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  1. Baranov, Y. I. and W. J. Lafferty (2011), The water-vapor continuum and selective absorption in the 3–5 μm spectral region at temperatures from 311 to 363 K, J. Quant. Spectrosc. Radiat. Transfer, 112(8), 1304–1313, doi:10.1016/j.jqsrt.2011.01.024.
  2. Barstow, J. K., C. C. C. Tsang, C. F. Wilson, P. G. J. Irwin, F. W. Taylor, K. McGouldrick, P. Drossart, G. Piccioni, and S. Tellmann (2012), Models of the global cloud structure on Venus derived from Venus Express observations, Icarus, 217, 542–560, doi:10.1016/j.icarus.2011.05.018.
  3. Bézard, B., A. Fedorova, J.-L. Bertaux, A. Rodin, and O. Korablev (2011), The 1.10- and 1.18-μm nightside windows of Venus observed by SPICAV-IR aboard Venus Express, Icarus, 216(1), 173–183, doi:10.1016/j.icarus.2011.08.025.
  4. Biermann, U. M., B. P. Luo, and Th. Peter (2000), Absorption Spectra and Optical Constants of Binary and Ternary Solutions of H2SO4, HNO3, and H2O in the Mid Infrared at Atmospheric Temperatures, J. Phys. Chem. A, 104(4), 783–793, doi:10.1021/jp992349i.
  5. Clancy, R. T., B. J. Sandor, and G. H. Moriarty-Schieven (2008), Venus upper atmospheric CO, temperature, and winds across the afternoon/evening terminator from June 2007 JCMT sub-millimeter line observations, Planet. Space Sci., 56, 1344 - 1354, doi:10.1016/j.pss.2008.05.007.
  6. Clancy, R. T., B. J. Sandor, and G. Moriarty-Schieven (2012), Circulation of the Venus upper mesosphere/lower thermosphere: Doppler wind measurements from 2001–2009 inferior conjunction, sub-millimeter CO absorption line observations, Icarus, 217, 794–81, doi:10.1016/j.icarus.2011.05.021.
  7. Clancy, R. T., B. J. Sandor, and G. Moriarty-Schieven (2012), Thermal structure and CO distribution for the Venus mesosphere/lower thermosphere: 2001–2009 inferior conjunction sub-millimeter CO absorption line observations, Icarus, 217, 779–793, doi:10.1016/j.icarus.2011.05.032.
  8. Clancy, R. T. and D. O. Muhleman (1985), Diurnal CO variations in the Venus mesophere from CO microwave spectra, Icarus, 64, 157–182, doi:10.1016/0019-1035(85)90084-3.
  9. Clancy, R. T. and D. O. Muhleman (1991), Long-term (1979–1990) changes in the thermal, dynamical, and compositional structure of the Venus Mesosphere as inferred from microwave spectral line observations of 12CO, 13CO, and C18O, Icarus, 89, 129–146, doi:10.1016/0019-1035(91)90093-9.
  10. Clough, S. A., M. W. Shephard, E. J. Mlawer, J. S. Delamere, M. Iacono, K. Cady-Pereira, S. Boukabara, and P. D. Brown (2005), Atmospheric radiative transfer modeling: a summary of the AER codes, J. Quant. Spectrosc. Radiat. Transfer, 91(2), 233–244, doi:10.1016/j.jqsrt.2004.05.058.
  11. Dickel, J. R. (1967), 6-cm Observations and the Microwave Spectrum of Venus, Icarus, 6, 417–426, doi:10.1016/0019-1035(67)90034-6.
  12. Encrenaz, T., E. Lellouch, G. Paubert, and S. Gulkis (1991), First detection of HDO in the atmosphere of Venus at radio wavelengths - an estimate of the H2O vertical distribution, A&A, 246, L63–L66.
  13. Encrenaz, Th., E. Lellouch, J. Cernicharo, G. Paubert, S. Gulkis, and T. Spilker (1995), The Thermal Profile and Water Abundance in the Venus Mesosphere from H2O and HDO Millimeter Observations, Icarus, 117, 162–172, doi:10.1006/icar.1995.1149.
  14. Fahd, A. K. and P. G. Steffes (1991), Laboratory Measurement of the Millimeter Wave Properties of Liquid Sulfuric Acid (H2SO4), J. Geophys. Res., 96(E2), 17471–17476, doi:10.1029/91JE01684.
  15. Fenn, R. W., S. A. Clough, W. O. Gallery, R. E. Good, F. X. Kneizys, J. D. Mill, L. S. Rothman, and E. P. Shettle (1985), Handbook of Geophysics and the Space Environment, chap. Optical and infrared properties of the atmosphere, Air Force Geophysics Laboratory, Hanscom AFB, MA, ASIN B000RNNASO.
  16. Forget, F., K. Dassas, M. Capderou, S. Lebonnois, G. Beaudin, A. Deschamps, P. Encrenaz, B. Germain, M. Gheudin, A. Maestrini, C. Prigent, B. Thomas, P. Ricaud, J. Urban and, M. Janssen, M. Frerking, S. Gulkis, L. Riley, M. Allen, T. Encrenaz, E. Lellouch, P. Hartogh, R. T. Clancy, E. Chassefiere, F. Lefevre, F. Montmessin, A. Emrich, D. Murtagh, R. Booth, U. Frisk, and A. Raisanen (2003), MAMBO: THE MARS ATMOSPHERE MICROWAVE BRIGHTNESS OBSERVER, In: Mars atmosphere modelling and observations Workshop, Granada, Spain.
