Calculation of Type III Radio Emission from a Particle Transport Model

Details Calculation of Type III Radio Emission from a Particle Transport Model Calculation of Type III Radio Emission from a Particle Transport Model

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3491e&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

type I I I radio bursts are produced when beams of electrons (2 to 50 keV) originating at the Sun generate radio emission at the local plasma frequency as they move out through the heliosphere. As the beams encounter successively lower and lower plasma density the emission frequency becomes lower. If the electrons actually reach the observer, the frequency can be as low as the local plasma frequency. Recent work concludes that there is an intimate connection between the propagation of electrons and protons, and among electrons of vastly different energies. As a result we have begun an effort to incorporate calculations of radio emission into our comprehensive propagation model. I report on the first results of this calculation.

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