Induced magnetosphere and its outer boundary at Venus
The induced magnetosphere at Venus consists of regions near the planet and its wake for which the magnetic pressure dominates all other pressure contributions. Initial Venus Express measurements indicate a well‐defined outer boundary, the magnetopause, of the induced magnetosphere. This magnetopause...
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Veröffentlicht in: | Journal of Geophysical Research. E. Planets 2008-09, Vol.113 (E9), p.n/a |
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container_title | Journal of Geophysical Research. E. Planets |
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creator | Zhang, T. L. Delva, M. Baumjohann, W. Volwerk, M. Russell, C. T. Wei, H. Y. Wang, C. Balikhin, M. Barabash, S. Auster, H.-U. Kudela, K. |
description | The induced magnetosphere at Venus consists of regions near the planet and its wake for which the magnetic pressure dominates all other pressure contributions. Initial Venus Express measurements indicate a well‐defined outer boundary, the magnetopause, of the induced magnetosphere. This magnetopause acts as an obstacle to deflect the solar wind. Across this boundary, the magnetic field exhibits abrupt directional changes and pronounced draping. In this paper, we examine the structure of the magnetopause using Venus Express magnetic measurements. We find that the magnetopause is a directional discontinuity resembling either a tangential or a rotational discontinuity depending on the interplanetary magnetic field orientation. |
doi_str_mv | 10.1029/2008JE003215 |
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L. ; Delva, M. ; Baumjohann, W. ; Volwerk, M. ; Russell, C. T. ; Wei, H. Y. ; Wang, C. ; Balikhin, M. ; Barabash, S. ; Auster, H.-U. ; Kudela, K.</creator><creatorcontrib>Zhang, T. L. ; Delva, M. ; Baumjohann, W. ; Volwerk, M. ; Russell, C. T. ; Wei, H. Y. ; Wang, C. ; Balikhin, M. ; Barabash, S. ; Auster, H.-U. ; Kudela, K.</creatorcontrib><description>The induced magnetosphere at Venus consists of regions near the planet and its wake for which the magnetic pressure dominates all other pressure contributions. Initial Venus Express measurements indicate a well‐defined outer boundary, the magnetopause, of the induced magnetosphere. This magnetopause acts as an obstacle to deflect the solar wind. Across this boundary, the magnetic field exhibits abrupt directional changes and pronounced draping. In this paper, we examine the structure of the magnetopause using Venus Express magnetic measurements. We find that the magnetopause is a directional discontinuity resembling either a tangential or a rotational discontinuity depending on the interplanetary magnetic field orientation.</description><identifier>ISSN: 0148-0227</identifier><identifier>EISSN: 2156-2202</identifier><identifier>DOI: 10.1029/2008JE003215</identifier><language>eng</language><publisher>Blackwell Publishing Ltd</publisher><subject>induced magnetosphere ; magnetopause ; Venus Express</subject><ispartof>Journal of Geophysical Research. E. 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Across this boundary, the magnetic field exhibits abrupt directional changes and pronounced draping. In this paper, we examine the structure of the magnetopause using Venus Express magnetic measurements. We find that the magnetopause is a directional discontinuity resembling either a tangential or a rotational discontinuity depending on the interplanetary magnetic field orientation.</description><subject>induced magnetosphere</subject><subject>magnetopause</subject><subject>Venus Express</subject><issn>0148-0227</issn><issn>2156-2202</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2008</creationdate><recordtype>article</recordtype><recordid>eNp9kMtOwzAQRS0EElXpjg_IihWB8Suxl9CW0lIB4r2znNiGQJoUOxH07wkKQqyYxcxizh3duQjtYzjCQOQxARCLKQAlmG-hQdeTmBAg22gAmIkYCEl30SiEV-iK8YQBHiA-r0ybWxOt9HNlmzqsX6y3ka5MVDQhqtvG-iir28pov4l0Ez3Yqg17aMfpMtjRzxyi-7Pp3fg8Xl7N5uOTZZwzTHGcaW4AS5dnTmgjmSOZNInGHKdUujQxXIIBwqSTQnR7mhDBbOYSISjNwNIhOujvrn393trQqFURcluWurJ1G1T3XioIFx142IO5r0Pw1qm1L1adZYVBfcej_sbT4aTHP4rSbv5l1WJ2MyU8xZ0o7kVFaOznr0j7N5WkNOXq8XKmntjt5GJyDeqUfgH0V3N4</recordid><startdate>200809</startdate><enddate>200809</enddate><creator>Zhang, T. L.</creator><creator>Delva, M.</creator><creator>Baumjohann, W.</creator><creator>Volwerk, M.</creator><creator>Russell, C. T.</creator><creator>Wei, H. Y.</creator><creator>Wang, C.</creator><creator>Balikhin, M.</creator><creator>Barabash, S.</creator><creator>Auster, H.-U.</creator><creator>Kudela, K.</creator><general>Blackwell Publishing Ltd</general><scope>BSCLL</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>F1W</scope><scope>H96</scope><scope>KL.</scope><scope>L.G</scope></search><sort><creationdate>200809</creationdate><title>Induced magnetosphere and its outer boundary at Venus</title><author>Zhang, T. L. ; Delva, M. ; Baumjohann, W. ; Volwerk, M. ; Russell, C. T. ; Wei, H. 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Y.</creatorcontrib><creatorcontrib>Wang, C.</creatorcontrib><creatorcontrib>Balikhin, M.</creatorcontrib><creatorcontrib>Barabash, S.</creatorcontrib><creatorcontrib>Auster, H.-U.</creatorcontrib><creatorcontrib>Kudela, K.</creatorcontrib><collection>Istex</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><jtitle>Journal of Geophysical Research. E. Planets</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Zhang, T. L.</au><au>Delva, M.</au><au>Baumjohann, W.</au><au>Volwerk, M.</au><au>Russell, C. T.</au><au>Wei, H. Y.</au><au>Wang, C.</au><au>Balikhin, M.</au><au>Barabash, S.</au><au>Auster, H.-U.</au><au>Kudela, K.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Induced magnetosphere and its outer boundary at Venus</atitle><jtitle>Journal of Geophysical Research. E. Planets</jtitle><addtitle>J. Geophys. Res</addtitle><date>2008-09</date><risdate>2008</risdate><volume>113</volume><issue>E9</issue><epage>n/a</epage><issn>0148-0227</issn><eissn>2156-2202</eissn><abstract>The induced magnetosphere at Venus consists of regions near the planet and its wake for which the magnetic pressure dominates all other pressure contributions. Initial Venus Express measurements indicate a well‐defined outer boundary, the magnetopause, of the induced magnetosphere. This magnetopause acts as an obstacle to deflect the solar wind. Across this boundary, the magnetic field exhibits abrupt directional changes and pronounced draping. In this paper, we examine the structure of the magnetopause using Venus Express magnetic measurements. We find that the magnetopause is a directional discontinuity resembling either a tangential or a rotational discontinuity depending on the interplanetary magnetic field orientation.</abstract><pub>Blackwell Publishing Ltd</pub><doi>10.1029/2008JE003215</doi><tpages>9</tpages></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 | induced magnetosphere magnetopause Venus Express |
title | Induced magnetosphere and its outer boundary at Venus |
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