Magnetospheric ion influence on magnetic reconnection at the duskside magnetopause
Magnetospheric ions from the ring current, warm plasma cloak, and the plasmaspheric drainage plume all interact with the dusk flank magnetopause. During periods of strong magnetospheric convection, these ions may contribute significantly to the magnetospheric mass density at the magnetopause. Observ...
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| Veröffentlicht in: | Geophysical research letters 2016-02, Vol.43 (4), p.1435-1442 |
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| creator | Fuselier, S. A. Burch, J. L. Cassak, P. A. Goldstein, J. Gomez, R. G. Goodrich, K. Lewis, W. S. Malaspina, D. Mukherjee, J. Nakamura, R. Petrinec, S. M. Russell, C. T. Strangeway, R. J. Torbert, R. B. Trattner, K. J. Valek, P. |
| description | Magnetospheric ions from the ring current, warm plasma cloak, and the plasmaspheric drainage plume all interact with the dusk flank magnetopause. During periods of strong magnetospheric convection, these ions may contribute significantly to the magnetospheric mass density at the magnetopause. Observations from the Magnetospheric Multiscale mission Hot Plasma Composition Analyzer at the duskside magnetopause near reconnection X lines show that ions from the ring current and warm plasma cloak may have high mass densities. However, these mass densities are not as large as the mass density in the magnetosheath. The results suggest that except for possible influence from the plasmaspheric drainage plume, the other major magnetospheric ion populations do not greatly influence asymmetric reconnection at the duskside magnetopause.
Key Points
Magnetospheric ions have significant density at the magnetopause
Magnetospheric ions do not influence reconnection significantly at the duskside magnetopause |
| doi_str_mv | 10.1002/2015GL067358 |
| format | Article |
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Key Points
Magnetospheric ions have significant density at the magnetopause
Magnetospheric ions do not influence reconnection significantly at the duskside magnetopause</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1002/2015GL067358</identifier><language>eng</language><publisher>Washington: John Wiley & Sons, Inc</publisher><subject>Analyzers ; Asymmetry ; boundary layers ; Convection ; Density ; Drainage ; Geophysics ; Ions ; Lines ; Magnetic fields ; Magnetic reconnection ; Magnetopause ; Magnetosheath ; Magnetospheres ; magnetosphere‐solar wind interaction ; Magnetospheric convection ; Magnetospheric ions ; magnetospheric Plasma ; Mass ; Multiscale analysis ; Plasma composition ; Plumes ; Populations ; Ring currents</subject><ispartof>Geophysical research letters, 2016-02, Vol.43 (4), p.1435-1442</ispartof><rights>2016. American Geophysical Union. All Rights Reserved.</rights><rights>Copyright Blackwell Publishing Ltd. Feb 2016</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c5080-82ea4434982313b234a75447bf94a1674cd4a33d5efada5e3838f8ea968336c03</citedby><cites>FETCH-LOGICAL-c5080-82ea4434982313b234a75447bf94a1674cd4a33d5efada5e3838f8ea968336c03</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%2F2015GL067358$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1002%2F2015GL067358$$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></links><search><creatorcontrib>Fuselier, S. A.</creatorcontrib><creatorcontrib>Burch, J. L.</creatorcontrib><creatorcontrib>Cassak, P. A.</creatorcontrib><creatorcontrib>Goldstein, J.</creatorcontrib><creatorcontrib>Gomez, R. G.</creatorcontrib><creatorcontrib>Goodrich, K.</creatorcontrib><creatorcontrib>Lewis, W. S.</creatorcontrib><creatorcontrib>Malaspina, D.</creatorcontrib><creatorcontrib>Mukherjee, J.</creatorcontrib><creatorcontrib>Nakamura, R.</creatorcontrib><creatorcontrib>Petrinec, S. M.</creatorcontrib><creatorcontrib>Russell, C. T.</creatorcontrib><creatorcontrib>Strangeway, R. J.</creatorcontrib><creatorcontrib>Torbert, R. B.</creatorcontrib><creatorcontrib>Trattner, K. J.</creatorcontrib><creatorcontrib>Valek, P.</creatorcontrib><title>Magnetospheric ion influence on magnetic reconnection at the duskside magnetopause</title><title>Geophysical research letters</title><description>Magnetospheric ions from the ring current, warm plasma cloak, and the plasmaspheric drainage plume all interact with the dusk flank magnetopause. During periods of strong magnetospheric convection, these ions may contribute significantly to the magnetospheric mass density at the magnetopause. Observations from the Magnetospheric Multiscale mission Hot Plasma Composition Analyzer at the duskside magnetopause near reconnection X lines show that ions from the ring current and warm plasma cloak may have high mass densities. However, these mass densities are not as large as the mass density in the magnetosheath. The results suggest that except for possible influence from the plasmaspheric drainage plume, the other major magnetospheric ion populations do not greatly influence asymmetric reconnection at the duskside magnetopause.
