Refraction of Jovian decametric radio emission. I - Distortion of the S-component radiation pattern

Details Refraction of Jovian decametric radio emission. I - Distortion of the S-component radiation pattern Refraction of Jovian decametric radio emission. I - Distortion of the S-component radiation pattern

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kfnt....5...68a&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 5, Sept.-Oct. 1989, p. 68-74. In Russian.

Computer Science

Decametric Waves, Jupiter Atmosphere, Planetary Magnetospheres, Radiation Distribution, Radio Emission, Refracted Waves, Io, Planetary Ionospheres, Plasma Radiation

Scientific paper

A computer program has been developed for calculating the refraction of
a fast extraordinary mode in the inner magnetosphere of Jupiter. The
calculations show that, if the realistic plasma model is used, the
refraction may explain the observed geometric S-radiation pattern and
its variations with Io longitude and frequency.

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