The Georgia Tech high sensitivity microwave measurement system

Astrophysics and Space Science

Volumn 236, Issue 1, 1996, Pages 111-124

  Deboer, David R ^a   Steffes, Paul G ^a  

^a GEORGIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0040051925     PISSN: 0004640X     EISSN: None     Source Type: Journal    
DOI: 10.1007/BF00644325     Document Type: Article

References (11)

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2. DePater, I. and Mitchell, D.L.: 1993, Radio observations of the planets: the importance of laboratory measurements, J. Geophys. Res. 98, 5471-5490.
3. 4), J. Geophys. Res. (Planets) 96, 17, 471-17, 476.
4. 2) under simulated conditions for the Venus atmosphere, Icarus 97, 200-210.
5. Jenkins, J.M. and Steffes, P.G.: 1988, Constraints on the microwave opacity of gaseous methane and water vapor in the Jovian atmosphere, Icarus 76, 378-382.
6. 3) under simulated Jovian conditions, Icarus 81, 386-395.
7. Spilker, T.R.: 1990, Laboratory measurements of microwave absorptivity and refractivity spectra of gas mixtures applicable to giant planet atmospheres, Ph.D. Thesis, Stanford University.
8. Steffes, P.G.: 1985, Laboratory measurements of the microwave opacity and vapor pressure of sulfuric acid under simulated conditions for the middle atmosphere of Venus, Icarus 64, 576-585.
9. 3) under simulated conditions for the Jovian atmosphere, Icarus 52, 35-47.
10. Townes, C.H. and Schawlow, A.L.: 1955, Microwave Spectroscopy, Dover Press, New York.
11. Tyler, G.L. and Howard, H.T.: 1969, Refractivity of carbon dioxide under simulated Martian conditions, Radio Sci. 4, 899-904.