๐”– Bobbio Scriptorium
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X-ray bright points, coronal heating and the solar cycle

โœ Scribed by M. H. Gokhale


Publisher
Springer
Year
1975
Tongue
English
Weight
362 KB
Volume
41
Category
Article
ISSN
0038-0938

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โœฆ Synopsis


Recent Skylab observations about the bright points in the solar X-ray images seem to confirm an essential prediction of a model proposed by this author for the appearance and the disappearance of the photospheric fields during a solar cycle.

The segments of the individually rising strands of the 'fundamental flux-loops' proposed in the model may lead to the X-ray bright points with the observed properties.

The emergence of such strands may substantially contribute to the coronal heating at different heights.


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