Energetic ion acceleration in Saturn's magnetotail: Substorms at Saturn?
Identifieur interne : 000553 ( Istex/Corpus ); précédent : 000552; suivant : 000554Energetic ion acceleration in Saturn's magnetotail: Substorms at Saturn?
Auteurs : D. G. Mitchell ; P. C. Brandt ; E. C. Roelof ; J. Dandouras ; S. M. Krimigis ; B. H. Mauk ; C. P. Paranicas ; N. Krupp ; D. C. Hamilton ; W. S. Kurth ; P. Zarka ; M. K. Dougherty ; E. J. Bunce ; D. E. ShemanskySource :
- Geophysical Research Letters [ 0094-8276 ] ; 2005-10.
Abstract
The Magnetospheric Imaging Instrument (MIMI) Ion and Neutral Camera (INCA) on the Cassini spacecraft has recorded abrupt increases in energetic neutral atom flux coming from the general direction of Saturn's magnetotail. These bursts of ion activity in the tail are well correlated with enhancements in the Saturn kilometric radiation. Given the similarities between these events and substorm activity on Earth, including their dependence on interplanetary conditions, we conclude that Earth‐like substorms occur within Saturn's magnetosphere.
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DOI: 10.1029/2005GL022647
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Mitchell</name><affiliation><mods:affiliation>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</mods:affiliation></affiliation><affiliation><mods:affiliation>E-mail: donald.g.mitchell@jhuapl.edu</mods:affiliation></affiliation></author><author><name sortKey="Brandt, P C" sort="Brandt, P C" uniqKey="Brandt P" first="P. C." last="Brandt">P. C. Brandt</name><affiliation><mods:affiliation>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</mods:affiliation></affiliation></author><author><name sortKey="Roelof, E C" sort="Roelof, E C" uniqKey="Roelof E" first="E. C." last="Roelof">E. C. Roelof</name><affiliation><mods:affiliation>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</mods:affiliation></affiliation></author><author><name sortKey="Dandouras, J" sort="Dandouras, J" uniqKey="Dandouras J" first="J." last="Dandouras">J. Dandouras</name><affiliation><mods:affiliation>Centre D'Etude Spatiale Des Rayonnements, Toulouse, France</mods:affiliation></affiliation></author><author><name sortKey="Krimigis, S M" sort="Krimigis, S M" uniqKey="Krimigis S" first="S. M." last="Krimigis">S. M. Krimigis</name><affiliation><mods:affiliation>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</mods:affiliation></affiliation></author><author><name sortKey="Mauk, B H" sort="Mauk, B H" uniqKey="Mauk B" first="B. H." last="Mauk">B. H. Mauk</name><affiliation><mods:affiliation>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</mods:affiliation></affiliation></author><author><name sortKey="Paranicas, C P" sort="Paranicas, C P" uniqKey="Paranicas C" first="C. P." last="Paranicas">C. P. Paranicas</name><affiliation><mods:affiliation>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</mods:affiliation></affiliation></author><author><name sortKey="Krupp, N" sort="Krupp, N" uniqKey="Krupp N" first="N." last="Krupp">N. Krupp</name><affiliation><mods:affiliation>Max‐Planck‐Institut für Sonnensystemforschung, Lindau, Germany</mods:affiliation></affiliation></author><author><name sortKey="Hamilton, D C" sort="Hamilton, D C" uniqKey="Hamilton D" first="D. C." last="Hamilton">D. C. Hamilton</name><affiliation><mods:affiliation>University of Maryland, Maryland, College Park, USA</mods:affiliation></affiliation></author><author><name sortKey="Kurth, W S" sort="Kurth, W S" uniqKey="Kurth W" first="W. S." last="Kurth">W. S. 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Bunce</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of Leicester, Leicester, U.K</mods:affiliation></affiliation></author><author><name sortKey="Shemansky, D E" sort="Shemansky, D E" uniqKey="Shemansky D" first="D. E." last="Shemansky">D. E. Shemansky</name><affiliation><mods:affiliation>Department of Aerospace Engineering, University of Southern California Los Angeles, California, USA</mods:affiliation></affiliation></author></analytic><monogr></monogr><series><title level="j">Geophysical Research Letters</title><title level="j" type="abbrev">Geophys. Res. Lett.