Kinematic model of loop prominences formation.
Abstract
The kinematics of the material motion in a variable magnetic field in the MHD approximation of a strong field and cold plasma is investigated. The variation of magnetic moments of two dipole systems leads to the development of such phenomena as loop prominences, coronal rain and funnel prominences.
- Publication:
-
Solar Physics
- Pub Date:
- September 1977
- DOI:
- 10.1007/BF00146422
- Bibcode:
- 1977SoPh...54...35I
- Keywords:
-
- Solar Magnetic Field;
- Solar Prominences;
- Stellar Models;
- Cold Plasmas;
- Magnetic Moments;
- Solar Corona;
- Solar Physics;
- Magnetic Field;
- Kinematic Model;
- Strong Field;
- Cold Plasma;
- Variable Magnetic Field;
- Solar Prominences:Loops;
- Solar Prominences: Models