New microstructure of decametre solar radio bursts

Details New microstructure of decametre solar radio bursts New microstructure of decametre solar radio bursts

Jan 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.253..329s&link_type=abstract

Nature, vol. 253, Jan. 31, 1975, p. 329, 330. Research supported by the Department of Space of India.

Computer Science

1

Decametric Waves, Microstructure, Radio Spectra, Solar Radio Bursts, Spectrum Analysis, Circular Polarization, Faraday Effect, Fine Structure, High Resolution, Noise Storms, Polarization Characteristics, Radio Antennas, Solar Spectra, Type 3 Bursts, Very High Frequencies

Scientific paper

A new type of solar decameter bursts has been observed. These bursts are characterized by two components, the first a fast drift burst comprising patches of strong and weak emissions, the second a narrow band of intense emission. This phenomenon could be due to either the same stream of electrons, or to two or three successive electron streams. There is no association between these bursts and type III bursts. Explanations for the occurrences are given.

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