Millisecond structures in solar radio emission close to 264 MHz

Details Millisecond structures in solar radio emission close to 264 MHz Millisecond structures in solar radio emission close to 264 MHz

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...90..111b&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 90, Jan. 1984, p. 111-115.

Physics

5

Microwave Spectra, Solar Radio Bursts, Solar Spectra, Fine Structure, Frequency Shift, Pulse Duration, Temporal Resolution, Type 3 Bursts

Scientific paper

High-time resolution spectral measurements of solar radio emission close to 264 MHz are reported. Instrumental resolutions of the order of a few kHz in frequency and tenths of milliseconds in time were used to resolve the burst fine structure in the time-frequency plane. Fine structures, having narrow bandwidths and durations of some 5 to 30 ms, have been observed mostly in association with type I and type III bursts. These very short duration bursts have negative frequency drifts of about -50 to -60 MHz/s. They can occur individually or in small groups where they sometimes display a quasi-periodicity of a few milliseconds.

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