Some properties of the narrow bandwidth millisecond pulsations in solar radio bursts at frequencies of 2.5 and 2.85 GHz

Details Some properties of the narrow bandwidth millisecond pulsations in solar radio bursts at frequencies of 2.5 and 2.85 GHz Some properties of the narrow bandwidth millisecond pulsations in solar radio bursts at frequencies of 2.5 and 2.85 GHz

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17..629y&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, July 1991, p. 629-636. In Russian.

Astronomy and Astrophysics

Astronomy

3

Solar Atmosphere, Solar Corona, Solar Radio Bursts, Sunspots, Narrowband, Radio Wave Refraction

Scientific paper

Results are presented of an investigation of the fine time structure of radio bursts based on solar observations at 2.5 and 2.85 GHz. It is shown that millisecond pulsations of burst intensity with 100-percent modulation have different time profiles at two adjacent frequencies without marked periodicity. It is assumed that pulsations arise due to refraction and dispersion of radio waves in the turbulent solar atmosphere.

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