Prediction of the ULYSSES Jovian hectometric observations

Details Prediction of the ULYSSES Jovian hectometric observations Prediction of the ULYSSES Jovian hectometric observations

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991jgr....9621207l&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 96, Dec. 1, 1991, p. 21,207-21,212.

Physics

8

Jupiter (Planet), Planetary Radiation, Plasma Waves, Radio Emission, Ulysses Mission, Circular Polarization, Radio Waves, Satellite Observation

Scientific paper

Based upon the HOM beaming and source model of Ladreiter and Leblanc (1990) several predictions can be made for the Ulysses unified radio and plasma wave experiment. During the inbound trajectory, Ulysses will, at first, be close to the Jovian equatorial plane when equal amounts of right-handed and left-handed circularly polarized HOM should be observed from the northern hemisphere and the southern hemisphere, respectively. At the closest approach, Ulysses will be very close to the LF HOM sources and will cross the HOM shadow zone, which extends out to about 20 Jovian radii close to the magnetic equatorial plane. During the outbound trajectory, the spacecraft will be at a fairly high southerly magnetic latitude and outside the main HOM emission beam, so that a relatively weak left-handed signal should be observed.

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