Stationary flux ropes at the southern terminator of Mars
Flux ropes have long been observed in the upper atmosphere of Venus and more recently at Mars. Here we present magnetic field measurements of flux ropes encountered at the southern terminator of Mars by Mars Global Surveyor and compare them to a flux rope model. This allows several parameters of eac...
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Veröffentlicht in: | Journal of Geophysical Research: Space Physics 2012-12, Vol.117 (A12), p.n/a |
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creator | Beharrell, M. J. Wild, J. A. |
description | Flux ropes have long been observed in the upper atmosphere of Venus and more recently at Mars. Here we present magnetic field measurements of flux ropes encountered at the southern terminator of Mars by Mars Global Surveyor and compare them to a flux rope model. This allows several parameters of each rope to be inferred. Remarkably similar flux ropes are met repeatedly at the southern terminator over a period of the Martian year, when strong crustal magnetic fields are upstream of their position, indicating that they are most likely stationary and attached to the upstream crustal fields. A mechanism is described that could produce the observed flux ropes.
Key Points
Stationary flux ropes identified at the southern terminator of Mars
Formation process proposed for stationary flux ropes at Mars
Flux rope model fitted to observations |
doi_str_mv | 10.1029/2012JA017738 |
format | Article |
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Key Points
Stationary flux ropes identified at the southern terminator of Mars
Formation process proposed for stationary flux ropes at Mars
Flux rope model fitted to observations</description><identifier>ISSN: 0148-0227</identifier><identifier>ISSN: 2169-9380</identifier><identifier>EISSN: 2156-2202</identifier><identifier>EISSN: 2169-9402</identifier><identifier>DOI: 10.1029/2012JA017738</identifier><language>eng</language><publisher>Washington, DC: Blackwell Publishing Ltd</publisher><subject>Astronomy ; Atmospheric sciences ; Earth, ocean, space ; Exact sciences and technology ; Fluctuations ; flux ropes ; Ionospheres; magnetospheres ; Magnetic fields ; Magnetism ; Mars ; Planetary, asteroid, and satellite characteristics and properties ; Planetology ; Planets ; Planets, their satellites and rings. Asteroids ; Solar system ; Upper atmosphere ; Upstream</subject><ispartof>Journal of Geophysical Research: Space Physics, 2012-12, Vol.117 (A12), p.n/a</ispartof><rights>2012 by the American Geophysical Union</rights><rights>2014 INIST-CNRS</rights><rights>Copyright American Geophysical Union 2012</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c4790-44d2c09d66a89ebf88642f9cd2ed6973635c40452103732ec4941cbcd90827db3</citedby><cites>FETCH-LOGICAL-c4790-44d2c09d66a89ebf88642f9cd2ed6973635c40452103732ec4941cbcd90827db3</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%2F2012JA017738$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F2012JA017738$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,776,780,1411,1427,11493,27901,27902,45550,45551,46384,46443,46808,46867</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=26842700$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Beharrell, M. J.</creatorcontrib><creatorcontrib>Wild, J. A.</creatorcontrib><title>Stationary flux ropes at the southern terminator of Mars</title><title>Journal of Geophysical Research: Space Physics</title><addtitle>J. Geophys. Res</addtitle><description>Flux ropes have long been observed in the upper atmosphere of Venus and more recently at Mars. Here we present magnetic field measurements of flux ropes encountered at the southern terminator of Mars by Mars Global Surveyor and compare them to a flux rope model. This allows several parameters of each rope to be inferred. Remarkably similar flux ropes are met repeatedly at the southern terminator over a period of the Martian year, when strong crustal magnetic fields are upstream of their position, indicating that they are most likely stationary and attached to the upstream crustal fields. A mechanism is described that could produce the observed flux ropes.
