Angular sizes of stria-burst sources in the range 24-26 MHz

Details Angular sizes of stria-burst sources in the range 24-26 MHz Angular sizes of stria-burst sources in the range 24-26 MHz

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...57..229a&link_type=abstract

Solar Physics, vol. 57, Mar. 1978, p. 229-235.

Physics

2

High Frequencies, Solar Corona, Solar Spectra, Type 3 Bursts, Decametric Waves, Radio Scattering, Radio Telescopes

Scientific paper

The UTR-2 antenna has been used to measure angular sizes of sources of narrow-band short-lived solar stria-bursts at frequencies 24-26 MHz. The majority of these sources have apparent diameters between 20 and 40 ft. According to this parameter they do not differ noticeably from that of type III bursts at the same frequency. The short duration of the stria-bursts prevents explanation of the large diameter by scattering in the solar corona.

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