</title><idno type="ISSN">0094-8276</idno><idno type="eISSN">1944-8007</idno><imprint><publisher>Blackwell Publishing Ltd</publisher><date type="published" when="2005-10">2005-10</date><biblScope unit="volume">32</biblScope><biblScope unit="issue">20</biblScope><biblScope unit="page" from="/">n/a</biblScope><biblScope unit="page" to="/">n/a</biblScope></imprint><idno type="ISSN">0094-8276</idno></series><idno type="istex">8544B2A29B7FA8846898C534DA19D03CFAFEA50A</idno><idno type="DOI">10.1029/2005GL022647</idno><idno type="ArticleID">2005GL022647</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0094-8276</idno></seriesStmt></fileDesc><profileDesc><textClass></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract">The Magnetospheric Imaging Instrument (MIMI) Ion and Neutral Camera (INCA) on the Cassini spacecraft has recorded abrupt increases in energetic neutral atom flux coming from the general direction of Saturn's magnetotail. These bursts of ion activity in the tail are well correlated with enhancements in the Saturn kilometric radiation. Given the similarities between these events and substorm activity on Earth, including their dependence on interplanetary conditions, we conclude that Earth‐like substorms occur within Saturn's magnetosphere.</div></front></TEI><istex><corpusName>wiley</corpusName><author><json:item><name>D. G. Mitchell</name><affiliations><json:string>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</json:string><json:string>E-mail: donald.g.mitchell@jhuapl.edu</json:string></affiliations></json:item><json:item><name>P. C. Brandt</name><affiliations><json:string>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</json:string></affiliations></json:item><json:item><name>E. C. 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Shemansky</name><affiliations><json:string>Department of Aerospace Engineering, University of Southern California Los Angeles, California, USA</json:string></affiliations></json:item></author><articleId><json:string>2005GL022647</json:string></articleId><language><json:string>eng</json:string></language><originalGenre><json:string>article</json:string></originalGenre><abstract>The Magnetospheric Imaging Instrument (MIMI) Ion and Neutral Camera (INCA) on the Cassini spacecraft has recorded abrupt increases in energetic neutral atom flux coming from the general direction of Saturn's magnetotail. These bursts of ion activity in the tail are well correlated with enhancements in the Saturn kilometric radiation. Given the similarities between these events and substorm activity on Earth, including their dependence on interplanetary conditions, we conclude that Earth‐like substorms occur within Saturn's magnetosphere.</abstract><qualityIndicators><score>3.816</score><pdfVersion>1.3</pdfVersion><pdfPageSize>592 x 807 pts</pdfPageSize><refBibsNative>true</refBibsNative><abstractCharCount>543</abstractCharCount><pdfWordCount>2916</pdfWordCount><pdfCharCount>17320</pdfCharCount><pdfPageCount>4</pdfPageCount><abstractWordCount>75</abstractWordCount></qualityIndicators><title>Energetic ion acceleration in Saturn's magnetotail: Substorms at Saturn?</title><refBibs><json:item><host><author></author><title>Bagenal, F., T. Dowling, and W. McKinnon (Eds.) (2004), Jupiter: The Planet, Satellites, and Magnetosphere, Cambridge Univ. Press, New York.</title></host></json:item><json:item><author><json:item><name>J. T. Clarke</name></json:item></author><host><volume>433</volume><pages><last>719</last><first>717</first></pages><author></author><title>Nature</title></host><title>Morphological differences of Saturn's ultraviolet aurora compared to those of Earth and Jupiter</title></json:item><json:item><author><json:item><name>A. H. Compton</name></json:item><json:item><name>I. A. Getting</name></json:item></author><host><volume>47</volume><pages><last>821</last><first>817</first></pages><author></author><title>Phys. Rev.