The time structure of solar radio emission variations at a wavelength of 3.3 MM

Details The time structure of solar radio emission variations at a wavelength of 3.3 MM The time structure of solar radio emission variations at a wavelength of 3.3 MM

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kfnt....6...36k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 6, July-Aug. 1990, p. 36-40. In Russian.

Computer Science

3

Millimeter Waves, Solar Radio Emission, Antennas, Computerized Simulation, Flocculating, Fourier Transformation, Radio Telescopes, Radiometers

Scientific paper

The fluctuations of the radio emission from parts of the solar disk at a wavelength of 3.3 mm are discussed. The contribution of atmospheric and instrumental interference is analyzed. The natural oscillation spectrum of the RT-22 radio telescope antenna contains a component in the 0.25-0.27 and 0.6-1.9 Hz frequency range. The existence of radio brightness oscillations with a repetition frequency of about 5 Hz is demonstrated.

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