1969
DOI: 10.1007/bf00150670
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Some features of the solar microwave emission and their connection with geomagnetic activity

Abstract: A statistical investigation of the slowly varying component of the 9.1-cm solar radio emission is based upon the Stanford radioheliograms covering the years 1962-66. On the average the peak value of the brightness temperature Tb is proportional to the area covered by the corresponding spot group. However, in individual cases the observed Tb is definitely lower or higher than is to be expected from the size of the spot group. We introduce the concept 'microwave importance'/in of the spot group, which is the Tb … Show more

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