A model support to analysis of high resolution radio observations of the sun

Details A model support to analysis of high resolution radio observations of the sun A model support to analysis of high resolution radio observations of the sun

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992balta...1..239r&link_type=abstract

Baltic Astronomy, vol. 1, p. 239

Physics

3

Solar Radio Emission, Radio Observation, Coronal Holes, Computerized Simulation, Solar Atmosphere, Solar Magnetic Field, Solar Physics, High Resolution, Stellar Models

Scientific paper

It is important to accompany radio observations of the sun by model simulations because of the variety of physical and geometrical conditions forming the radio image. Computer models of cm and dm radiation of the local source, the coronal hole, and the quiet solar atmosphere are presented. The model support for the analysis of radio observations of the sun with the telescope RATAN-600 is exemplified.

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