On flares, substorms, and the theory of impulsive flux transfer events
โ Scribed by A. Bratenahl; P. J. Baum
- Publisher
- Springer
- Year
- 1976
- Tongue
- English
- Weight
- 807 KB
- Volume
- 47
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
โฆ Synopsis
Solar flares and magnetospheric substorms are discussed in the context of a general theory of impulsive flux transfer events (IFTE). IFI'E theory, derived from laboratory observations in the Double Inverse Pinch Device (DIPD), provides a quantitative extension of "neutral sheet" theories to include nonsteady field line reconnection. Current flow along the reconnection line increases with magnetic flux storage. When flux build-up exceeds the level corresponding to a critical limit on the current, instabilities induce a sudden transition in the mode of conduction. The resulting IFTE, indifferent to the specific modes and instabilities involved, is the more energetic, the lower the initial resistivity. It is the more violent, the greater the resulting resistivity increase and the faster its growth. Violent events can develop very large voltage transients along the reconnection line. Persistent build-up promoting conditions produce relaxation oscillations in the quantity of flux and energy stored (bnild-up-IFTE cycles). It is dilficult to avoid the conclusion: flares and substorms are examples of IFrE.
๐ SIMILAR VOLUMES
It is shown that the stability analysis of coronae envisaged by does not lead to a unique stable configuration. The chromosphere-corona transition region is inevitably non-steady. Spicules are a manifestation of this. It is suggested that a point to point analysis of energy losses and gains, rather