Structure and Dynamics of Small Magnetic Flux Concentrations: Observation versus Theory
Abstract
Observational results and theoretical model calculations for small magnetic flux concentrations in the solar photosphere are compared. The formation of flux concentrations and their magnetic, thermal and velocity structure are considered. Flux tube geometry, interaction with the environment and, finally, their destruction are discussed. In the conclusion, the necessity of further development and support of MHD model calculations in connection with new observational projects is emphasized.
- Publication:
-
The Role of Fine-Scale Magnetic Fields on the Structure of the Solar Atmosphere
- Pub Date:
- 1987
- Bibcode:
- 1987rfsm.conf..223S