Source location determination of Uranian kilometric radiation from ray tracing and emission lobe modelling

Details Source location determination of Uranian kilometric radiation from ray tracing and emission lobe modelling Source location determination of Uranian kilometric radiation from ray tracing and emission lobe modelling

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991sri..reptq....m&link_type=abstract

Final Report Southwest Research Inst., San Antonio, TX. Instrumentation and Space Research Div.

Astronomy and Astrophysics

Astronomy

Kilometric Waves, Planetary Radiation, Radio Emission, Ray Tracing, Spaceborne Astronomy, Uranus (Planet), Magnetic Fields, Radio Astronomy, Three Dimensional Models, Ultraviolet Radiation

Scientific paper

We use an analytical fit to an emission lobe profile together with three-dimensional ray tracing to model the broad-banded smooth Uranian kilometric radiation (UKR). We assume the radiation is gyroemission from sources along magnetic field lines. Using an iterative technique that modifies the lobe function and source region, the results are compared to observations at a frequency of 481 kHz. The best-fit calculations are compared to previously published models and to recent ultraviolet (UV) observations.

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