Coronal Magnetic Field Measurements Through Quasi-Transverse Propagation

Details Coronal Magnetic Field Measurements Through Quasi-Transverse Propagation Coronal Magnetic Field Measurements Through Quasi-Transverse Propagation

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004assl..314..135r&link_type=abstract

Solar and Space Weather Radiophysics, Astrophysics and Space Science Library, Volume 314. ISBN 978-1-4020-2813-7. Springer Scien

Astronomy and Astrophysics

Astrophysics

1

Sun: Corona, Sun: Radio, Magnetic Field

Scientific paper

The QT-propagation of microwaves as a means to measure coronal magnetic fields and the inversion of circular polarization as an observational proof of the QT-propagation are discussed. The first part of the chapter briefly outlines the relevant geometry and mathematical relations. Then the state of the art in the coronal magnetography and some possibilities are demonstrated. We discuss use of the technique for coronal magnetography and give some estimates concerning the coronal magnetography with the forthcoming Frequency Agile Solar Radiotelescope.

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