</title></host><title>An apparent effect of the galactic rotation on the intensity of cosmic rays</title></json:item><json:item><author><json:item><name>S. W. H. Cowley</name></json:item></author><host><volume>110</volume><author></author><title>J. Geophys. Res.</title></host><title>Reconnection in a rotation‐dominated magnetosphere and its relation to Saturn's auroral dynamics</title></json:item><json:item><author><json:item><name>F. J. Crary</name></json:item></author><host><volume>433</volume><pages><last>722</last><first>720</first></pages><author></author><title>Nature</title></host><title>Solar wind dynamic pressure and electric field as the main factors controlling Saturn's aurorae</title></json:item><json:item><author><json:item><name>D. C. Delcourt</name></json:item></author><host><volume>64</volume><pages><last>559</last><first>551</first></pages><author></author><title>J. Atmos. Sol. Terr. Phys.</title></host><title>Particle acceleration by inductive electric fields in the inner magnetosphere</title></json:item><json:item><author><json:item><name>M. D. Desch</name></json:item></author><host><volume>87</volume><pages><last>4554</last><first>4549</first></pages><author></author><title>J. Geophys. Res.</title></host><title>Evidence for solar wind control of Saturn radio emission</title></json:item><json:item><author><json:item><name>L. W. Esposito</name></json:item></author><host><volume>307</volume><pages><last>1255</last><first>1251</first></pages><author></author><title>Science</title></host><title>Ultraviolet imaging spectroscopy shows an active Saturnian system</title></json:item><json:item><author><json:item><name>C. M. Jackman</name></json:item><json:item><name>N. Achilleos</name></json:item><json:item><name>E. J. Bunce</name></json:item><json:item><name>S. W. H. Cowley</name></json:item><json:item><name>M. K. Dougherty</name></json:item><json:item><name>G. H. Jones</name></json:item><json:item><name>S. E. Milan</name></json:item><json:item><name>E. J. Smith</name></json:item></author><host><volume>109</volume><author></author><title>J. Geophys. Res.</title></host><title>Interplanetary magnetic field at ∼9 AU during the declining phase of the solar cycle and its implications for Saturn's magnetospheric dynamics</title></json:item><json:item><author><json:item><name>S. M. Krimigis</name></json:item></author><host><volume>114</volume><pages><last>329</last><first>233</first></pages><issue>1–4</issue><author></author><title>Space Sci. Rev.</title></host><title>Magnetospheric Imaging Instrument (MIMI) on the Cassini mission to Saturn/Titan</title></json:item><json:item><author><json:item><name>S. M. Krimigis</name></json:item></author><host><volume>307</volume><pages><last>1273</last><first>1270</first></pages><author></author><title>Science</title></host><title>Dynamics of Saturn's magnetosphere from the Magnetosphere Imaging Instrument during Cassini's orbital insertion</title></json:item><json:item><author><json:item><name>N. Krupp</name></json:item></author><host><pages><last>638</last><first>617</first></pages><author></author><title>Jupiter</title></host><title>The dynamics of the Jovian magnetosphere</title></json:item><json:item><author><json:item><name>W. S. Kurth</name></json:item></author><host><volume>433</volume><pages><last>725</last><first>722</first></pages><author></author><title>Nature</title></host><title>An Earth‐like correspondence between Saturn's auroral features and radio emission</title></json:item><json:item><author><json:item><name>R. L. McPherron</name></json:item></author><host><pages><first>400</first></pages><author></author><title>Introduction to Space Physics</title></host><title>Magnetospheric dynamics</title></json:item><json:item><author><json:item><name>R. Nakamura</name></json:item></author><host><volume>29</volume><issue>20</issue><author></author><title>Geophys. Res. Lett.