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.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Appleton, Nature, 156, 534, (1945).
Hey, Nature, 157, 47, (1946).
Pawsey, Payne-Scott, and McCready, Nature, 157, 158, (1946).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
RYLE, M., VONBERG, D. Solar Radiation on 175 Mc./s. Nature 158, 339–340 (1946). https://doi.org/10.1038/158339b0
Issue Date:
DOI: https://doi.org/10.1038/158339b0
- Springer Nature Limited
This article is cited by
-
Radio Imaging With SWAN
Resonance (2022)
-
A space-based decametric wavelength radio telescope concept
Experimental Astronomy (2018)
-
Radio observations of active galactic nuclei with mm-VLBI
The Astronomy and Astrophysics Review (2017)