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Radio-astronomy, Radiometry and Infra-red Techniques

Published online by Cambridge University Press:  18 January 2010

C. M. Cade
Affiliation:
(Kelvin & Hughes Ltd.)

Extract

The year 1932 was one which had no great apparent significance for navigators, and yet it saw the commencement of two new lines of research which today, after an interval of more than a quarter-of-a-century, promise important contributions to the safety of navigators both at sea and in the air.

The two lines of research were superficially quite unrelated, but fundamentally they relied upon the same principle—the detection of radiant energy emitted by objects solely as a result of their temperature. The first of these small beginnings was the discovery by K. G. Jansky that radio waves could be detected from extra-terrestrial sources: the second was the commencement by the U.S. Signal Corps Engineering Laboratories of an intensive study of infra-red devices with the object of obtaining night vision without illumination of the field of view.

From Jansky's discovery has sprung the whole science of radio astronomy, which has revolutionized our ideas about the universe, and brought in its wake, as one practical benefit, the radio sextant. From the work of the U.S. Signal Corps there resulted a number of very useful infra-red components, including the pneumatic detector, better known as the Golay cell.

Type
Research Article
Copyright
Copyright © The Royal Institute of Navigation 1961

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References

REFERENCES

1Jansky, K. G. (1932). Proc. Inst. Radio Engrs, N.Y., 20, 1920.Google Scholar
2Golay, M. J. E. (1947). Review of Scientific Instruments, 18, 357.CrossRefGoogle Scholar
3Pawsey, J. L. and Smerd, S. F. (1953). The Sun, Chicago U.P.Google Scholar
4Sinton, W. M. (1955). J. Opt. Soc. Amer., 45, 975.CrossRefGoogle Scholar
5Kraus, J. D. (1956). Nature, Lond., 178, 33, 103, 159.CrossRefGoogle Scholar
6Burke, B. F. and Franklin, K. L. (1955). J. Geophys. Res., 60, 213.CrossRefGoogle Scholar
7Ts'e-Tsung, Hsi (1955). Acta Astronomica Sinica, 3, 183.Google Scholar
8Bolton, J. G., Stanley, G. J. and Slee, O. B. (1949). Nature, Lond., 164, 101.CrossRefGoogle Scholar
9Allen, C. W. (1955). Astrophysical Quantities, Athlone Press, London.Google Scholar
10Hanbury Brown, R. and Hazard, C. (1952). Nature, Lond., 170, 364.CrossRefGoogle Scholar
11Bolton, J. G., Stanley, G. J. and Slee, O. B. (1949). Nature, Lond., 164, 101.CrossRefGoogle Scholar
12Reber, G. (1944). Astr. J., 100, 279.CrossRefGoogle Scholar
13Baade, W., and Minkowski, R. (1954). Astr. J., 119, 206, 215.CrossRefGoogle Scholar
14Sadler, D. H. (1956). This Journal, 9, 1.Google Scholar
Marner, G. R. (1959), This Journal, 12, 249.Google Scholar
Cade, C. M. (1960), This Journal, 13, 70.Google Scholar
15Klass, P. J. (1957). Aviation Week, issue of July 1st.Google Scholar
16Cade, C. M. (1960). British Communications and Electronics, 7, 414 and 510.Google Scholar
17Nichols, L. W. (1959), et al. Proc. Inst. Radio Engrs, N.Y., 47, 1611.Google Scholar
18Cade, C. M. (1959). British Communications and Electronics, 6, 592.Google Scholar
19Huxford, W. S. and Platt, J. R. (1948). J. Opt. Soc. Amer., 38, 253.CrossRefGoogle Scholar