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Plasma regions, cha...
Plasma regions, charged dust and field-aligned currents near Enceladus
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- Engelhardt, Ilka. A. D. (author)
- Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen,Rymd- och plasmafysik
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- Wahlund, Jan -Erik (author)
- Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
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- Andrews, David J. (author)
- Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
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- Eriksson, Anders. I. (author)
- Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
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- Ye, S. (author)
- Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA.
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- Kurth, W. S. (author)
- Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA.
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- Gurnett, D. A. (author)
- Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA.
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- Morooka, M. W. (author)
- Univ Colorado, Atmospher & Space Phys Lab, Boulder, CO 80303 USA.
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- Farrell, W. M. (author)
- NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA.
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- Dougherty, M. K. (author)
- Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London SW7 2BZ, England.
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(creator_code:org_t)
- Elsevier BV, 2015
- 2015
- English.
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In: Planetary and Space Science. - : Elsevier BV. - 0032-0633 .- 1873-5088. ; 117, s. 453-469
- Related links:
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https://urn.kb.se/re...
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https://doi.org/10.1...
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Abstract
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- We use data from several instruments on board Cassini to determine the characteristics of the plasma and dust regions around Saturn's moon Enceladus. For this we utilize the Langmuir probe and the electric antenna connected to the wideband receiver of the radio and plasma wave science (RPWS) instrument package as well as the magnetometer (MAG). We show that there are several distinct plasma and dust regions around Enceladus. Specifically they are the plume filled with neutral gas, plasma, and charged dust, with a distinct edge boundary region. Here we present observations of a new distinct plasma region, being a dust trail on the downstream side. This is seen both as a difference in ion and electron densities, indicating the presence of charged dust, and directly from the signals created on RPWS antennas by the dust impacts on the spacecraft. Furthermore, we show a very good scaling of these two independent dust density measurement methods over four orders of magnitude in dust density, thereby for the first time cross-validating them. To establish equilibrium with the surrounding plasma the dust becomes negatively charged by attracting free electrons. The dust distribution follows a simple power law and the smallest dust particles in the dust trail region are found to be 10 nm in size as well as in the edge region around the plume. Inside the plume the presence of even smaller particles of about 1 nm is inferred. From the magnetic field measurements we infer strong field-aligned currents at the geometrical edge of Enceladus.
Subject headings
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Keyword
- Enceladus
- Langmuir probe
- Plasma
- Charged dust
- MAG
- RPWS
Publication and Content Type
- ref (subject category)
- art (subject category)
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Engelhardt, Ilka ...
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Wahlund, Jan -Er ...
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Andrews, David J ...
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Eriksson, Anders ...
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Ye, S.
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Kurth, W. S.
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Gurnett, D. A.
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Morooka, M. W.
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Farrell, W. M.
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Dougherty, M. K.
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Uppsala University