</title></host><title>Motion of the dipolarization front during a flow burst event observed by Cluster</title></json:item><json:item><author><json:item><name>R. Prangé</name></json:item><json:item><name>L. Pallier</name></json:item><json:item><name>K. C. Hansen</name></json:item><json:item><name>R. Howard</name></json:item><json:item><name>A. Vourladis</name></json:item><json:item><name>R. Courtin</name></json:item><json:item><name>C. Parkinson</name></json:item></author><host><volume>432</volume><pages><last>81</last><first>78</first></pages><author></author><title>Nature</title></host><title>An interplanetary shock traced by planetary auroral storms from the Sun to Saturn</title></json:item></refBibs><genre><json:string>article</json:string></genre><host><volume>32</volume><publisherId><json:string>GRL</json:string></publisherId><pages><total>4</total><last>n/a</last><first>n/a</first></pages><issn><json:string>0094-8276</json:string></issn><issue>20</issue><subject><json:item><value>Saturn's Magnetosphere: First Results From Cassini</value></json:item><json:item><value>MAGNETOSPHERIC PHYSICS</value></json:item><json:item><value>Magnetospheric configuration and dynamics</value></json:item><json:item><value>Plasmasphere</value></json:item><json:item><value>Solar wind/magnetosphere interactions</value></json:item><json:item><value>Magnetic storms and substorms</value></json:item><json:item><value>Substorms</value></json:item><json:item><value>NATURAL HAZARDS</value></json:item><json:item><value>Space weather</value></json:item><json:item><value>SPACE WEATHER</value></json:item><json:item><value>Magnetic storms</value></json:item><json:item><value>Space Sciences</value></json:item></subject><genre><json:string>journal</json:string></genre><language><json:string>unknown</json:string></language><eissn><json:string>1944-8007</json:string></eissn><title>Geophysical Research Letters</title><doi><json:string>10.1002/(ISSN)1944-8007</json:string></doi></host><categories><wos><json:string>science</json:string><json:string>geosciences, multidisciplinary</json:string></wos><scienceMetrix><json:string>natural sciences</json:string><json:string>earth & environmental sciences</json:string><json:string>meteorology & atmospheric sciences</json:string></scienceMetrix></categories><publicationDate>2005</publicationDate><copyrightDate>2005</copyrightDate><doi><json:string>10.1029/2005GL022647</json:string></doi><id>8544B2A29B7FA8846898C534DA19D03CFAFEA50A</id><score>0.12044529</score><fulltext><json:item><extension>pdf</extension><original>true</original><mimetype>application/pdf</mimetype><uri>https://api.istex.fr/document/8544B2A29B7FA8846898C534DA19D03CFAFEA50A/fulltext/pdf</uri></json:item><json:item><extension>zip</extension><original>false</original><mimetype>application/zip</mimetype><uri>https://api.istex.fr/document/8544B2A29B7FA8846898C534DA19D03CFAFEA50A/fulltext/zip</uri></json:item><istex:fulltextTEI uri="https://api.istex.fr/document/8544B2A29B7FA8846898C534DA19D03CFAFEA50A/fulltext/tei"><teiHeader><fileDesc><titleStmt><title level="a" type="main" xml:lang="en">Energetic ion acceleration in Saturn's magnetotail: Substorms at Saturn?</title></titleStmt><publicationStmt><authority>ISTEX</authority><publisher>Blackwell Publishing Ltd</publisher><availability><p>Copyright 2005 by the American Geophysical Union.</p></availability><date>2005</date></publicationStmt><sourceDesc><biblStruct type="inbook"><analytic><title level="a" type="main" xml:lang="en">Energetic ion acceleration in Saturn's magnetotail: Substorms at Saturn?</title><author xml:id="author-1"><persName><forename type="first">D. G.</forename><surname>Mitchell</surname></persName><email>donald.g.mitchell@jhuapl.edu</email><affiliation>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</affiliation></author><author xml:id="author-2"><persName><forename type="first">P. C.