Other
Scientific paper
Mar 1953
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1953natur.171..445t&link_type=abstract
Nature, Volume 171, Issue 4349, pp. 445 (1953).
Other
Scientific paper
IT has been reported previously that the daily values of intensity of solar radio emission are approximately proportional to the whole disk Wolf's sunspot relative number or sun spot area1,2. On the other hand, there is a tendency for the intense radiation to be observed when active sunspots are near the central meridian, especially in the metre wavelength region. If the solar radio emission has such a tendency, the daily values of solar radio emission will show better correlation with the sunspot relative number, nA1 + A2, than the whole disk sunspot relative number, A1 + A2, where A1, A2 indicate Wolf's relative sunspot number in the central-circle zone (half-diameter circle) and in the outer zone respectively, and n is a parameter which indicates the importance of the sunspots located in the central-circle zone compared with those in the outer zone. To investigate the directivity of solar radio emission from the sunspots quantitatively, the value of n to give a maximum correlation coefficient was determined.
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