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Magnetic configuration of coronal streamers and threads

โœ Scribed by S. Koutchmy; V. A. Koutvitsky; M. M. Molodensky; L. S. Solov'iev; O. Koutchmy


Publisher
Springer Netherlands
Year
1994
Tongue
English
Weight
390 KB
Volume
70
Category
Article
ISSN
0038-6308

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The rotation of the solar electron corona is determined for intervals when nearly periodic variations dominated the polarization brightness record during 1964-1976. Coronal rotation rates derived for 765 intervals vary with height, latitude, and interval length. These rotation rates show a decrease