Duration and Band-width of Short-lived Transients in Solar Noise

Details Duration and Band-width of Short-lived Transients in Solar Noise Duration and Band-width of Short-lived Transients in Solar Noise

Jun 1958

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1958natur.181.1676d&link_type=abstract

Nature, Volume 181, Issue 4624, pp. 1676-1677 (1958).

Physics

1

Scientific paper

THE duration of small bursts in solar radio noise at 400 Mc./s. has been stated1 recently to be 0.18 +/- 0.03 sec. This value was a maximum in a histogram. On days with an intense small-scale activity, the material obtained is so abundant that reliable histograms can be obtained for periods as short as two hours. Fig. 1 shows an example of such a set. The shift of the maximum and of the entire curve is undoubtedly significant in most cases, and it should be possible to correlate it with a similar shift in the circumstances in which the bursts originate.

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