-03-28&rft.volume=42&rft.issue=6&rft.spage=1646&rft.epage=1653&rft.pages=1646-1653&rft.issn=0094-8276&rft.eissn=1944-8007&rft_id=info:doi/10.1002/2015GL063164&rft_dat=%3Cproquest_cross%3E1910861254%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c5040-4aa2aa999d601e41bfdd5d217b8eb598e60074aaea431533ffdc9c66083e29ab3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=1673811822&rft_id=info:pmid/&rfr_iscdi=true |