Radio emission from the sun at 843 MHz. I - Instrumentation

Details Radio emission from the sun at 843 MHz. I - Instrumentation Radio emission from the sun at 843 MHz. I - Instrumentation

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..125..359g&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 125, Feb. 1990, p. 359-369.

Physics

2

Centimeter Waves, Microwave Emission, Solar Radio Emission, Multibeam Antennas, Radio Telescopes, Solar Observatories, Synthetic Arrays

Scientific paper

The Molonglo Observatory Synthesis Telescope (MOST) has recently been modified to permit observations of the sun. With a collecting area of 18,000 sq m, MOST makes high-sensitivity measurements in right-hand circular polarization over a 3 MHz bandwidth at 843 MHz. This paper decribes the instrument and the procedures used to make various types of solar observations, and exhibits some of the first data collected.

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