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

✍ Scribed by Sh. B. Akhmedov; G. B. Gelfreikh; F. Fürstenberg; J. Hildebrandt; A. Krüger


Publisher
Springer
Year
1983
Tongue
English
Weight
309 KB
Volume
88
Category
Article
ISSN
0038-0938

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✦ Synopsis


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.