Excitation and Propagation of Jovian Quasi-Periodic Radio Bursts

Details Excitation and Propagation of Jovian Quasi-Periodic Radio Bursts Excitation and Propagation of Jovian Quasi-Periodic Radio Bursts

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..638k&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.638

Computer Science

Scientific paper

We discussed the source location, directivity, and propagation process of QP bursts based on the ray tracing analysis, comparing with the observation results, especially with the latitudinal beaming and shadow zone [Kimura et al., 2010]. The parametric survey indicated that QP bursts observed at high and low latitudes have the source region at 2-10 Rj altitude along high-latitudinal field lines (L>20). It was suggested that these QP bursts have significantly broadened beaming patterns like a "filled cone".

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