Periodic Structure in Solar Radio Bursts and its Relation to Burst Energy

Details Periodic Structure in Solar Radio Bursts and its Relation to Burst Energy Periodic Structure in Solar Radio Bursts and its Relation to Burst Energy

Apr 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.222..158c&link_type=abstract

Nature, Volume 222, Issue 5189, pp. 158-159 (1969).

Computer Science

11

Scientific paper

DURING the period November 1967-October 1968, observations of solar radio emission were made at the Radio and Space Research Station, Slough, using a correlation type of polarimeter at a frequency of 2.8 GHz. The output corresponding to the left-hand component of polarization was recorded on paper chart at the comparatively fast speed of 60 cm h-1, giving resolution in time of about 2 s. It was found that many bursts which looked simple in form when recorded at 3 inches h-1 were resolved at the higher recording speed into complex structures, some of which were extremely impulsive.

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