Magnetic Reconnection in the Solar Wind
It is only within the last 5 years that we have learned how to recognize the unambiguous signature of magnetic reconnection in the solar wind in the form of roughly Alfvénic accelerated plasma flows embedded within bifurcated magnetic field reversal regions (current sheets). This paper provides a br...
Gespeichert in:
| Veröffentlicht in: | Space science reviews 2012-11, Vol.172 (1-4), p.187-200 |
|---|---|
| 1. Verfasser: | |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 200 |
|---|---|
| container_issue | 1-4 |
| container_start_page | 187 |
| container_title | Space science reviews |
| container_volume | 172 |
| creator | Gosling, J. T. |
| description | It is only within the last 5 years that we have learned how to recognize the unambiguous signature of magnetic reconnection in the solar wind in the form of roughly Alfvénic accelerated plasma flows embedded within bifurcated magnetic field reversal regions (current sheets). This paper provides a brief overview of what has since been learned about reconnection in the solar wind from both single and multi-spacecraft observations of these so-called reconnection exhausts. |
| doi_str_mv | 10.1007/s11214-011-9747-2 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1257759697</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1257759697</sourcerecordid><originalsourceid>FETCH-LOGICAL-c382t-e5e3e3d4f7156c32c7569c1ce24f8d56d4912eabb4d5ad7e424380ec04c2d4513</originalsourceid><addsrcrecordid>eNp1kEtLxDAURoMoOI7-AHcFF7qJ5t4kTbuUwReMCD5wGTrp7dihk45Ju_Df21IXIri6m3M-LoexUxCXIIS5igAIigsAnhtlOO6xGWiDPE8N7rOZEDLjqRTZITuKcSPEaJkZO38s1p662iXP5FrvyXV165PaJ90HJS9tU4TkvfblMTuoiibSyc-ds7fbm9fFPV8-3T0srpfcyQw7TpokyVJVBnTqJDqj09yBI1RVVuq0VDkgFauVKnVRGlKoZCbICeWwVBrknF1Mu7vQfvYUO7uto6OmKTy1fbSA2hidp7kZ0LM_6Kbtgx--swAKFKLSOFAwUS60MQaq7C7U2yJ8WRB2jGCndHZIZ8d0dnRwcuLA-jWFX8v_St8tpm5l</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1141422452</pqid></control><display><type>article</type><title>Magnetic Reconnection in the Solar Wind</title><source>Springer Nature - Complete Springer Journals</source><creator>Gosling, J. T.</creator><creatorcontrib>Gosling, J. T.</creatorcontrib><description>It is only within the last 5 years that we have learned how to recognize the unambiguous signature of magnetic reconnection in the solar wind in the form of roughly Alfvénic accelerated plasma flows embedded within bifurcated magnetic field reversal regions (current sheets). This paper provides a brief overview of what has since been learned about reconnection in the solar wind from both single and multi-spacecraft observations of these so-called reconnection exhausts.</description><identifier>ISSN: 0038-6308</identifier><identifier>EISSN: 1572-9672</identifier><identifier>DOI: 10.1007/s11214-011-9747-2</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Aerospace Technology and Astronautics ; Astrophysics and Astroparticles ; Magnetic fields ; Physics ; Physics and Astronomy ; Planetology ; Solar energy ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Spacecraft ; Wind</subject><ispartof>Space science reviews, 2012-11, Vol.172 (1-4), p.187-200</ispartof><rights>Springer Science+Business Media B.V. 2011</rights><rights>Springer Science+Business Media Dordrecht 2012</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c382t-e5e3e3d4f7156c32c7569c1ce24f8d56d4912eabb4d5ad7e424380ec04c2d4513</citedby><cites>FETCH-LOGICAL-c382t-e5e3e3d4f7156c32c7569c1ce24f8d56d4912eabb4d5ad7e424380ec04c2d4513</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s11214-011-9747-2$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s11214-011-9747-2$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,27901,27902,41464,42533,51294</link.rule.ids></links><search><creatorcontrib>Gosling, J. T.</creatorcontrib><title>Magnetic Reconnection in the Solar Wind</title><title>Space science reviews</title><addtitle>Space Sci Rev</addtitle><description>It is only within the last 5 years that we have learned how to recognize the unambiguous signature of magnetic reconnection in the solar wind in the form of roughly Alfvénic accelerated plasma flows embedded within bifurcated magnetic field reversal regions (current sheets). This paper provides a brief overview of what has since been learned about reconnection in the solar wind from both single and multi-spacecraft observations of these so-called reconnection exhausts.