On the height scale of magnetic fields above sunspots derived from RATAN-600 observations

Details On the height scale of magnetic fields above sunspots derived from RATAN-600 observations On the height scale of magnetic fields above sunspots derived from RATAN-600 observations

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...88..103a&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 88, Oct. 1983, p. 103-108.

Physics

9

Height, Microwave Emission, Radio Observation, Solar Magnetic Field, Sunspots, Electron Density Profiles, Mathematical Models, Polarization Characteristics, Radiant Flux Density, Radio Telescopes, Solar Physics, Temperature Distribution

Scientific paper

Model calculations of the S-component are compared with observations of the RATAN-600 telescope at five discrete microwave frequencies referring to active region McMath No. 15974 on May 1, 1979. The spectral variations of source diameter, flux density, and degree of polarization are used to derive the height scale of the magnetic field in accordance with a magnetic dipole distribution under the assumption of advanced temperature and electron density distributions according to most recent EUV observations.

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