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MacMeice Spicer
AIP Conference Proceedings Vol.267
Electromechanical Coupling of the Solar System

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).

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
ISBN: 978-1-56396-110-6

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