๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Photospheric Magnetic Fields on March 7, 1970

โœ Scribed by LIVINGSTON, W.; HARVEY, J.; SLAUGHTER, C.


Book ID
109672092
Publisher
Nature Publishing Group
Year
1970
Tongue
English
Weight
636 KB
Volume
226
Category
Article
ISSN
0028-0836

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๐Ÿ“œ SIMILAR VOLUMES


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The common observation that where photospheric magnetic fields are strong, the overlying corona is bright is examined quantitatively. White light coronal brightness is employed because it is independent of coronal temperature and is directly related to coronal electron density. Brightness data for t

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We consider proposed mechanisms for the formation of coronal holes, and identify as crucial the issue whether the holes are permeated by rigidly rotating fields. It is suggested that the interaction between such a field and the differentially rotating, diffusive solar envelope will produce a fore af