Abstract
A NEW series of observations of the galactic radio emission has been conducted at the frequencies of 20, 30 and 85 Mc/s. These low-resolution observations made with scaled aerials were intended to investigate the spectral index of the galactic radio emission in the frequency region 10–100 Mc/s.
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Turtle, A. J., Pugh, J. F., Kenderdine, S., and Pauliny-Toth, I. I. K., Mon. Not. Roy. Astro. Soc., 124, 297 (1962).
Ellis, G. R. A., Nature, 204, 171 (1964).
Shain, C. A., and Higgins, C. S., Austral. J. Phys., 7, 130 (1954).
Mills, B. Y., Publ. Astro. Soc. Pacific, 71, 267 (1959).
Turtle, A. J., Mon. Not. Roy. Astro. Soc., 126, 405 (1963).
Hartz, T. R., Nature, 203, 173 (1964).
Walsh, D., Haddock, F. T., and Schulte, D. H., Univ. Michigan, Radio-astronomy Report (June 1963).
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WIELEBINSKI, R., YATES, K. Spectrum of the Galactic Radio Emission. Nature 205, 581–582 (1965). https://doi.org/10.1038/205581a0
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DOI: https://doi.org/10.1038/205581a0
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