Changes in the solar magnetic field preceding a coronal mass ejection
โ Scribed by L.K Harra
- Publisher
- Elsevier Science
- Year
- 2002
- Tongue
- English
- Weight
- 128 KB
- Volume
- 64
- Category
- Article
- ISSN
- 1364-6826
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๐ SIMILAR VOLUMES
Coronal mass ejection transients observed with the white light coronagraph on Skylab are found to be associated with several other forms of solar activity. There is a strong correlation between such mass ejection transients and chromospheric Ha activity, with three-quarters of the transients apparen
It is shown that the simultaneous consideration of observed values of the solar wind proton flux density at 1 AU and of the electron pressure at the base of the solar corona leads to relatively strong constraints on the coronal temperature in the region of subsonic solar wind flow. The extreme upper