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    Source location determination of Uranian kilometric radiation from ray tracing and emission lobe modelling (1991)
    In:  CASI
    Details
    Publication Date: 2019-06-28
    Description: 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.
    Keywords: SPACE RADIATION
    Type: NASA-CR-190482 , JPL-9950-1369 , NAS 1.26:190482
    Format: application/pdf
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