A Low-Frequency (30 - 110 MHz) Antenna System for Observations of Polarized Radio Emission from the Solar Corona

Physics

Scientific paper

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Magnetic Fields, Solar Corona, Radio Observations, Polarization

Scientific paper

An interferometer antenna system to observe polarized radio emission from the solar corona at different frequencies in the range 30 - 110 MHz has been commissioned recently by the Indian Institute of Astrophysics at the Gauribidanur Radio Observatory (latitude 13°36'12''N and longitude 77°27'07''E), about 100 km north of Bangalore ( http://www.iiap.res.in/centres_radio.htm ). This paper describes the antenna system, associated analog/digital receiver setup, calibration scheme, and preliminary results.

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