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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References
Fürstenberg, F., Information Bull. Solar Radio Observatories, Utrecht (to be published).
Michel, H.-St., Information Bull. Solar Radio Observatories, Utrecht, No. 17 (December, 1964).
Priese, J., Monatsberichte D.A.W., Berlin (to be published).
Swarup, G., Kakinuma, T., Covington, E. A., Harvey, G. A., Mullaly, R. F., and Rome, J., Astrophys. J., 137, 1251 (1963).
Molchanow, A. P., Astron. J. (U.S.S.R.), 38, 849 (1961).
Tanaka, H., Proc. Res. Inst. Atm. Nagoya Univ., 11, 41 (1964).
Krüger, A., Krüger, W., and Wallis, G., Z. Astrophys., 59, 37 (1964).
Hirth, W., Beitr. Plasma Physik (to be published).
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KRÜGER, A., MICHEL, HS. A New Feature of the Spectrum of the s-Component of Solar Radio Emission. Nature 206, 601–602 (1965). https://doi.org/10.1038/206601a0
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DOI: https://doi.org/10.1038/206601a0
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