Microwave radar observations of the sun

Details Microwave radar observations of the sun Microwave radar observations of the sun

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....76..354b&link_type=abstract

Astronomy and Astrophysics, vol. 76, no. 3, July 1979, p. 354, 355.

Astronomy and Astrophysics

Astrophysics

7

Electrostatic Probes, Plasma Waves, Radar Measurement, Solar Radio Bursts, Solar Wind, Microwave Equipment, Plasma Frequencies, Power Spectra, Raman Spectra, Solar Corona, Telescopes

Scientific paper

A pilot experiment on microwave radar observations of the sun has been conducted with the Arecibo 300-m telescope. Data obtained at 2600 MHz with a bandwidth of 100 MHz are presented. This frequency is shifted from the transmitted frequency by the expected Langmuir waves in the range from 170 to 270 MHz. The results show the absence of such waves in the corona with energy densities above about 0.0006, 0.08, and 0.02 nKT for a possible type I radio source region, a prominence, and streamer, respectively.

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