The radio approach of magnetic fine structures in solar atmosphere.

Details The radio approach of magnetic fine structures in solar atmosphere. The radio approach of magnetic fine structures in solar atmosphere.

Sep 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997pabei..15..198f&link_type=abstract

Prog. Astron., Vol. 15, No. 3, p. 198 - 217

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Solar Atmosphere: Radio Radiation, Solar Magnetic Fields: Structure, Solar Microwave Bursts

Scientific paper

The investigation on the magnetic field in the solar atmosphere is essential not only to solar atmosphere physics but also to solar activity. Radio observation in close connection with information obtained in other spectral ranges, e.g. the optical and X-ray regions is almost a unique method for the determination of the magnetic field in the corona and chromosphere outside the photosphere. On the basis of relevant emission mechanism and propagation processes in microwave and meter wavebands, basic radio methods for the deduction of the information on magnetic fields of background and source region are introduced. The radio dynamic spectra of fast fine structures in microwave bursts provide a significant means for the diagnosis of fine magnetic structures. It is also the major scientific object of "Solar Radio Broadband Spectrometer" which is being set up as a key project for the 23rd solar activity cycle.

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