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New Observational Aspects

Published online by Cambridge University Press:  08 February 2017

Oddbj⊘rn Engvold
Oddbj⊘rn Engvold*
Affiliation:
Institute of Theoretical Astrophysics University of Oslo P.O.Box 1029, Blindern N-0315 Oslo 3, Norway

Abstract

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The requirements and conditions for high resolution imaging and polarimetry of the Sun are reviewed. Various methods and techniques are discussed for image stabilization and sharpening in solar observations. The new solar facilities in the Canary Islands in particular are frequently reaching diffraction limited resolution and yield new insight in the structure and dynamics of the solar atmosphere. Future ground based telescopes like THEMIS and LEST, as well as planned solar missions in space will trigger a next advance in solar physics.

Type
VIII. Future Directions
Information
Symposium - International Astronomical Union , Volume 138: Solar Photosphere: Structure, Convection and Magnetic Fields , 1990 , pp. 469 - 487
Copyright
Copyright © Kluwer 1990 

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