Abstract
IN the present minimum of solar activity, investigations of the spectrum of the quiet Sun in the cm- and dm-regions as well as the spectrum of single centres of the slowly varying component (s-component) of solar radio emission are of particular interest. Absolute calibrations of radio telescopes carried out at the Heinrich Hertz Institute, Berlin-Adlershof (HHI), led during recent years to spectra of the quiet Sun flux density and of the s-component which are somewhat different from earlier assumed spectra.
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