In search of water vapor on Jupiter: Laboratory measurements of the microwave properties of water vapor under simulated jovian conditions

Icarus - Tập 212 - Trang 210-223 - 2011
Bryan M. Karpowicz1, Paul G. Steffes2
1School of Earth and Atmospheric Sciences, Georgia Institute of Technology, Atlanta, GA 30332-0250, United States
2School of Electrical and Computer Engineering, Georgia Institute of Technology, Atlanta, GA 30332-0250, United States

Tài liệu tham khảo

Bleaney, 1950, The inversion spectra of NH3, CH3Cl and CH3Br at high pressures, Proc. Phys. Soc.: Sec. A, 63, 483, 10.1088/0370-1298/63/5/307 DeBoer, D.R., 1995. The microwave opacity of H2S with applications to the tropospheric vertical structure of the jovian planets. Ph.D. Thesis, Georgia Institute of Technology. DeBoer, 1996, The Georgia Tech high sensitivity microwave measurement system, Astrophys. Space Sci., 236, 111, 10.1007/BF00644325 de Pater, 2005, Retrieval of water in Jupiter’s deep atmosphere using microwave spectra of its brightness temperature, Icarus, 173, 425, 10.1016/j.icarus.2004.06.019 Fahd, A.K., 1992. Study and interpretation of the millimeter-wave spectrum of venus. Ph.D. Thesis, Georgia Institute of Technology, Atlanta. Goodman, G.C., 1969. Models of Jupiter’s atmosphere. Ph.D. Thesis, University of Illinois. Hanley, T.R., 2008. The microwave opacity of ammonia and water vapor: Application to remote sensing of the atmosphere of Jupiter. Ph.D. Thesis, Georgia Institute of Technology. Hanley, 2007, A high-sensitivity laboratory system for measuring the microwave properties of gases under simulated conditions for planetary atmospheres, Radio Sci, 42, 1, 10.1029/2007RS003693 Hanley, 2009, A new model of the hydrogen and helium broadened microwave opacity of ammonia based on extensive laboratory measurements, Icarus, 202, 316, 10.1016/j.icarus.2009.02.002 Ho, 1966, Laboratory measurement of microwave absorption in models of the atmosphere of Venus, J. Geophys. Res., 71, 5091, 10.1029/JZ071i021p05091 Hoffman, 2001, Laboratory measurements of the microwave opacity of phosphine: Opacity formalism and application to the atmospheres of the outer planets, Icarus, 152, 172, 10.1006/icar.2001.6622 Janssen, 2005, Microwave remote sensing of Jupiter’s atmosphere from an orbiting spacecraft, Icarus, 173, 447, 10.1016/j.icarus.2004.08.012 Joiner, 1991, Modeling of Jupiter’s millimeter wave emission utilizing laboratory measurements of ammonia (NH3) opacity, J. Geophys. Res., 96, 17463, 10.1029/91JE01740 Karpowicz, B.M., 2010. In search of water vapor on Jupiter: Laboratory measurements of the microwave properties of water vapor and simulations of Jupiter’s microwave emission in support of the Juno mission. Ph.D. Thesis, Georgia Institute of Technology. Leachman, J., 2007. Fundamental equations of state for parahydrogen, normal hydrogen, and orthohydrogen. Master’s thesis, University of Idaho. Matousek, S., 2005. The Juno new frontiers mission. Tech. Rep. IAC-05-A3.2.A.04, California Institute of Technology. Matthaei, 1980 McCarty, 1990, A new wide range equation of state for helium, Adv. Cryogenic Eng., 35, 1465 Mohammed, 2003, Laboratory measurements of the ka-band (7.5mm to 9.2mm) opacity of phosphine (PH3) and ammonia (NH3) under simulated conditions for the Cassini–Saturn encounter, Icarus, 166, 425, 10.1016/j.icarus.2003.09.003 Morris, 1970, Microwave absorption by gas mixtures at pressures up to several hundred bars, Aus. J. Phys., 23, 335 Payne, 2008, Air-broadened half-widths of the 22- and 183-GHz water-vapor lines, IEEE Trans. Geosci. Rem. Sens., 46, 3601, 10.1109/TGRS.2008.2002435 Payne, V., Mlawer, E., Cady-Pereira, K., Moncet, J., 2011. Water vapor continuum absorption in the microwave. IEEE Trans. Geosci. Rem. Sens., in press. Pozar, 1998 Rabinovich, 1995 Rosenkranz, 1998, Water vapor microwave continuum absorption: A comparison of measurements and models, Radio Sci., 33, 919, 10.1029/98RS01182 Rothman, L.S. et al., 2009. The HITRAN 2008 molecular spectroscopic database. J. Quant. Spectrosc. Radiat. Trans. 110, 533–572. Seward, 1981, The system hydrogen–water up to 440°C and 2500 bar pressure, Ber. Bunsenges. Phys. Chem., 85, 2, 10.1002/bbpc.19810850103 Seward, T.M., Suleimenov, O.M., Franck, E.U., 2000. pVT data for binary H2–H2O mixtures in the homogeneous region to 450°C and 2500 bar. In: Steam, Water, and Hydrothermal Systems: Physics and Chemistry Meeting the Needs of Industry: Proceedings of the 13th International Conference on the Properties of Water and Steam. NRC Research Press, pp. 104–109. Tyler, 1969, Refractivity of carbon dioxide under simulated martian conditions, Radio Sci., 4, 899, 10.1029/RS004i010p00899 von Zahn, 1998, Helium in Jupiter’s atmosphere: Results from the Galileo probe helium interferometer experiment, J. Geophys. Res., 103, 22815, 10.1029/98JE00695 Wagner, W., Pruß, A., 2002. The IAPWS formulation 1995 for the thermodynamic properties of ordinary water substance for general and scientific use. J. Phys. Chem. Ref. Data 387–535.