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Dust-plasma interaction through magnetosphere-ionosphere coupling in Saturn's plasma disk
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Swedish Institute of Space Physics, Uppsala Division. Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Space Plasma Physics.
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2013 (English)In: Planetary and Space Science, ISSN 0032-0633, E-ISSN 1873-5088, Vol. 75, no 1, 11-16 p.Article, review/survey (Refereed) Published
Abstract [en]

The ion bulk speeds in the equatorial region of Saturn's inner magnetosphere, according to data from the Langmuir Probe (LP) on board the Cassini spacecraft, are about 60% of the ideal co-rotation speed; the ion speeds are between the co-rotation and Keplerian speeds (Holmberg et al.; Ion densities and velocities in the inner plasma torus of Saturn, Planetary and Space Science). These findings suggest that sub-micrometer negatively charged E ring dust contributes to the plasma dynamics in the plasma disk. We calculated the ion speeds by using a multi-species fluid model, taking into account dust interactions to investigate the effects of ion-dust coulomb collision, mass loading, as well as taking into account magnetosphere-ionosphere coupling to investigate the effect of the magnetospheric electric field. The results show that the ion speeds can be significantly reduced by the electric fields generated by the collisions between ions and dusts when the dust density is high and the thickness of dust distribution is large. We also show that the ion speeds from our model are consistent with the LP observations when the maximum density of dust is larger than ∼105 m-3.

Place, publisher, year, edition, pages
2013. Vol. 75, no 1, 11-16 p.
Keyword [en]
Co-rotation lag, Dust-plasma interaction, Dusty plasma, Magnetosphere-ionosphere coupling, Saturn
National Category
Natural Sciences
Identifiers
URN: urn:nbn:se:uu:diva-195037DOI: 10.1016/j.pss.2012.11.003ISI: 000315136600002OAI: oai:DiVA.org:uu-195037DiVA: diva2:606834
Available from: 2013-02-20 Created: 2013-02-20 Last updated: 2017-12-06Bibliographically approved

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Holmberg, Madeleine K. G.Wahlund, Jan-Erik

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