</forename><surname>Brandt</surname></persName><affiliation>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</affiliation></author><author xml:id="author-3"><persName><forename type="first">E. C.</forename><surname>Roelof</surname></persName><affiliation>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</affiliation></author><author xml:id="author-4"><persName><forename type="first">J.</forename><surname>Dandouras</surname></persName><affiliation>Centre D'Etude Spatiale Des Rayonnements, Toulouse, France</affiliation></author><author xml:id="author-5"><persName><forename type="first">S. M.</forename><surname>Krimigis</surname></persName><affiliation>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</affiliation></author><author xml:id="author-6"><persName><forename type="first">B. H.</forename><surname>Mauk</surname></persName><affiliation>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</affiliation></author><author xml:id="author-7"><persName><forename type="first">C. P.</forename><surname>Paranicas</surname></persName><affiliation>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</affiliation></author><author xml:id="author-8"><persName><forename type="first">N.</forename><surname>Krupp</surname></persName><affiliation>Max‐Planck‐Institut für Sonnensystemforschung, Lindau, Germany</affiliation></author><author xml:id="author-9"><persName><forename type="first">D. C.</forename><surname>Hamilton</surname></persName><affiliation>University of Maryland, Maryland, College Park, USA</affiliation></author><author xml:id="author-10"><persName><forename type="first">W. S.</forename><surname>Kurth</surname></persName><affiliation>Department of Physics and Astronomy, University of Iowa, Iowa, Iowa City, USA</affiliation></author><author xml:id="author-11"><persName><forename type="first">P.</forename><surname>Zarka</surname></persName><affiliation>Observatory of Paris, Meudon, France</affiliation></author><author xml:id="author-12"><persName><forename type="first">M. K.</forename><surname>Dougherty</surname></persName><affiliation>Space and Atmospheric Physics, Imperial College, London, U.K</affiliation></author><author xml:id="author-13"><persName><forename type="first">E. J.</forename><surname>Bunce</surname></persName><affiliation>Department of Physics & Astronomy, University of Leicester, Leicester, U.K</affiliation></author><author xml:id="author-14"><persName><forename type="first">D. E.</forename><surname>Shemansky</surname></persName><affiliation>Department of Aerospace Engineering, University of Southern California Los Angeles, California, USA</affiliation></author></analytic><monogr><title level="j">Geophysical Research Letters</title><title level="j" type="abbrev">Geophys. Res. Lett.</title><idno type="pISSN">0094-8276</idno><idno type="eISSN">1944-8007</idno><idno type="DOI">10.1002/(ISSN)1944-8007</idno><imprint><publisher>Blackwell Publishing Ltd</publisher><date type="published" when="2005-10"></date><biblScope unit="volume">32</biblScope><biblScope unit="issue">20</biblScope><biblScope unit="page" from="/">n/a</biblScope><biblScope unit="page" to="/">n/a</biblScope></imprint></monogr><idno type="istex">8544B2A29B7FA8846898C534DA19D03CFAFEA50A</idno><idno type="DOI">10.1029/2005GL022647</idno><idno type="ArticleID">2005GL022647</idno></biblStruct></sourceDesc></fileDesc><profileDesc><creation><date>2005</date></creation><langUsage><language ident="en">en</language></langUsage><abstract><p>The Magnetospheric Imaging Instrument (MIMI) Ion and Neutral Camera (INCA) on the Cassini spacecraft has recorded abrupt increases in energetic neutral atom flux coming from the general direction of Saturn's magnetotail. These bursts of ion activity in the tail are well correlated with enhancements in the Saturn kilometric radiation. Given the similarities between these events and substorm activity on Earth, including their dependence on interplanetary conditions, we conclude that Earth‐like substorms occur within Saturn's magnetosphere.