Abstract
SINCE the early days of radio-astronomy, several solar eclipses have been studied in detail at various radio frequencies, the results being summarized in a review by Castelli and Aarons1.
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References
Castelli, J., and Aarons, J., Solar System Radio Astronomy (edit. by Aarons, J.), 49 (Plenum Press, 1965).
Bonvini, L. A., Croom, D. L., and Gordon-Smith, A. C., J. Atmos. Terr. Phys., 28, 891 (1966).
Allen, C. W., Radio Astronomy, I. A. U. Symp. No. 4 (edit. by Van De Hulst, H. C.), 253 (Cambridge University Press, 1957).
Castelli, J. P., and Straka, R. M., Sky and Telescope, 32, 84 (1966).
Piatelli, M., and Tofani, G., Osservazioni e Mem. dell'Osserv. Astrofis. di Arcetri, 85, 55 (1967).
Sinton, W. M., Physics and Astronomy of the Moon (edit. by Kopal, Z.) 421 (Academic Press, 1962).
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CROOM, D., POWELL, R. Solar Radiation at 19.0 Gc/s during the Eclipse of May 20, 1966. Nature 215, 260–261 (1967). https://doi.org/10.1038/215260a0
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DOI: https://doi.org/10.1038/215260a0
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