Observations of the Solar Continuum Radio Emission at Decameter Wavelengths

Details Observations of the Solar Continuum Radio Emission at Decameter Wavelengths Observations of the Solar Continuum Radio Emission at Decameter Wavelengths

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1206..440b&link_type=abstract

ASTROPHYSICS AND COSMOLOGY AFTER GAMOW: Proceedings of the 4th Gamow International Conference on Astrophysics and Cosmology Afte

Physics

High Energy Physics

Solar Radio Emission, Solar Corona, Radio Telescopes, Solar Electromagnetic Emission, Corona, Radio Telescopes And Instrumentation, Heterodyne Receivers

Scientific paper

Results of study of the continuum radio emission of the Sun in the decameter range are presented. Observations were carried out with radio telescope URAN-2 in summer months in 2008-2009. Radio fluxes at frequencies 20 MHz and 25 MHz in frequency band 250 kHz were obtained during the time, when there were no active regions on the solar disk. Their average values for two years were 670 Jy and 850 Jy at frequencies 20 MHz and 25 MHz correspondingly. These fluxes are in agreement with high frequency values.

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