Magnetic and microwave structure in solar active regions

Details Magnetic and microwave structure in solar active regions Magnetic and microwave structure in solar active regions

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...51...65f&link_type=abstract

Solar Physics, vol. 51, Jan.-Feb. 1977, p. 65-81.

Astronomy and Astrophysics

Astronomy

11

Magnetic Field Configurations, Microwave Emission, Photosphere, Solar Activity, Solar Magnetic Field, Solar Radio Emission, Magnetic Signatures, Radio Astronomy, Stellar Structure

Scientific paper

The structure of six active regions observed at 2.8 cm with the Stanford interferometer is compared with the configuration of the underlying photospheric magnetic fields, as given by the Kitt Peak magnetograph. The similar resolution and accuracy on the measured positions of both instruments allowed us to establish a more detailed spatial correspondence between radio and magnetic features than previously reached. The radio features which correspond to the cores of the active sources are always found to overlay regions of enhanced magnetic fields. Different spatial associations have been found depending on the brightness temperature of the sources. The possibility that this effect might be due to the development of the active region is also considered.

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