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Wideband Spectrometers for Millimetre Wavelengths

Published online by Cambridge University Press:  14 August 2015

B. J. Robinson*
Affiliation:
Division of Radiophysics, CSIRO, Sydney, Australia

Extract

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Millimetre-wave spectral lines show a wide range of linewidths, from 0.1 km s-1 in dark clouds to 30 km s-1 in some massive molecular clouds; at 100 GHz the corresponding Doppler widths range from 33 kHz to 10 MHz. SiO masers at 86 GHz have two lines typically 1 MHz wide spaced by 6 MHz. For most applications a resolution of 100 or 250 kHz is suitable.

Type
Research Article
Copyright
Copyright © Reidel 1980 

References

Hecht, D.L.: 1977, IEEE Ultrasonics Symposium Proceedings.Google Scholar
Kaifu, N., Ukita, N., Chikada, Y., and Miyaji, T.: 1977, Publ. Astron. Soc. Japan 29, p. 429.Google Scholar
Lambert, L.E.: 1962, I.R.E. Int. Conv. Rec. 10, Pt. 6, p. 69.Google Scholar
Mauzy, B.: 1974, NRAO Electronics Division Report No. 146.Google Scholar
Milne, D.K., and Cole, T.W.: 1979, Proc. Inst. Radio Electron. Eng. Aust. 40, p. 43.Google Scholar