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Millisecond structures in solar radio emission close to 264 MHz (1984)

Barrow, C. H. ; Flagg, R. S. ; Perrenoud, M.

Springer

Solar physics 90 (1984), S. 111-115

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ISSN: 1573-093X

Source: Springer Online Journal Archives 1860-2000

Topics: Physics

Notes: Abstract 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-1. They can occur individually or in small groups where they sometimes display a quasi-periodicity of a few milliseconds.

Type of Medium: Electronic Resource

URL: http://dx.doi.org/10.1007/BF00153788

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