We present a spicule model whose eruption occurs as a result of the sudden pressure enhancement at the bright point located at the root of the spicule. To show this, one dimensional (constant cross sectional) and time dependent hydrodynamic equations are solved numerically in the realistic solar atm
โฆ LIBER โฆ
A 2D numerical study of explosive events in the solar atmosphere
โ Scribed by S.-P. Jin; B. Inhester; D. Innes
- Publisher
- Springer
- Year
- 1996
- Tongue
- English
- Weight
- 944 KB
- Volume
- 168
- Category
- Article
- ISSN
- 0038-0938
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