Abstract
IT has been suggested by Barrow1 that a rigorous comparison of solar, geomagnetic and Jupiter activity in radio emission cannot be made until continuous observation of Jupiter is possible throughout an apparition. The results summarized in this communication will, it is hoped, help to fill some gaps in the available figures for the 1962 apparition.
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References
Barrow, C. H., Astrophys. J., 135, 847 (1962).
Carr, T. D., Smith, A. G., Bollhagen, H., Six, F., and Chatterton, N. E., Astrophys. J., 134, 105 (1961).
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GLEDHILL, J., GRUBER, G. & BOSCH, M. Radio Observations of Jupiter during 1962. Nature 197, 474–475 (1963). https://doi.org/10.1038/197474b0
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DOI: https://doi.org/10.1038/197474b0
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