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CoMStOC: The Coronal Magnetic Structures Observing Campaign

Published online by Cambridge University Press:  19 July 2016

J.T. Schmelz
J.T. Schmelz*
Affiliation:
Applied Research Corp./Lockheed SMM-XRP Code 602.6 NASA/GSFC Greenbelt, MD 20715

Abstract

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The Coronal Magnetic Structures Observing Campaign (CoMStOC) was designed to measure the magnetic field strength and determine its structure in the solar corona. Simultaneous soft X-ray and microwave data separate the contributions of the two dominant microwave emission mechanisms - gyroresonance and thermal bremsstrahlung. Where gyroresonance dominates, the magnetic field can be determined.

Type
1. A Survey of Magnetic Phenomena near the Solar Photosphere, in the Corona, and in Stellar Winds
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 20
Copyright
Copyright © Kluwer 1990