Abstract
Appleton1 and Hey2 have directed attention to the fact that radio-frequency energy, with some of the characteristics of random ‘noise’, is emitted with greatly increased intensity from the sun under the conditions of violent disturbance associated with a large sunspot. These observations were confined mainly to the region of frequencies near 60 Mc./s.
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References
Appleton, Nature, 156, 534, (1945).
Hey, Nature, 157, 47, (1946).
Pawsey, Payne-Scott, and McCready, Nature, 157, 158, (1946).
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RYLE, M., VONBERG, D. Solar Radiation on 175 Mc./s. Nature 158, 339–340 (1946). https://doi.org/10.1038/158339b0
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DOI: https://doi.org/10.1038/158339b0
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