𝔖 Bobbio Scriptorium
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On Rotation of the Solar Corona

✍ Scribed by Lorenc, M.; Rybanský, M.; Dorotovič, I.

Book ID
118810533
Publisher
Springer
Year
2012
Tongue
English
Weight
442 KB
Volume
281
Category
Article
ISSN
0038-0938

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📜 SIMILAR VOLUMES

Solar rotation in the chromosphere and c
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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

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✍ Olga G. Badalyan 📂 Article 📅 2010 🏛 Elsevier Science 🌐 English ⚖ 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