</description><subject>Aerospace Technology and Astronautics</subject><subject>Astrophysics and Astroparticles</subject><subject>Magnetic fields</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Planetology</subject><subject>Solar energy</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Spacecraft</subject><subject>Wind</subject><issn>0038-6308</issn><issn>1572-9672</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNp1kEtLxDAURoMoOI7-AHcFF7qJ5t4kTbuUwReMCD5wGTrp7dihk45Ju_Df21IXIri6m3M-LoexUxCXIIS5igAIigsAnhtlOO6xGWiDPE8N7rOZEDLjqRTZITuKcSPEaJkZO38s1p662iXP5FrvyXV165PaJ90HJS9tU4TkvfblMTuoiibSyc-ds7fbm9fFPV8-3T0srpfcyQw7TpokyVJVBnTqJDqj09yBI1RVVuq0VDkgFauVKnVRGlKoZCbICeWwVBrknF1Mu7vQfvYUO7uto6OmKTy1fbSA2hidp7kZ0LM_6Kbtgx--swAKFKLSOFAwUS60MQaq7C7U2yJ8WRB2jGCndHZIZ8d0dnRwcuLA-jWFX8v_St8tpm5l</recordid><startdate>20121101</startdate><enddate>20121101</enddate><creator>Gosling, J. T.</creator><general>Springer Netherlands</general><general>Springer Nature B.V</general><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>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>20121101</creationdate><title>Magnetic Reconnection in the Solar Wind</title><author>Gosling, J. T.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c382t-e5e3e3d4f7156c32c7569c1ce24f8d56d4912eabb4d5ad7e424380ec04c2d4513</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Aerospace Technology and Astronautics</topic><topic>Astrophysics and Astroparticles</topic><topic>Magnetic fields</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Planetology</topic><topic>Solar energy</topic><topic>Space Exploration and Astronautics</topic><topic>Space Sciences (including Extraterrestrial Physics</topic><topic>Spacecraft</topic><topic>Wind</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gosling, J. T.</creatorcontrib><collection>CrossRef</collection><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>Space science reviews</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gosling, J. T.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Magnetic Reconnection in the Solar Wind</atitle><jtitle>Space science reviews</jtitle><stitle>Space Sci Rev</stitle><date>2012-11-01</date><risdate>2012</risdate><volume>172</volume><issue>1-4</issue><spage>187</spage><epage>200</epage><pages>187-200</pages><issn>0038-6308</issn><eissn>1572-9672</eissn><abstract>It is only within the last 5 years that we have learned how to recognize the unambiguous signature of magnetic reconnection in the solar wind in the form of roughly Alfvénic accelerated plasma flows embedded within bifurcated magnetic field reversal regions (current sheets). This paper provides a brief overview of what has since been learned about reconnection in the solar wind from both single and multi-spacecraft observations of these so-called reconnection exhausts.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s11214-011-9747-2</doi><tpages>14</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0038-6308 |
| ispartof | Space science reviews, 2012-11, Vol.172 (1-4), p.187-200 |
| issn | 0038-6308 1572-9672 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_1257759697 |
| source | Springer Nature - Complete Springer Journals |
| subjects | Aerospace Technology and Astronautics Astrophysics and Astroparticles Magnetic fields Physics Physics and Astronomy Planetology Solar energy Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Spacecraft Wind |
| title | Magnetic Reconnection in the Solar Wind |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-15T19%3A07%3A46IST&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%20Solar%20Wind&rft.jtitle=Space%20science%20reviews&rft.au=Gosling,%20J.%20T.&rft.date=2012-11-01&rft.volume=172&rft.issue=1-4&rft.spage=187&rft.epage=200&rft.pages=187-200&rft.issn=0038-6308&rft.eissn=1572-9672&rft_id=info:doi/10.1007/s11214-011-9747-2&rft_dat=%3Cproquest_cross%3E1257759697%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1141422452&rft_id=info:pmid/&rfr_iscdi=true |