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
Rotation and lifetime of coronal features
โ Scribed by Ester Antonucci; Maria Adele Dodero
- Publisher
- Springer
- Year
- 1979
- Tongue
- English
- Weight
- 296 KB
- Volume
- 62
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
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