It is now known that the corona is filled with a multitude of loop-like structures. The likelihood of these loops being in static equilibrium is small and so this paper explores the possibility of steady isothermal or adiabatic flows, driven by a pressure difference between the loop feet. For a symm
โฆ LIBER โฆ
Stability of siphon flow in coronal magnetic loops
โ Scribed by Fu Xu; Sheng Rong
- Publisher
- Elsevier Science
- Year
- 1986
- Tongue
- English
- Weight
- 341 KB
- Volume
- 10
- Category
- Article
- ISSN
- 0275-1062
No coin nor oath required. For personal study only.
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We present here a model, based on observations, for the magnetic-field equilibrium of a cool coronal loop. The pressure structure, taken from the Harvard/Skylab EUV data, is used to modify the usual force-free-field form in quasi-cylindrical symmetry. The resulting field, which has the same directio