Abstract
Martyn1 and Shklovsky2 have suggested that plasma oscillations in the corona may provide a source of radio-frequency radiation. It has also been shown that radiation of a few metres wave-length must originate at heights above the chromosphere of the order of a solar radius.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
References
Martyn, Nature, 159, 26 (1947).
Shklovsky, Nature, 159, 752 (1947).
Appleton and Hey, Phil. Mag., 37, 73 (1946).
Allen, private communication.
Williams and Hands, Nature, 158, 511 (1946).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
WILLIAMS, S. Solar Radio-Frequency Noise Fluctuations and Chromospheric Flares. Nature 160, 708–709 (1947). https://doi.org/10.1038/160708a0
Issue Date:
DOI: https://doi.org/10.1038/160708a0
Comments
By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.