Growth Rate Analysis of Ordinary Mode Saturn Kilometric Radiation

Details Growth Rate Analysis of Ordinary Mode Saturn Kilometric Radiation Growth Rate Analysis of Ordinary Mode Saturn Kilometric Radiation

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufm.p33b1284m&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #P33B-1284

Physics

[2772] Magnetospheric Physics / Plasma Waves And Instabilities, [5719] Planetary Sciences: Fluid Planets / Interactions With Particles And Fields, [5737] Planetary Sciences: Fluid Planets / Magnetospheres

Scientific paper

On October 17, 2008, the Cassini spacecraft encountered a source region of Saturn kilometric radiation (SKR) allowing in situ measurements of wave intensity and polarization, as well as the electron phase space density. The dominant emission is right-hand extraordinary (R-X) mode, but in addition, there is clear evidence of weaker left-hand ordinary (L-O) mode mission. The L-O mode occurs in narrow-banded frequency ranges for frequencies greater than the local cyclotron frequency. In this study we concentrate on the L-O mode emission, seeking to account for the observed frequency ranges and intensity relative to the R-X mode.

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