Two types of differential rotation of the solar corona
The differential rotation of the solar corona has been analyzed using as the input data the brightness of the coronal green line Fe xiv 530.3nm 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 m...
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Veröffentlicht in: | New astronomy 2010-01, Vol.15 (1), p.135-143 |
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Format: | Artikel |
Sprache: | eng |
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