The Interaction of Saturn's Magnetosphere with the Icy Satellites: A Plasma Wave Perspective

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

5737 Magnetospheres (2756), 5780 Tori And Exospheres, 6280 Saturnian Satellites

Scientific paper

The early portion of the Cassini orbital tour at Saturn has provided a first reconnaissance of the interactions of the icy moons Enceladus, Tethys, Dione, Rhea, and Hyperion with the magnetosphere. While this reconnaissance consists of, for most of these moons, a single flyby which is not necessarily optimized for the study of the magnetospheric interaction, there are plasma wave phenomena observed near most of these moons which provide some insight into the interactions. Given the volatile nature of the icy crusts of these moons, all were considered possible sources of plasma for the magnetosphere prior to Cassini's arrival at Saturn. Detection of the upper hybrid band during the satellite flybys provides an accurate measurement of the electron plasma density along Cassini's trajectory. Contrary to the situation near the Galilean satellites, Saturn's icy satellites do not appear as sources of `fresh' electrons, strongly suggesting that the plasma originating at these bodies is the result of charge exchange. This is perhaps most clear from the closest approach to Enceladus where only a general increase in the total plasma density was found in the near- equatorial plasma sheet and not a localized spike in density in the near vicinity of the moon. This conclusion is consistent with the observation of enhanced electromagnetic fluxes of ion cyclotron waves near the orbits of Enceladus and Tethys observed with the Cassini magnetometer. In addition to the above waves, another common class of wave mode present near the encounters are in the whistler mode frequency range and could be present due to anisotropic electron distributions related to the presence of the moon. The radio and plasma wave science instrument is also sensitive to impacts of micron-sized dust; these are particularly evident in the close flyby of Enceladus on 14 July 2005.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The Interaction of Saturn's Magnetosphere with the Icy Satellites: A Plasma Wave Perspective does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Interaction of Saturn's Magnetosphere with the Icy Satellites: A Plasma Wave Perspective, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Interaction of Saturn's Magnetosphere with the Icy Satellites: A Plasma Wave Perspective will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-962646

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.