It is shown that the direct current dissipation is very unlikely to be the heat source of the coronal loop, because it accompanies unacceptably high heating rate in the chromospheric portion of the loop. This also suggests that a rather weak current density can supply the heat to a small (R < 107 cm
โฆ LIBER โฆ
Coronal heating by dissipation of magnetic structure
โ Scribed by Mitchell A Berger
- Publisher
- Springer Netherlands
- Year
- 1994
- Tongue
- English
- Weight
- 756 KB
- Volume
- 68
- Category
- Article
- ISSN
- 0038-6308
No coin nor oath required. For personal study only.
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