</p></abstract><textClass><keywords scheme="Journal Subject"><list><head>index-terms</head><item><term>Saturn's Magnetosphere: First Results From Cassini</term></item><item><term>MAGNETOSPHERIC PHYSICS</term></item><item><term>Magnetospheric configuration and dynamics</term></item><item><term>Plasmasphere</term></item><item><term>Solar wind/magnetosphere interactions</term></item><item><term>Magnetic storms and substorms</term></item><item><term>Substorms</term></item><item><term>NATURAL HAZARDS</term></item><item><term>Space weather</term></item><item><term>SPACE WEATHER</term></item><item><term>Magnetic storms</term></item></list></keywords></textClass><textClass><keywords scheme="Journal Subject"><list><head>article-category</head><item><term>Space Sciences</term></item></list></keywords></textClass></profileDesc><revisionDesc><change when="2005-02-07">Received</change><change when="2005-04-07">Registration</change><change when="2005-10">Published</change></revisionDesc></teiHeader></istex:fulltextTEI><json:item><extension>txt</extension><original>false</original><mimetype>text/plain</mimetype><uri>https://api.istex.fr/document/8544B2A29B7FA8846898C534DA19D03CFAFEA50A/fulltext/txt</uri></json:item></fulltext><metadata><istex:metadataXml wicri:clean="Wiley, elements deleted: body"><istex:xmlDeclaration>version="1.0" encoding="UTF-8" standalone="yes"</istex:xmlDeclaration><istex:document><component type="serialArticle" version="2.0" xml:lang="en" xml:id="grl19700"><header><publicationMeta level="product"><doi>10.1002/(ISSN)1944-8007</doi><issn type="print">0094-8276</issn><issn type="electronic">1944-8007</issn><idGroup><id type="product" value="GRL"></id><id type="coden" value="GPRLAJ"></id></idGroup><titleGroup><title type="main" xml:lang="en" sort="GEOPHYSICAL RESEARCH LETTERS">Geophysical Research Letters</title><title type="short">Geophys. Res. 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G.</givenNames></author>, et al. (<pubYear year="2005">2005</pubYear>), <articleTitle>Energetic ion acceleration in Saturn's magnetotail: Substorms at Saturn?</articleTitle> <journalTitle>Geophys. Res. Lett.</journalTitle>, <vol>32</vol>, L20S01, doi:<accessionId ref="info:doi/10.1029/2005GL022647">10.1029/2005GL022647</accessionId>.</citation></selfCitationGroup><linkGroup><link type="toTypesetVersion" href="file:GRL.GRL19700.pdf"></link></linkGroup></publicationMeta><contentMeta><countGroup><count type="figureTotal" number="4"></count></countGroup><titleGroup><title type="main">Energetic ion acceleration in Saturn's magnetotail: Substorms at Saturn?</title><title type="short">SUBSTORMS AT SATURN?</title><title type="shortAuthors">Mitchell <i>et al</i>.</title></titleGroup><creators><creator creatorRole="author" xml:id="grl19700-cr-0001" affiliationRef="#grl19700-aff-0001"><personName><givenNames>D. G.</givenNames> <familyName>Mitchell</familyName></personName><contactDetails><email normalForm="donald.g.mitchell@jhuapl.edu">donald.g.mitchell@jhuapl.edu</email></contactDetails></creator><creator creatorRole="author" xml:id="grl19700-cr-0002" affiliationRef="#grl19700-aff-0001"><personName><givenNames>P. C.</givenNames> <familyName>Brandt</familyName></personName></creator><creator creatorRole="author" xml:id="grl19700-cr-0003" affiliationRef="#grl19700-aff-0001"><personName><givenNames>E. C.</givenNames> <familyName>Roelof</familyName></personName></creator><creator creatorRole="author" xml:id="grl19700-cr-0004" affiliationRef="#grl19700-aff-0002"><personName><givenNames>J.</givenNames> <familyName>Dandouras</familyName></personName></creator><creator creatorRole="author" xml:id="grl19700-cr-0005" affiliationRef="#grl19700-aff-0001"><personName><givenNames>S. 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E.