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A Study of the Rotation of the Solar Corona

✍ Scribed by Richard C. Altrock

Book ID
110432725
Publisher
Springer
Year
2003
Tongue
English
Weight
349 KB
Volume
213
Category
Article
ISSN
0038-0938

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πŸ“œ SIMILAR VOLUMES

Rigid and differential rotation of the s
Rigid and differential rotation of the solar corona
✍ Ester Antonucci; Leif Svalgaard πŸ“‚ Article πŸ“… 1974 πŸ› Springer 🌐 English βš– 423 KB

The rotation of the solar corona has been studied using recurrence properties of the green coronal line (5303 A,) for the interval 1947-1970. Short-lived coronal activity is found to show the same differential rotation as short-lived photospheric magnetic field features. Long-lived recurrences show

Solar rotation in the chromosphere and c
Solar rotation in the chromosphere and corona
✍ William Henze; A. K. Dupree πŸ“‚ Article πŸ“… 1973 πŸ› Springer 🌐 English βš– 275 KB

Extreme ultraviolet spectroheliograms in Mg x (625 ~) and the Lyman continuum (897/~) obtained from OSO-6 are used to determine the differential rotation rate in the solar chromosphere and corona. The equatorial rotation rate agrees with spectroscopic measurements of the photospheric plasma velocity

Two types of differential rotation of th
Two types of differential rotation of the solar corona
✍ Olga G. Badalyan πŸ“‚ Article πŸ“… 2010 πŸ› Elsevier Science 🌐 English βš– 948 KB

The differential rotation of the solar corona has been analyzed using as the input data the brightness of the coronal green line Fe XIV 530.3 nm for more than five activity cycles. It is found that the character of rotation of the solar corona changes during the activity cycle. Approximately at the

Photometric Study of the Solar Corona
Photometric Study of the Solar Corona
✍ KOUTCHMY, S.; LAFFINEUR, M. πŸ“‚ Article πŸ“… 1970 πŸ› Nature Publishing Group 🌐 English βš– 273 KB