Abstract
ON October 21, 1965, a rare solar event occurred. The “Sun-grazing” Comet 1965f (Ikeya-Seki) passed through the solar corona at a perihelion distance of less than 500,000 km from the Sun's surface, or 1.66 R0 from its centre, where R0 is the optical solar radius1. The rarity of such an event is shown by the fact that in the 23 yr from the discovery of radio emissions from the Sun in 1942 to the time of the present investigation, only two other known comets passed within 6 R0 of the centre of the Sun. These were Comet du Toit (1945 VII), the perihelion distance of which on December 18, 1945, was 1.35 R0, and Comet Pereyra (1963 V), the perihelion distance of which on August 23, 1963, was 1.11 R0 (ref. 2).
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
International Astronomical Union (Nice, France). Circulars Nos. 1947 (1965); and 1949 (1966).
Mem. B.A.A., 39 (1961); Mem. B.A.A., 40 (1966).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
CROOM, D. Search for Very High Frequency Radiation resulting from the Passage of Comet 1965f through the Solar Corona. Nature 213, 1002–1003 (1967). https://doi.org/10.1038/2131002a0
Received:
Issue Date:
DOI: https://doi.org/10.1038/2131002a0
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.