Similarities and differences between magnetospheric substorms and solar flares
โ Scribed by K. Schindler
- Publisher
- Springer
- Year
- 1976
- Tongue
- English
- Weight
- 424 KB
- Volume
- 47
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
โฆ Synopsis
Magnetospheric substorms and solar flares seem to follow a pattern where a sudden transition from a slow passive evolution to a fast active evolution occurs. This concept which has proven useful for constructing a theory of the onset of magnetospheric substorms is tentatively applied to current sheets which may be relevant to flares.
๐ SIMILAR VOLUMES
It has been proposed that magnetospheric substorms and solar flares are a result of the same mechanism. In our view this mechanism is connected with the escape, or attempted escape, of energized plasma from a region of closed magnetic field lines bounded by a magnetic bottle. In the case of the Eart
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A superposed epoch analysis of [1964][1965][1966][1967][1968][1969][1970] solar flares shows a marked increase in flare occurrence within a day (13 ~ of longitude) of (-- ยง solar sector boundaries as well as a local minimum in flare occurrence near (+ --)sector boundaries. This preference for (--+)b