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A 10 Micron Heterodyne Receiver for Ultra High Resolution Astronomical Spectroscopy

Published online by Cambridge University Press:  14 August 2015

D. Buhl ,
G. Chin ,
J. Faris ,
T. Kostiuk ,
M. J. Mumma  and
D. Zipoy
D. Buhl
Affiliation:
Infrared and Radio Astronomy Branch NASA/Goddard Space Flight Center Greenbelt, MD 20771
G. Chin
Affiliation:
Infrared and Radio Astronomy Branch NASA/Goddard Space Flight Center Greenbelt, MD 20771
J. Faris
Affiliation:
Infrared and Radio Astronomy Branch NASA/Goddard Space Flight Center Greenbelt, MD 20771
T. Kostiuk
Affiliation:
Infrared and Radio Astronomy Branch NASA/Goddard Space Flight Center Greenbelt, MD 20771
M. J. Mumma
Affiliation:
Infrared and Radio Astronomy Branch NASA/Goddard Space Flight Center Greenbelt, MD 20771
D. Zipoy
Affiliation:
Department of Astronomy, University of Maryland

Extract

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Infrared heterodyne spectroscopy is extremely useful in determining by precise measurements of atomic and molecular infrared line spectra the molecular abundances, velocity structure, and excitation conditions of the interstellar medium, and the temperature- and pressure-profiles of planetary atmospheres (cf. Kostiuk et al. 1977, Betz et al. 1976, 1977, Abbas et al. 1978).

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 633 - 636
Copyright
Copyright © Reidel 1980 

References

Abbas, M.M., Kostiuk, T., Mumma, M.J., Buhl, D., Kunde, V., and Brown, L.W.: 1978, Geophysical Research Letters 5, 317.CrossRefGoogle Scholar
Betz, A.L., Johnson, M.A., McLaren, R.A., and Sutton, E.C.: 1976, Astrophys. J. (Letters) 208, L141.Google Scholar
Betz, A.L., McLaren, R.A., Sutton, E.C., and Johnson, M.A.: 1977, Icarus 30, 650.Google Scholar
Kostiuk, T., Mumma, M.J., Hillman, J.J., Buhl, D., and Brown, L.W.: 1977, Infrared Physics 17, 431.Google Scholar
Mumma, M.J., Kostiuk, T., and Buhl, D.: 1978, Opt. Eng. 17, 50.Google Scholar