Relationship between bKOM and nKOM radio emissions and structures in the solar wind during the Cassini gravity-assist flyby

Details Relationship between bKOM and nKOM radio emissions and structures in the solar wind during the Cassini gravity-assist flyby Relationship between bKOM and nKOM radio emissions and structures in the solar wind during the Cassini gravity-assist flyby

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja.....6650h&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #6650

Physics

Scientific paper

Jupiter is a very powerful source of radio waves. These radio waves range in frequencies from a few kHz to many tens of MHz, and show a great deal of variability. Previous studies have shown that part of this variability appears to be controlled by structures in the solar wind. One example of this influence is the relationship between the interplanetary magnetic field sector structure in the solar wind and the occurrence of broadband kilometric (bKOM) and narrowband kilometric (nKOM) radio emissions. Reiner et al. (GRL, 27, 297-300, 2000), using Ulysses data, found a relationship between the intensity and occurrence of the bKOM and nKOM emissions and the sector boundaries occurring in the solar wind. The Cassini gravity-assist flyby in December 2000 provides a new opportunity to examine this relationship.

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