Key Points
Stationary flux ropes identified at the southern terminator of Mars
Formation process proposed for stationary flux ropes at Mars
Flux rope model fitted to observations</description><subject>Astronomy</subject><subject>Atmospheric sciences</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Fluctuations</subject><subject>flux ropes</subject><subject>Ionospheres; magnetospheres</subject><subject>Magnetic fields</subject><subject>Magnetism</subject><subject>Mars</subject><subject>Planetary, asteroid, and satellite characteristics and properties</subject><subject>Planetology</subject><subject>Planets</subject><subject>Planets, their satellites and rings. Asteroids</subject><subject>Solar system</subject><subject>Upper atmosphere</subject><subject>Upstream</subject><issn>0148-0227</issn><issn>2169-9380</issn><issn>2156-2202</issn><issn>2169-9402</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNp9kE9PAjEQxRujiQS5-QE2Md5cbafd_jkSUJQgJqjh2JRuNy7CLra7Eb69JRjiybm8y--9NzMIXRJ8SzCoO8AExn1MhKDyBHWAZDwFwHCKOpgwmWIAcY56ISxxHJZxhkkHydfGNGVdGb9LilW7TXy9cSExTdJ8uCTUbRRfJY3z67IyTe2TukiejQ8X6Kwwq-B6v9pF7w_3b4PHdPIyehr0J6llQuGUsRwsVjnnRiq3KKTkDAplc3A5V4JymlkWtwGCqaDgLFOM2IXNFZYg8gXtoqtD7sbXX60LjV7Wra9ipSZAVSZI7InUzYGyvg7Bu0JvfLmOR2mC9f49-u97In79G2qCNavCm8qW4egBLhkIjCNHD9x3uXK7fzP1eDTrAwDdu9KDqwyN2x5dxn9qLqjI9Hw60nwwnMn5VOgh_QFsFX-e</recordid><startdate>201212</startdate><enddate>201212</enddate><creator>Beharrell, M. J.</creator><creator>Wild, J. A.</creator><general>Blackwell Publishing Ltd</general><general>American Geophysical Union</general><scope>BSCLL</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><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>BHPHI</scope><scope>BKSAR</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>PCBAR</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope></search><sort><creationdate>201212</creationdate><title>Stationary flux ropes at the southern terminator of Mars</title><author>Beharrell, M. J. ; Wild, J. A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c4790-44d2c09d66a89ebf88642f9cd2ed6973635c40452103732ec4941cbcd90827db3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Astronomy</topic><topic>Atmospheric sciences</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Fluctuations</topic><topic>flux ropes</topic><topic>Ionospheres; magnetospheres</topic><topic>Magnetic fields</topic><topic>Magnetism</topic><topic>Mars</topic><topic>Planetary, asteroid, and satellite characteristics and properties</topic><topic>Planetology</topic><topic>Planets</topic><topic>Planets, their satellites and rings. Asteroids</topic><topic>Solar system</topic><topic>Upper atmosphere</topic><topic>Upstream</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Beharrell, M. J.</creatorcontrib><creatorcontrib>Wild, J. 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J.</au><au>Wild, J. A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Stationary flux ropes at the southern terminator of Mars</atitle><jtitle>Journal of Geophysical Research: Space Physics</jtitle><addtitle>J. Geophys. Res</addtitle><date>2012-12</date><risdate>2012</risdate><volume>117</volume><issue>A12</issue><epage>n/a</epage><issn>0148-0227</issn><issn>2169-9380</issn><eissn>2156-2202</eissn><eissn>2169-9402</eissn><abstract>Flux ropes have long been observed in the upper atmosphere of Venus and more recently at Mars. Here we present magnetic field measurements of flux ropes encountered at the southern terminator of Mars by Mars Global Surveyor and compare them to a flux rope model. This allows several parameters of each rope to be inferred. Remarkably similar flux ropes are met repeatedly at the southern terminator over a period of the Martian year, when strong crustal magnetic fields are upstream of their position, indicating that they are most likely stationary and attached to the upstream crustal fields. A mechanism is described that could produce the observed flux ropes.
Key Points
Stationary flux ropes identified at the southern terminator of Mars
Formation process proposed for stationary flux ropes at Mars
Flux rope model fitted to observations</abstract><cop>Washington, DC</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/2012JA017738</doi><tpages>13</tpages><oa>free_for_read</oa></addata></record> |
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source | Wiley Free Content; Wiley-Blackwell AGU Digital Library; Wiley Online Library Journals Frontfile Complete; Alma/SFX Local Collection |
subjects | Astronomy Atmospheric sciences Earth, ocean, space Exact sciences and technology Fluctuations flux ropes Ionospheres magnetospheres Magnetic fields Magnetism Mars Planetary, asteroid, and satellite characteristics and properties Planetology Planets Planets, their satellites and rings. Asteroids Solar system Upper atmosphere Upstream |
title | Stationary flux ropes at the southern terminator of Mars |
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