Abstract
EARLY observations of the decametric radio emissions of Jupiter appeared to show that they had a narrow spectrum with a peak in the vicinity of 20 Mc./s. (refs. 1 and 2). As a result there were attempts to explain the radiation in terms of some appropriate single frequency mechanism such as plasma oscillations in a Jovian ionosphere2. More recently, however, with the passage of the solar activity maximum and consequent improving terrestrial observing conditions at low frequencies, the radiation has been detected at 10 Mc./s. (ref. 3). Here the results of observations at 4.8 Mc./s. will be reported.
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References
Gardner, F. F., and Shain, C. A., Austral. J. Phys., 11, 55 (1958).
Smith, A. G., and Carr, T. D., Astrophys. J., 130, 641 (1959).
Carr, T. D., Smith, A. G., Bolhagen, H., Six, N. F., and Chatterton, N. E., Astrophys. J., 134, 105 (1961).
Shain, C. A., Austral. J. Phys., 9, 61 (1956).
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ELLIS, G. Radiation from Jupiter at 4.8 Mc./s.. Nature 194, 667–668 (1962). https://doi.org/10.1038/194667a0
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DOI: https://doi.org/10.1038/194667a0
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