Solar corona observations at decameter wavelengths

Details Solar corona observations at decameter wavelengths Solar corona observations at decameter wavelengths

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011yera.confe..22k&link_type=abstract

The 41st Young European Radio Astronomers Conference, held at University of Manchester/Jodrell Bank Observatory, 18-20 July 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

The antenna system UTR-2 (Ukrainian T-shaped radio telescope, Mark 2) of the Braude Radio Observatory (Kharkov, Ukraine) has been used to observe the radio emission from the quiet Sun in the frequency range 16.5-33 MHz. The monitoring of solar corona has been carried out during the summer-autumn of 2010. The investigations included the measurement of solar flux density and the determination of angular equatorial and polar diameters of solar corona from day to day. Moreover the heliograph capability of UTR-2 was applied too. Preliminary results are presented.

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