MESSENGER Observations of Magnetic Reconnection in Mercury's Magnetosphere
Solar wind energy transfer to planetary magnetospheres and ionospheres is controlled by magnetic reconnection, a process that determines the degree of connectivity between the interplanetary magnetic field (IMF) and a planet's magnetic field. During MESSENGER's second flyby of Mercury, a s...
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Veröffentlicht in: | Science (American Association for the Advancement of Science) 2009-05, Vol.324 (5927), p.606-610 |
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creator | Slavin, James A Acuña, Mario H Anderson, Brian J Baker, Daniel N Benna, Mehdi Boardsen, Scott A Gloeckler, George Gold, Robert E Ho, George C Korth, Haje Krimigis, Stamatios M McNutt, Ralph L. Jr Raines, Jim M Sarantos, Menelaos Schriver, David Solomon, Sean C Trávníček, Pavel Zurbuchen, Thomas H |
description | Solar wind energy transfer to planetary magnetospheres and ionospheres is controlled by magnetic reconnection, a process that determines the degree of connectivity between the interplanetary magnetic field (IMF) and a planet's magnetic field. During MESSENGER's second flyby of Mercury, a steady southward IMF was observed and the magnetopause was threaded by a strong magnetic field, indicating a reconnection rate approximately 10 times that typical at Earth. Moreover, a large flux transfer event was observed in the magnetosheath, and a plasmoid and multiple traveling compression regions were observed in Mercury's magnetotail, all products of reconnection. These observations indicate that Mercury's magnetosphere is much more responsive to IMF direction and dominated by the effects of reconnection than that of Earth or the other magnetized planets. |
doi_str_mv | 10.1126/science.1172011 |
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Jr ; Raines, Jim M ; Sarantos, Menelaos ; Schriver, David ; Solomon, Sean C ; Trávníček, Pavel ; Zurbuchen, Thomas H</creator><creatorcontrib>Slavin, James A ; Acuña, Mario H ; Anderson, Brian J ; Baker, Daniel N ; Benna, Mehdi ; Boardsen, Scott A ; Gloeckler, George ; Gold, Robert E ; Ho, George C ; Korth, Haje ; Krimigis, Stamatios M ; McNutt, Ralph L. Jr ; Raines, Jim M ; Sarantos, Menelaos ; Schriver, David ; Solomon, Sean C ; Trávníček, Pavel ; Zurbuchen, Thomas H</creatorcontrib><description>Solar wind energy transfer to planetary magnetospheres and ionospheres is controlled by magnetic reconnection, a process that determines the degree of connectivity between the interplanetary magnetic field (IMF) and a planet's magnetic field. During MESSENGER's second flyby of Mercury, a steady southward IMF was observed and the magnetopause was threaded by a strong magnetic field, indicating a reconnection rate approximately 10 times that typical at Earth. Moreover, a large flux transfer event was observed in the magnetosheath, and a plasmoid and multiple traveling compression regions were observed in Mercury's magnetotail, all products of reconnection. These observations indicate that Mercury's magnetosphere is much more responsive to IMF direction and dominated by the effects of reconnection than that of Earth or the other magnetized planets.</description><identifier>ISSN: 0036-8075</identifier><identifier>EISSN: 1095-9203</identifier><identifier>DOI: 10.1126/science.1172011</identifier><identifier>PMID: 19407194</identifier><identifier>CODEN: SCIEAS</identifier><language>eng</language><publisher>Washington, DC: American Association for the Advancement of Science</publisher><subject>Astronomy ; Earth ; Earth, ocean, space ; Electric and magnetic fields ; Exact sciences and technology ; Ionospheres; magnetospheres ; Magnetic fields ; Magnetic flux ; Magnetospheres ; Mercury ; Planetary magnetic fields ; Planetary magnetospheres ; Planetary, asteroid, and satellite characteristics and properties ; Planets, their satellites and rings. 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Jr</au><au>Raines, Jim M</au><au>Sarantos, Menelaos</au><au>Schriver, David</au><au>Solomon, Sean C</au><au>Trávníček, Pavel</au><au>Zurbuchen, Thomas H</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>MESSENGER Observations of Magnetic Reconnection in Mercury's Magnetosphere</atitle><jtitle>Science (American Association for the Advancement of Science)</jtitle><addtitle>Science</addtitle><date>2009-05-01</date><risdate>2009</risdate><volume>324</volume><issue>5927</issue><spage>606</spage><epage>610</epage><pages>606-610</pages><issn>0036-8075</issn><eissn>1095-9203</eissn><coden>SCIEAS</coden><abstract>Solar wind energy transfer to planetary magnetospheres and ionospheres is controlled by magnetic reconnection, a process that determines the degree of connectivity between the interplanetary magnetic field (IMF) and a planet's magnetic field. 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source | Jstor Complete Legacy; Science Online《科学》周刊 |
subjects | Astronomy Earth Earth, ocean, space Electric and magnetic fields Exact sciences and technology Ionospheres magnetospheres Magnetic fields Magnetic flux Magnetospheres Mercury Planetary magnetic fields Planetary magnetospheres Planetary, asteroid, and satellite characteristics and properties Planets, their satellites and rings. Asteroids Plasmas Solar system Solar wind Space exploration Spacecraft |
title | MESSENGER Observations of Magnetic Reconnection in Mercury's Magnetosphere |
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