Cassini Measurements of Satellite Influence on Jupiter's Radio Emission

Details Cassini Measurements of Satellite Influence on Jupiter's Radio Emission Cassini Measurements of Satellite Influence on Jupiter's Radio Emission

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agusm.p41b..02h&link_type=abstract

American Geophysical Union, Spring Meeting 2007, abstract #P41B-02

Physics

2732 Magnetosphere Interactions With Satellites And Rings, 2756 Planetary Magnetospheres (5443, 5737, 6033), 6939 Magnetospheric Physics (2700)

Scientific paper

Jupiter decameter wavelength emissions (DAM) have a known correlation with the orbital phases of the four Galilean satellites. In particular, the 2.0-5.6 MHz band of the DAM emission shows a small but significant enhancement in occurrence probability at specific orbital phases of the satellites. We performed a similar study using Cassini data that includes rotation period averaging and removal of the known satellite influences. We confirm the Galileo and Voyager studies in the 2.0-5.6 MHz band of the DAM emission and investigate the higher frequency bands 6-16 MHz. These analyses give further evidence for Alfvénic interactions between the satellites and Jupiter.

Affiliated with

Also associated with

No associations

Rating

Cassini Measurements of Satellite Influence on Jupiter's Radio Emission 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 Cassini Measurements of Satellite Influence on Jupiter's Radio Emission, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cassini Measurements of Satellite Influence on Jupiter's Radio Emission will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1035518