Proceedings of the Conference Held in Capri, Italy, May 1991
The principal objective of the third OSL workshop was an in-depth assessment of our present theoretical and experimental understanding of how radiation, velocity, and magnetic fields, together with thermodynamic variables, behave as a fully coupled system. A key topic of discussion was the role of magnetic fields in the electromechanical coupling of different parts of the solar atmosphere.
Partial Contents
- Magnetic Flux Tubes as Communication Channels (B. Roberts).
- Magnetic Field Line Topology in Solar Active Regions (N. Seehafer).
- Explosive Events and Magnetic Reconnection in the Solar Atmosphere (K.P. Dere).
- Three-Dimensional Kinematic Reconnection of Plasmoids with Nulls (Y.-T. Lan and J.M. Finn).
- The X-ray Ultraviolet Imager for the Orbiting Solar Laboratory (E. Antonucci et al.).
- On Non-local Transport Processes in the Solar Atmosphere (P.MacNeice).
Readership:
Solar physicists and those involved in dynamo theory, chaos theory, MHD turbulence, and wave propagation theory.
Springer Verlag / American Institute of Physics, 1992, 170 S.
117,65 Euro
Hardcover
ISBN: 978-1-56396-110-6
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