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The quiet Sun brightness temperature at 127 MHz
Authors:Kazimierz M. Borkowski
Affiliation:(1) Toru"nacute" Radio Astronomy Observatory, Nicolaus Copernicus University, Toru"nacute", Poland
Abstract:A correction and analysis of routine total flux measurements made in Torunacute at 127 MHz allowed for the determination of the peak brightness temperature of the Sun (above 9 × 105 K) in three periods grouped around the last minimum, and for estimation of the brightness temperature of the coronal holes: (7.3 ± 1.4) × 105 K.
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