</givenNames> <familyName>Shemansky</familyName></personName></creator></creators><affiliationGroup><affiliation countryCode="US" type="organization" xml:id="grl19700-aff-0001"><orgDiv>Applied Physics Laboratory</orgDiv><orgName>Johns Hopkins University</orgName><address><city>Laurel</city><countryPart>Maryland</countryPart><country>USA</country></address></affiliation><affiliation countryCode="FR" type="organization" xml:id="grl19700-aff-0002"><orgName>Centre D'Etude Spatiale Des Rayonnements</orgName><address><city>Toulouse</city><country>France</country></address></affiliation><affiliation countryCode="DE" type="organization" xml:id="grl19700-aff-0003"><orgName>Max‐Planck‐Institut für Sonnensystemforschung</orgName><address><city>Lindau</city><country>Germany</country></address></affiliation><affiliation countryCode="US" type="organization" xml:id="grl19700-aff-0004"><orgName>University of Maryland</orgName><address><city>College Park</city><countryPart>Maryland</countryPart><country>USA</country></address></affiliation><affiliation countryCode="US" type="organization" xml:id="grl19700-aff-0005"><orgDiv>Department of Physics and Astronomy</orgDiv><orgName>University of Iowa</orgName><address><city>Iowa City</city><countryPart>Iowa</countryPart><country>USA</country></address></affiliation><affiliation countryCode="FR" type="organization" xml:id="grl19700-aff-0006"><orgName>Observatory of Paris</orgName><address><city>Meudon</city><country>France</country></address></affiliation><affiliation type="organization" xml:id="grl19700-aff-0007"><orgDiv>Space and Atmospheric Physics</orgDiv><orgName>Imperial College</orgName><address><city>London</city><country>U.K</country></address></affiliation><affiliation type="organization" xml:id="grl19700-aff-0008"><orgDiv>Department of Physics & Astronomy</orgDiv><orgName>University of Leicester</orgName><address><city>Leicester</city><country>U.K</country></address></affiliation><affiliation countryCode="US" type="organization" xml:id="grl19700-aff-0009"><orgDiv>Department of Aerospace Engineering</orgDiv><orgName>University of Southern California Los Angeles</orgName><address><countryPart>California</countryPart><country>USA</country></address></affiliation></affiliationGroup><abstractGroup><abstract type="main"><p xml:id="grl19700-para-0001" label="1">The Magnetospheric Imaging Instrument (MIMI) Ion and Neutral Camera (INCA) on the Cassini spacecraft has recorded abrupt increases in energetic neutral atom flux coming from the general direction of Saturn's magnetotail. These bursts of ion activity in the tail are well correlated with enhancements in the Saturn kilometric radiation. Given the similarities between these events and substorm activity on Earth, including their dependence on interplanetary conditions, we conclude that Earth‐like substorms occur within Saturn's magnetosphere.</p></abstract></abstractGroup></contentMeta></header></component></istex:document></istex:metadataXml><mods version="3.6"><titleInfo lang="en"><title>Energetic ion acceleration in Saturn's magnetotail: Substorms at Saturn?</title></titleInfo><titleInfo type="abbreviated" lang="en"><title>SUBSTORMS AT SATURN?</title></titleInfo><titleInfo type="alternative" contentType="CDATA" lang="en"><title>Energetic ion acceleration in Saturn's magnetotail: Substorms at Saturn?</title></titleInfo><name type="personal"><namePart type="given">D. G.</namePart><namePart type="family">Mitchell</namePart><affiliation>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</affiliation><affiliation>E-mail: donald.g.mitchell@jhuapl.edu</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">P. C.</namePart><namePart type="family">Brandt</namePart><affiliation>Applied Physics Laboratory, Johns Hopkins University, Maryland, Laurel, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">E. 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J.</namePart><namePart type="family">Bunce</namePart><affiliation>Department of Physics & Astronomy, University of Leicester, Leicester, U.K</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">D. E.