Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-30T02:29:59.000Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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