Radio Diagnostics of Magnetic Fields in the Solar Corona

Details Radio Diagnostics of Magnetic Fields in the Solar Corona Radio Diagnostics of Magnetic Fields in the Solar Corona

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...3e..93b&link_type=abstract

Solar Active Regions and 3D Magnetic Structure, 26th meeting of the IAU, Joint Discussion 3, 16-17 August, 2006, Prague, Czech R

Physics

Scientific paper

Measurement of the coronal magnetic field has been an elusive goal for many years. In recent years, however, progress has been made in developing techniques at radio and IR wavelengths to measure or constrain the magnetic field in the quiet and active corona. In this talk, radio diagnostic techniques are reviewed in a variety of contexts, including the quiet corona, active regions, flares, and coronal mass ejections. Techniques that exploit emission intrinsic to the phenomena themselves - e.g., gyrosynchrotron radiation - and those which exploit external probes such as spacecraft beacons or extragalactic background sources are both discussed. Prospects for exploiting these techniques with future generations of radio instrumentation are also considered.

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