</namePart><namePart type="family">Shemansky</namePart><affiliation>Department of Aerospace Engineering, University of Southern California Los Angeles, California, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><typeOfResource>text</typeOfResource><genre type="article" displayLabel="article"></genre><originInfo><publisher>Blackwell Publishing Ltd</publisher><dateIssued encoding="w3cdtf">2005-10</dateIssued><dateCaptured encoding="w3cdtf">2005-02-07</dateCaptured><dateValid encoding="w3cdtf">2005-04-07</dateValid><edition>Mitchell, D. G., et al. (2005), Energetic ion acceleration in Saturn's magnetotail: Substorms at Saturn? Geophys. Res. Lett., 32, L20S01, doi:10.1029/2005GL022647.</edition><copyrightDate encoding="w3cdtf">2005</copyrightDate></originInfo><language><languageTerm type="code" authority="rfc3066">en</languageTerm><languageTerm type="code" authority="iso639-2b">eng</languageTerm></language><physicalDescription><internetMediaType>text/html</internetMediaType><extent unit="figures">4</extent></physicalDescription><abstract>The Magnetospheric Imaging Instrument (MIMI) Ion and Neutral Camera (INCA) on the Cassini spacecraft has recorded abrupt increases in energetic neutral atom flux coming from the general direction of Saturn's magnetotail. These bursts of ion activity in the tail are well correlated with enhancements in the Saturn kilometric radiation. Given the similarities between these events and substorm activity on Earth, including their dependence on interplanetary conditions, we conclude that Earth‐like substorms occur within Saturn's magnetosphere.</abstract><relatedItem type="host"><titleInfo><title>Geophysical Research Letters</title></titleInfo><titleInfo type="abbreviated"><title>Geophys. Res. Lett.</title></titleInfo><genre type="journal">journal</genre><subject><genre>index-terms</genre><topic authorityURI="http://psi.agu.org/specialSection/CASSINI1">Saturn's Magnetosphere: First Results From Cassini</topic><topic authorityURI="http://psi.agu.org/taxonomy5/2700">MAGNETOSPHERIC PHYSICS</topic><topic authorityURI="http://psi.agu.org/taxonomy5/2740">Magnetospheric configuration and dynamics</topic><topic authorityURI="http://psi.agu.org/taxonomy5/2768">Plasmasphere</topic><topic authorityURI="http://psi.agu.org/taxonomy5/2784">Solar wind/magnetosphere interactions</topic><topic authorityURI="http://psi.agu.org/taxonomy5/2788">Magnetic storms and substorms</topic><topic authorityURI="http://psi.agu.org/taxonomy5/2790">Substorms</topic><topic authorityURI="http://psi.agu.org/taxonomy5/4300">NATURAL HAZARDS</topic><topic authorityURI="http://psi.agu.org/taxonomy5/4305">Space weather</topic><topic authorityURI="http://psi.agu.org/taxonomy5/7900">SPACE WEATHER</topic><topic authorityURI="http://psi.agu.org/taxonomy5/7954">Magnetic storms</topic></subject><subject><genre>article-category</genre><topic>Space Sciences</topic></subject><identifier type="ISSN">0094-8276</identifier><identifier type="eISSN">1944-8007</identifier><identifier type="DOI">10.1002/(ISSN)1944-8007</identifier><identifier type="CODEN">GPRLAJ</identifier><identifier type="PublisherID">GRL</identifier><part><date>2005</date><detail type="volume"><caption>vol.</caption><number>32</number></detail><detail type="issue"><caption>no.</caption><number>20</number></detail><extent unit="pages"><start>n/a</start><end>n/a</end><total>4</total></extent></part></relatedItem><identifier type="istex">8544B2A29B7FA8846898C534DA19D03CFAFEA50A</identifier><identifier type="DOI">10.1029/2005GL022647</identifier><identifier type="ArticleID">2005GL022647</identifier><accessCondition type="use and reproduction" contentType="copyright">Copyright 2005 by the American Geophysical Union.</accessCondition><recordInfo><recordContentSource>WILEY</recordContentSource></recordInfo></mods></metadata><serie></serie></istex></record>Pour manipuler ce document sous Unix (Dilib)
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