Abstract
ON March 7, 1970, the solar eclipse was observed at 30 and 16 GHz using the Crawford Hill Sun tracker1. At Crawford Hill the eclipse was partial with greatest magnitude of 0.964. The measurement consisted of an accurate determination of the residual flux at the time of greatest magnitude as a proportion of the total solar flux. From these data, the size of the radio Sun at 30 and 16 GHz is determined.
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
Rent or buy this article
Prices vary by article type
from$1.95
to$39.95
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
References
Wilson, R. W., Bell System Tech. J., 48, 1383 (1969).
Simon, M., Astrophys. J., 141, 1513 (1965).
Simon, M., and Zirin, H., Solar Phys., 9, 317 (1969).
Castelli, J. P., and Aarons, J., in Solar System Radio Astronomy (edit. by Aarons, J.) (Plenum Press, NY, 1965).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
WRIXON, G. Solar Eclipse Measurements at 16 and 30 GHz. Nature 227, 1231–1232 (1970). https://doi.org/10.1038/2271231a0
Received:
Issue Date:
DOI: https://doi.org/10.1038/2271231a0
This article is cited by
-
Solar Radius at Subterahertz Frequencies and Its Relation to Solar Activity
Solar Physics (2017)
-
Interferometer observations of the solar brightness distribution at 8.6 mm wavelength
Solar Physics (1976)
-
The radio radius of the Sun at millimeter and centimeter wavelengths
Solar Physics (1973)
-
High resolution observations of the chromosphere at mm and cm wavelengths
Solar Physics (1971)
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.