Journal article
The Dusty Plasma Disk Around the Janus/Epimetheus Ring
Journal of geophysical research. Space physics, Vol.123(6), pp.4668-4678
06/2018
DOI: 10.1002/2017JA024917
Abstract
We report on the electron, ion, and dust number densities and the electron temperatures obtained by the Radio and Plasma Wave Science instruments onboard Cassini during the Ring-Grazing orbits. The numerous ring passage observations show a consistent picture as follows: (1) Beyond 0.1 R-S above and below the equator the electron and ion densities are quasi-neutral with a distribution similar to the one obtained in the plasma disk. (2) A sharp ion density enhancement occurs at vertical bar Z vertical bar < 0.1 R-S, to more than 200 cm(-3) at the equator, while the electron density remains low only to values of 50cm(-3). The electron/ion density ratio is <= 0.1 at the equator. (3) Micrometer-sized dust has also been observed at the equator. However, the region of intense dust signals is significantly narrower (vertical bar Z vertical bar<0.02 R-S) than the enhanced ion density regions. (4) The electron temperature (T-e) generally decreases with decreasing Z with small T-e enhancements near the equator. We show that the dust size characteristics are different depending on the distance from the equator, and the large micrometer-sized grains are more perceptible in a narrow region near the equator where the power law slope of the dust size distribution becomes less steep. As a result, different scale heights are obtained for nanometer and micrometer grains. Throughout the ring, the dominant part of the negative charges is carried by the small nanometer-sized grains. The electron/ion density ratio is variable from orbit to orbit, suggesting changes in the dust charging over time scales of weeks.
Plain Language Summary The Radio and Plasma Wave Science instrument onboard Cassini observed a dusty plasma during the Ring-Grazing orbits. Dusty plasma is composed of, in addition to the electrons and ions, charged dust grains, and those grains play an important role in the plasma dynamics. The observed electron, ion, and dust number densities and the electron temperatures showed the layered structure of the faint Janus/Epimetheus rings. The core of the dusty ring composed of micron-sized dust is surrounded by a dusty plasma consisting of the ions and the negatively charged nanometer grains and further surrounded by the pristine plasma. The electron/ion density ratio of the dusty plasma varies from orbit to orbit, implying that the dust charging characteristics of the dusty ring change over time scales of weeks.
Details
- Title: Subtitle
- The Dusty Plasma Disk Around the Janus/Epimetheus Ring
- Creators
- M. W. Morooka - Swedish Institute of Space PhysicsJ. -E. Wahlund - Swedish Institute of Space PhysicsD. J. Andrews - Swedish Institute of Space PhysicsA. M. Persoon - University of IowaS. -Y. Ye - University of IowaW. S. Kurth - University of IowaD. A. Gurnett - University of IowaW. M. Farrell - Goddard Space Flight Center
- Resource Type
- Journal article
- Publication Details
- Journal of geophysical research. Space physics, Vol.123(6), pp.4668-4678
- Publisher
- Amer Geophysical Union
- DOI
- 10.1002/2017JA024917
- ISSN
- 2169-9380
- eISSN
- 2169-9402
- Number of pages
- 11
- Grant note
- Swedish National Space Board Dnr 174/15 / Swedish National Space Board NASA; National Aeronautics & Space Administration (NASA) 1415150 / NASA; National Aeronautics & Space Administration (NASA) Jet Propulsion Laboratory; National Aeronautics & Space Administration (NASA)
- Language
- English
- Date published
- 06/2018
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984455544802771
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