Bremsstrahlung and Synchrotron Radiation from Planet Magnetospheres

Details Bremsstrahlung and Synchrotron Radiation from Planet Magnetospheres Bremsstrahlung and Synchrotron Radiation from Planet Magnetospheres

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..812..389k&link_type=abstract

PLASMA 2005: Int. Conf. on Research and Applications of Plasmas; 3rd German-Polish Conf.on Plasma Diagnostics for Fusion and App

Statistics

Applications

Electromagnetic Wave Propagation, Mhd Waves, Plasma Waves, And Instabilities, Magnetospheric Modeling And Forecasting

Scientific paper

Bremsstrahlung and synchrotron radiation from the moving charged particles was calculated in planet magnetospheres. A program package RADIATION was developed for these calculations. The radiative intensity is projected on a far sphere. The directional dependence of the radiation during the penetration of charged particles through the polar cusp was calculated. The program package RADIATION can be also used for treating the radiation of plasma cluster penetrating through the electric double layer, MHD and compress magnetic bow shock, plasma fibers and pinches and in other important situations. Intensity of radiation was derived from advanced and retarded potentials calculated from the Maxwell set of equations. Only radiative fields are displayed (I ~ 1/r2) and the space intensity distribution does not depend on the distance of the projection sphere. In future non-radiative fields will be treated as well. In this case the distance of the projection sphere will be important parameter. The program was written in FORTRAN CVF 6.5A. The Earth magnetosphere and ionosphere form a natural protective shield from cosmic radiation and solar wind. Various models of the magnetosphere are compared (Tsyganenko, Safrankova-Nemecek, IGRF, and others) in the end of the contribution.

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