Spectrum S-component flux and active region magnetic field

Details Spectrum S-component flux and active region magnetic field Spectrum S-component flux and active region magnetic field

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985prian..32....1s&link_type=abstract

Nagoya University, Research Institute of Atmospherics, Proceedings (ISSN 0077-264X), vol. 32, March 1985, p. 1-9.

Computer Science

Solar Activity, Solar Magnetic Field, Solar Spectra, Centimeter Waves, Magnetic Field Configurations, Magnetic Flux, Photosphere, Sunspots

Scientific paper

Characteristics are examined of an active region magnetic field structure whose spectral peak of an S-component source flux is of a higher frequency than that of a normal source. The flux ratio at 3 cm and 8 cm wavelengths (F3/F8) is used as an indicator of the peak frequency. The magnetic field structure of an active region with a high flux ratio is compared with the structure of that with a low flux ratio. It is shown that low-lying magnetic lines of force are characteristic of active regions with high flux ratio. The high-temperature and high-density plasma confined by low-lying magnetic lines of force intensifies the flux at short wavelengths, thus the flux peak shifts to a shorter wavelength.

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