Limits to the Sub-millimetre isotropic background [Letter]

Beckman, J. E., Ade, Peter A. R. ORCID: https://orcid.org/0000-0002-5127-0401, Huizinga, J. S., Robson, E. I., Vickers, D. G. and Harries, J. E. 1972. Limits to the Sub-millimetre isotropic background [Letter]. Nature 237 (5351) , pp. 154-157. 10.1038/237154a0

Full text not available from this repository.

Abstract

A phase-modulated Michelson interferometer and a helium cooled Rollin photoconductive far infrared detector, at the focus of a 35 cm aperture Cassegrain telescope, were flown at a height of 12.1 km from the Royal Aircraft Establishment, Farnborough, in a Comet 2E aircraft, on November 11, 12 and 16, 1971. The emission spectrum of the stratosphere was obtained in the wavenumber range from 36 cm−1 to 5 cm−1 (wavelengths 280 µm to 2 mm)3. Here we describe an analysis of a portion of this spectrum for features produced by sources outside the Earth's atmosphere.

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Publisher:	Nature Publishing Group
ISSN:	0028-0836
Last Modified:	25 Oct 2022 09:49
URI:	https://orca.cardiff.ac.uk/id/eprint/60185

Citation Data

Cited 6 times in Scopus. View in Scopus. Powered By Scopus® Data

Actions (repository staff only)

Edit Item