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The height of the 9 cm solar emission

โœ Scribed by M. Waldmeier


Publisher
Springer
Year
1978
Tongue
English
Weight
126 KB
Volume
57
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES


The height of 9.1 cm solar emission from
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Active regions that are sources of microwave solar emission should appear displaced in latitude relative to the associated optical feature and from this displacement it should be possible to deduce the height. Although the displacement is only about one-third of a rain of' arc at the most, it was fo

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The apparent height of radio sources above the photosphere was determined for the period of 1968-1971, by a method which makes use of the displacement in latitude of the centroid of the radio emission relative to the associated optical feature. The apparent height fell progressively in time by amou

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A possible connection between solar radio emission from 1.0 to 9.4 GHz and the interplanetary sector boundaries has been previously reported in the literature. The present research does not support the previous work as expected. The 9.1 cm activity appears to be organized around sector boundaries on