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CoMStOC: The Coronal Magnetic Structures Observing Campaign
Published online by Cambridge University Press: 19 July 2016
Abstract
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
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- Copyright © Kluwer 1990