Observations of the Fine Structure of Enhanced Solar Radio Radiation with a Narrow-Band Spectrum Analyser

Details Observations of the Fine Structure of Enhanced Solar Radio Radiation with a Narrow-Band Spectrum Analyser Observations of the Fine Structure of Enhanced Solar Radio Radiation with a Narrow-Band Spectrum Analyser

Sep 1959

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1959natur.184..887e&link_type=abstract

Nature, Volume 184, Issue 4690, pp. 887-888 (1959).

Computer Science

17

Scientific paper

THE different components of the solar radio emission at metre wave-lengths were classified according to their spectral properties by Wild and McCready1 in 1950. In this classification the noise storm or type 1 radiation is characterized by a relatively steady enhancement over a wide range of frequencies, usually with short-lived, narrow-band bursts superposed (storm bursts, type 1 bursts). With equipment of high resolving power these bursts may be resolved into pips, each lasting for a fraction of a second only.

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