Microwave polarization inversion observed

Details Microwave polarization inversion observed Microwave polarization inversion observed

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991eostr..72..449b&link_type=abstract

EOS (ISSN 0096-3941), vol. 72, no. 42, Oct. 15, 1991, p. 449, 454.

Physics

3

Inversions, Microwave Emission, Polarization (Waves), Solar Activity Effects, Solar Corona, Solar Magnetic Field, Electron Density (Concentration), Photosphere

Scientific paper

Observations of an inversion of solar-active-region microwave polarization are described as they occurred during the Coronal Magnetic Structures Observing Campaign. Data regarding the microwave frequencies, soft X-ray emissions, brightness temperatures, and column emissions are obtained with the observations. The data are employed in the potential-field extrapolation procedure by Sakurai (1982) to calculate the coronal magnetic-field vector, and the microwave polarization observations yield reasonable coronal densities and evidence of an inversion.

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