Long-term variations in the rotation of the solar corona
β Scribed by A. G. Tlatov
- Book ID
- 110216260
- Publisher
- Springer
- Year
- 2006
- Tongue
- English
- Weight
- 582 KB
- Volume
- 50
- Category
- Article
- ISSN
- 1063-7729
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π SIMILAR VOLUMES
Long-lived brightness structures in the solar electron corona persist over many solar rotation periods and permit an observational determination of coronal magnetic tracer rotation as a ftmction of latitude and height in the solar atmosphere. For observations over 1964-1976 spanning solar cycle 20,
A model is presented which shows that large numbers of energetic electrons (0.3-> 10 MeV) and protons (1-30 MeV) can be stored in the solar corona at altitudes around 3 β’ 105 km for periods in excess of 5 days. Specific reference is made to the time period July 6-16 1968 as an excellent example of e