Abstract
This paper presents several magnetohydrostatic equilibrium models for
prominences with fibril-like fine structure. For all the models ad hoc
temperature profiles are used without discussing the energetics. For the
models fine structure is assumed to occur either across the prominence
axis or along it. This approach is intended as a first step toward more
realistic models based upon a series of vertical fibril structures.
Original language | English |
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Pages (from-to) | 331-351 |
Journal | Solar Physics |
Volume | 138 |
DOIs | |
Publication status | Published - 1 Apr 1992 |
Keywords
- Solar Corona
- Solar Prominences
- Solar Temperature
- Thermal Instability
- Boundary Conditions
- Solar Magnetic Field
- Temperature Profiles