Measurement of coronal fields using spatially resolved microwave spectroscopy

Details Measurement of coronal fields using spatially resolved microwave spectroscopy Measurement of coronal fields using spatially resolved microwave spectroscopy

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2442..319h&link_type=abstract

In NASA. Goddard Space Flight Center Coronal and Prominence Plasmas p 319-323 (SEE N87-20871 13-92)

Astronomy and Astrophysics

Astronomy

5

Brightness Temperature, Coronal Loops, Field Strength, Microwave Emission, Microwave Spectra, Solar Magnetic Field, Astronomical Spectroscopy, High Resolution, Spatial Resolution, Spectral Resolution, Sunspots

Scientific paper

The authors consider the potential implications of observations which combine both high spatial and high spectral resolution. In particular, they are interested in the ability to measure the magnetic field at the base of the corona on a point by point basis, as in a true magnetograph. They present model calculations of the microwave brightness temperature spectrum along specific lines of sight near a sunspot. They believe that spatially resolved microwave spectroscopy provides a promising new coronal diagnostic. At present, however, a key limitation in its application is the lack of sufficient number of antennas with which to map complex active regions.

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