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SIMURIS: High-Resolution Solar Physics

Published online by Cambridge University Press:  12 April 2016

Robert J. Rutten  and
Luc Damé
Robert J. Rutten
Affiliation:
Sterrekundig Instituut, Postbus 80 000, NL-3508 TA Utrecht, TheNetherlands
Luc Damé
Affiliation:
Service d’Aeronomie CNRS, BP N° 3, F-91371 Verrières-le-Buisson Cedex, France

Abstract

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The magnetic fields of the Sun provide the major incentive to do solar physics. The small spatial extent of the magnetically constrained structures and processes in the solar atmosphere provide the major incentive for high resolution solar telescopes. The visibility of the outer solar atmosphere in the ultraviolet and X-ray domains provide the major incentive for solar space telescopes. Cost provides the major incentive to use interferometric techniques. SIMURIS employs short-wave interferometry from space to measure solar structures and processes with high resolution.

Type
Session 3. Techniques of Magnetic Field Measurements
Information
International Astronomical Union Colloquium , Volume 141: The Magnetic and Velocity Fields of Solar Active Regions , 1993 , pp. 184 - 187
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

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