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Automatic Radio-celestial Navigation

Published online by Cambridge University Press:  18 January 2010

Gene R. Marner
Gene R. Marner
Affiliation:
(Collins Radio Company)
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Extract

The accurate, continuous determination of position, heading and course at all times, under all normal operational conditions, would be very desirable. This ideal has not been achieved for flights or voyages of long duration, but the many developments of recent years begin to give some promise that it may be possible. For high altitude aircraft the continuous optical observation of celestial bodies offers an evident solution, and doppler systems can give continuous speed over ground. For ships, however, the attainment of such an ideal navigation system is difficult. The various shore-based radio navigation systems have made important contributions, as have the development of inertial techniques. In addition, automatic optical sextants have been developed which can be used in clear weather.

Information

Type
Research Article
Information
The Journal of Navigation , Volume 12 , Issue 3-4 , October 1959 , pp. 249 - 259
Copyright
Copyright © The Royal Institute of Navigation 1959

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References

REFERENCES

Bean, B. R. and Cahoon, B. A. (1957). The use of surface weather observations to predict the total atmospheric bending of radio rays at small elevation angles, National Bureau of Standards Report 5082.Google Scholar
Bellville, W. H., Holt, J. M. and Iliff, W. R. (1958). Atmospheric factors affecting precision location of celestial radio sources, URSI Annual Meeting.Google Scholar
Hagen, J. P. (1951). Temperature gradient in the Sun's atmosphere measured at radio frequencies, Astrophys. J., 113, 547.CrossRefGoogle Scholar
Hepperle, C. M., Giberson, W. E., Malandrinos, H. J. and Ringoen, R. M. (1947). Interim report on the microwave radiometry project, Collins Research Report No. 102.Google Scholar
Mansur, G. F. (1958). The output fluctuations of radiometers, URSI Annual Meeting.Google Scholar
Marner, G. R. (1955). High precision computer for automatic solution of the celestial triangle, Navigation, 4, 281.CrossRefGoogle Scholar
Marner, G. R. (1956). Radiometric measurement of 8.7 mm. atmospheric attenuation, Doctoral Thesis, State University of lowa, Collins Engineering Report 479.Google Scholar
Marner, G. R. (1958a). New determinations of atmospheric microwave absorption by radio-astronomical methods, URSI Annual Meeting.Google Scholar
Marner, G. R. (1958b). Atmospheric radiation received by directional antennas, URSI Annual Meeting.Google Scholar
Marner, G. R. and Iliff, W. R. (1958). Observed 8.7 mm. refraction as a function of surface meteorological conditions, URSI Annual Meeting.Google Scholar
Marner, G. R. and Ringoen, R. M. (1956). Atmospheric refraction of 8.7 mm. radiation, Inst. of Radio Engineers Convention Record, March 1956, and Collins Technical Report 162, 20 April 1956.Google Scholar
Marner, G. R., Stewart, C., Stiles, R. G. and Whear, H. (1958). Antarctic evaluation of the radio sextant, presented at the annual meeting of the (American) Institute of Navigation. To be published in Navigation.Google Scholar
Marner, G. R. and Willis, T. R. (1959). A precision solar-lunar radio sextant, to be presented at the Third National Convention on Military Electronics, Washington, D.C., 1 July 1959.Google Scholar
McCoy, D. O. (1955). An all-weather radio sextant, Navigation, 4, 309.CrossRefGoogle Scholar
Roman, N. G. and Haddock, F. T. (1956). A model for nonthermal radio-source spectra, Astrophys. J., 124, 35.CrossRefGoogle Scholar
Whitfield, G. R. (1957). The spectra of radio stars, Mon. Not. R. astr. Soc., 117, 680.CrossRefGoogle Scholar