Key Points
Magnetospheric ions have significant density at the magnetopause
Magnetospheric ions do not influence reconnection significantly at the duskside magnetopause</description><subject>Analyzers</subject><subject>Asymmetry</subject><subject>boundary layers</subject><subject>Convection</subject><subject>Density</subject><subject>Drainage</subject><subject>Geophysics</subject><subject>Ions</subject><subject>Lines</subject><subject>Magnetic fields</subject><subject>Magnetic reconnection</subject><subject>Magnetopause</subject><subject>Magnetosheath</subject><subject>Magnetospheres</subject><subject>magnetosphere‐solar wind interaction</subject><subject>Magnetospheric convection</subject><subject>Magnetospheric ions</subject><subject>magnetospheric Plasma</subject><subject>Mass</subject><subject>Multiscale analysis</subject><subject>Plasma composition</subject><subject>Plumes</subject><subject>Populations</subject><subject>Ring currents</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><recordid>eNqF0cFKxEAMANBBFFxXb35AwYsHVzOTTGfmKKKrsCKInss4TbXabddOi_j3jq4H8aCnJOQREiLEvoRjCaBOFEg9X0BuUNsNMZGOaGYBzKaYALiUK5Nvi50YnwEAAeVE3F77x5aHLq6euK9DVndtVrdVM3IbOEvF8qufOj2Hrm05DJ_ED9nwxFk5xpdYl_ytupUfI--Krco3kfe-41TcX5zfnV3OFjfzq7PTxSxosJCWYU-E5KxCiQ8KyRtNZB4qR17mhkJJHrHUXPnSa0aLtrLsXW4R8wA4FYfruau-ex05DsWyjoGbxrfcjbGQ6XRyqHP3PzVWK1RENtGDX_S5G_s2HVJIB0ZbVC7_UxlDGnNLMqmjtQp9F2PPVbHq66Xv3wsJxefHip8fS1yt-Vvd8PuftpjfLjQBAX4AqOaUmw</recordid><startdate>20160228</startdate><enddate>20160228</enddate><creator>Fuselier, S. 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L. ; Cassak, P. A. ; Goldstein, J. ; Gomez, R. G. ; Goodrich, K. ; Lewis, W. S. ; Malaspina, D. ; Mukherjee, J. ; Nakamura, R. ; Petrinec, S. M. ; Russell, C. T. ; Strangeway, R. J. ; Torbert, R. B. ; Trattner, K. 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A.</au><au>Burch, J. L.</au><au>Cassak, P. A.</au><au>Goldstein, J.</au><au>Gomez, R. G.</au><au>Goodrich, K.</au><au>Lewis, W. S.</au><au>Malaspina, D.</au><au>Mukherjee, J.</au><au>Nakamura, R.</au><au>Petrinec, S. M.</au><au>Russell, C. T.</au><au>Strangeway, R. J.</au><au>Torbert, R. B.</au><au>Trattner, K. J.</au><au>Valek, P.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Magnetospheric ion influence on magnetic reconnection at the duskside magnetopause</atitle><jtitle>Geophysical research letters</jtitle><date>2016-02-28</date><risdate>2016</risdate><volume>43</volume><issue>4</issue><spage>1435</spage><epage>1442</epage><pages>1435-1442</pages><issn>0094-8276</issn><eissn>1944-8007</eissn><abstract>Magnetospheric ions from the ring current, warm plasma cloak, and the plasmaspheric drainage plume all interact with the dusk flank magnetopause. During periods of strong magnetospheric convection, these ions may contribute significantly to the magnetospheric mass density at the magnetopause. Observations from the Magnetospheric Multiscale mission Hot Plasma Composition Analyzer at the duskside magnetopause near reconnection X lines show that ions from the ring current and warm plasma cloak may have high mass densities. However, these mass densities are not as large as the mass density in the magnetosheath. The results suggest that except for possible influence from the plasmaspheric drainage plume, the other major magnetospheric ion populations do not greatly influence asymmetric reconnection at the duskside magnetopause.
Key Points
Magnetospheric ions have significant density at the magnetopause
Magnetospheric ions do not influence reconnection significantly at the duskside magnetopause</abstract><cop>Washington</cop><pub>John Wiley & Sons, Inc</pub><doi>10.1002/2015GL067358</doi><tpages>8</tpages><oa>free_for_read</oa></addata></record> |
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| ispartof | Geophysical research letters, 2016-02, Vol.43 (4), p.1435-1442 |
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| language | eng |
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| source | Wiley Journals; Wiley-Blackwell AGU Digital Library; EZB-FREE-00999 freely available EZB journals; Wiley Online Library (Open Access Collection) |
| subjects | Analyzers Asymmetry boundary layers Convection Density Drainage Geophysics Ions Lines Magnetic fields Magnetic reconnection Magnetopause Magnetosheath Magnetospheres magnetosphere‐solar wind interaction Magnetospheric convection Magnetospheric ions magnetospheric Plasma Mass Multiscale analysis Plasma composition Plumes Populations Ring currents |
| title | Magnetospheric ion influence on magnetic reconnection at the duskside magnetopause |
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