Both in solar regions of strong (100-1000 gauss) magnetic field (active regions) and in regions of weaker field (quiet regions), filaments of chromospheric material reside in and trace out sheared magnetic fields over magnetic inversion lines. Such filaments, and hence the sheared fields that they t
โฆ LIBER โฆ
Observed form and action of the magnetic energy release in flares
โ Scribed by Marcos E. Machado; Ronald L. Moore
- Book ID
- 107936274
- Publisher
- Elsevier Science
- Year
- 1986
- Tongue
- English
- Weight
- 900 KB
- Volume
- 6
- Category
- Article
- ISSN
- 0273-1177
No coin nor oath required. For personal study only.
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