Article (Scientific journals)
Recurrent energization of plasma in the midnight-to-dawn quadrant of Saturn's magnetosphere, and its relationship to auroral UV and radio emissions
Mitchell, D. G.; Krimigis, S. M.; Paranicas, C. et al.
2009In Planetary and Space Science, 57, p. 1732-1742
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Keywords :
Cassini; Saturn; aurora; magnetosphere
Abstract :
[en] We demonstrate that under some magnetospheric conditions protons and oxygen ions are accelerated once per Saturn magnetosphere rotation, at a preferred local time between midnight and dawn. Although enhancements in energetic neutral atom (ENA) emission may in general occur at any local time and at any time in a Saturn rotation, those enhancements that exhibit a recurrence at a period very close to Saturn's rotation period usually recur in the same magnetospheric location. We suggest that these events result from current sheet acceleration in the 15-20 Rs range, probably associated with reconnection and plasmoid formation in Saturn's magnetotail. Simultaneous auroral observations by the Hubble Space Telescope (HST) and the Cassini Ultraviolet Imaging Spectrometer (UVIS) suggest a close correlation between these dynamical magnetospheric events and dawn-side transient auroral brightenings. Likewise, many of the recurrent ENA enhancements coincide closely with bursts of Saturn kilometric radiation, again pointing to possible linkage with high latitude auroral processes. We argue that the rotating azimuthal asymmetry of the ring current pressure revealed in the ENA images creates an associated rotating field aligned current system linking to the ionosphere and driving the correlated auroral processes.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Mitchell, D. G.;  Johns Hopkins University Applied Physics Laboratory, MP3 E-132, 11100 Johns Hopkins Road, Laurel, MD 21042, USA
Krimigis, S. M.;  Johns Hopkins University Applied Physics Laboratory, MP3 E-132, 11100 Johns Hopkins Road, Laurel, MD 21042, USA
Paranicas, C.;  Johns Hopkins University Applied Physics Laboratory, MP3 E-132, 11100 Johns Hopkins Road, Laurel, MD 21042, USA
Brandt, P. C.;  Johns Hopkins University Applied Physics Laboratory, MP3 E-132, 11100 Johns Hopkins Road, Laurel, MD 21042, USA
Carbary, J. F.;  Johns Hopkins University Applied Physics Laboratory, MP3 E-132, 11100 Johns Hopkins Road, Laurel, MD 21042, USA
Roelof, E. C.;  Johns Hopkins University Applied Physics Laboratory, MP3 E-132, 11100 Johns Hopkins Road, Laurel, MD 21042, USA
Kurth, W. S.;  University of Iowa > Department of Physics and Astronomy
Gurnett, D. A.;  Department of Physics and Astronomy, University of Iowa, Iowa City, IA, USA
Clarke, J. T.;  Center for Space Physics Boston University, Boston, USA
Nichols, J. D.;  Department of Physics and Astronomy, University of Leicester, Leicester, UK
Gérard, Jean-Claude  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Labo de physique atmosphérique et planétaire (LPAP)
Grodent, Denis  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Labo de physique atmosphérique et planétaire (LPAP)
Dougherty, M. K.;  Blackett Laboratory, Imperial College, London, UK
Pryor, W. R.;  Central Arizona College, Coolidge, AZ, USA
More authors (4 more) Less
Language :
English
Title :
Recurrent energization of plasma in the midnight-to-dawn quadrant of Saturn's magnetosphere, and its relationship to auroral UV and radio emissions
Publication date :
01 December 2009
Journal title :
Planetary and Space Science
ISSN :
0032-0633
Publisher :
Pergamon Press - An Imprint of Elsevier Science
Volume :
57
Pages :
1732-1742
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 15 November 2010

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