Energetic ion acceleration in Saturn's magnetotail: Substorms at Saturn?
Identifieur interne : 002C66 ( Main/Exploration ); précédent : 002C65; suivant : 002C67Energetic ion acceleration in Saturn's magnetotail: Substorms at Saturn?
Auteurs : D. G. Mitchell [États-Unis] ; P. C. Brandt [États-Unis] ; E. C. Roelof [États-Unis] ; J. Dandouras [France] ; S. M. Krimigis [États-Unis] ; B. H. Mauk [États-Unis] ; C. P. Paranicas [États-Unis] ; N. Krupp [Allemagne] ; D. C. Hamilton [États-Unis] ; W. S. Kurth [États-Unis] ; P. Zarka [France] ; M. K. Dougherty [Royaume-Uni] ; E. J. Bunce [Royaume-Uni] ; D. E. Shemansky [États-Unis]Source :
- 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.
Url:
DOI: 10.1029/2005GL022647
Affiliations:
- Allemagne, France, Royaume-Uni, États-Unis
- Angleterre, Californie, Grand Londres, Iowa, Maryland, Midi-Pyrénées, Occitanie (région administrative)
- College Park (Maryland), Iowa City, Londres, Toulouse
- Université de l'Iowa, Université du Maryland
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Bunce</name><affiliation wicri:level="1"><country xml:lang="fr">Royaume-Uni</country><wicri:regionArea>Department of Physics & Astronomy, University of Leicester, Leicester</wicri:regionArea><wicri:noRegion>Leicester</wicri:noRegion></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 wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Aerospace Engineering, University of Southern California Los Angeles, California</wicri:regionArea><placeName><region type="state">Californie</region></placeName></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><affiliations><list><country><li>Allemagne</li><li>France</li><li>Royaume-Uni</li><li>États-Unis</li></country><region><li>Angleterre</li><li>Californie</li><li>Grand Londres</li><li>Iowa</li><li>Maryland</li><li>Midi-Pyrénées</li><li>Occitanie (région administrative)</li></region><settlement><li>College Park (Maryland)</li><li>Iowa City</li><li>Londres</li><li>Toulouse</li></settlement><orgName><li>Université de l'Iowa</li><li>Université du Maryland</li></orgName></list><tree><country name="États-Unis"><noRegion><name sortKey="Mitchell, D G" sort="Mitchell, D G" uniqKey="Mitchell D" first="D. G." last="Mitchell">D. G. Mitchell</name></noRegion><name sortKey="Brandt, P C" sort="Brandt, P C" uniqKey="Brandt P" first="P. C." last="Brandt">P. C. Brandt</name><name sortKey="Hamilton, D C" sort="Hamilton, D C" uniqKey="Hamilton D" first="D. C." last="Hamilton">D. C. Hamilton</name><name sortKey="Krimigis, S M" sort="Krimigis, S M" uniqKey="Krimigis S" first="S. M." last="Krimigis">S. M. Krimigis</name><name sortKey="Kurth, W S" sort="Kurth, W S" uniqKey="Kurth W" first="W. S." last="Kurth">W. S. Kurth</name><name sortKey="Mauk, B H" sort="Mauk, B H" uniqKey="Mauk B" first="B. H." last="Mauk">B. H. Mauk</name><name sortKey="Mitchell, D G" sort="Mitchell, D G" uniqKey="Mitchell D" first="D. G." last="Mitchell">D. G. Mitchell</name><name sortKey="Paranicas, C P" sort="Paranicas, C P" uniqKey="Paranicas C" first="C. P." last="Paranicas">C. P. Paranicas</name><name sortKey="Roelof, E C" sort="Roelof, E C" uniqKey="Roelof E" first="E. C." last="Roelof">E. C. 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