  17. Gamache, Robert R., Anne L. Laraia, and Julien Lamouroux (2011), Half-widths, their temperature dependence, and line shifts for the HDO-CO2 collision system for applications to CO2-rich planetary atmospheres, Icarus, 213(2), 720–730, doi:10.1016/j.icarus.2011.03.021.
  18. Gurwell, M. A., G. J. Melnick, V. Tolls, E. A. Bergin, and B. M. Patten (2007), SWAS observations of water vapor in the Venus mesosphere, Icarus, 188, 28–304, doi:10.1016/j.icarus.2006.12.004.
  19. Haus, R. and G. Arnold (2010), Radiative transfer in the atmosphere of Venus and application to surface emissivity retrieval from VIRTIS/VEX measurements, Planet. Space Sci., 58(12), 1578–1598, doi:10.1016/j.pss.2010.08.001.
  20. Ho, W., I. A. Kaufman, and P. Thaddeus (1966), Laboratory measurement of microwave absorption in models of the atmosphere of Venus, J. Geophys. Res., 71(21), 5091–5108.
  21. Hummel, J. R., E. P. Shettle, and D. R. Longtin (1988), A New Background Stratospheric Aerosol Model for Use in Atmospheric Radiation Models, AFGL-TR-88-0166, Air Force Geophysics Laboratory, Hanscom AFB, MA.
  22. Imamura, T., T. Toda, A. Tomiki, D. Hirahara, T. Hayashiyama, N. Mochizuki, Z. Yamamoto, T. Abe, T. Iwata, H. Noda, et al. (2011), Radio occultation experiment of the Venus atmosphere and ionosphere with the Venus orbiter Akatsuki, Earth Planets Space, 63(6), 493–501.
  23. James, E. P., O. B. Toon, and G. Schubert (1997), A Numerical Microphysical Model of the Condensational Venus Cloud, Icarus, 129, 147–171, doi:10.1006/icar.1997.5763.
  24. Jenkins, J. M., M. A. Kolodner, B. J. Butler, S. H. Suleimann, and P. G. Steffes (2002), Microwave Remote Sensing of the Temperature and Distribution of Sulfur Compounds in the Lower Atmosphere of Venus, Icarus, 158(2), 312–328, doi:10.1006/icar.2002.6894.
  25. Kellermann, K. I. (1966), The thermal radio emission from Mercury, Venus, Mars, Saturn, and Uranus, Icarus, 5, 478–490, doi:10.1016/0019-1035(66)90060-1.
  26. Knollenberg, R. G. and D. M. Hunten (1980), The Microphysics of the Clouds of Venus: Results of the Pioneer Venus Particle Size Spectrometer Experiment, J. Geophys. Res., 85(A13), 8039–8058, doi:10.1029/JA085iA13p08039.
  27. Koukouli, M. E., P. G. J. Irwin, and F. W. Taylor (2005), Water vapor abundance in Venus' middle atmosphere from Pioneer Venus OIR and Venera 15 FTS measurements, Icarus, 173(1), 84–99, doi:10.1016/j.icarus.2004.08.023.
  28. Krasnopolsky, V. A. (1985), Chemical Composition of Venus Clouds, Planet. Space Sci., 33(1), 109–117, doi:10.1016/0032-0633(85)90147-3.
  29. Lopez-Valverde, M. A., L. Montabone, M. Sornig, and G. Sonnabend (2016), On the Retrieval of Mesospheric Winds on Mars and Venus from Ground-based Observations at 10 μm, Astrophys. J., 816(2), 103, doi:10.3847/0004-637X/816/2/103.
  30. Oschlisniok, J., B. Häusler, M. Pätzold, G. L. Tyler, M. K. Bird, S. Tellmann, S. Remus, and T. Andert (2012), Microwave absorptivity by sulfuric acid in the Venus atmosphere: First results from the Venus Express Radio Science experiment VeRa, Icarus, 221(2), 940–948, doi:10.1016/j.icarus.2012.09.029.
  31. Parish, H. F., G. Schubert, C. Covey, R. L. Walterscheid, A. Grossman, and S. Lebonnois (2011), Decadal variations in a Venus general circulation model, Icarus, 212(1), 42–65, doi:10.1016/j.icarus.2010.11.015.
  32. Payne, V. H., E. J. Mlawer, K. E. Cady-Pereira, and J.-L. Moncet (2011), Water Vapor Continuum Absorption in the Microwave, IEEE Geosci. Remote Sens., 49(6), 2194–2208, doi:10.1109/TGRS.2010.2091416.
  33. Rengel, M., P. Hartogh, and Ch. Jarchow (2008), HHSMT observations of the Venusian mesospheric temperature, winds, and CO abundance around the MESSENGER flyby, Planet. Space Sci., 56, 1688–1695, doi:10.1016/j.pss.2008.07.014.
  34. Rossow, W. B. and C. Sagan (1975), Microwave Boundary Conditions on the Atmosphere and Clouds of Venus, J. Atmos. Sci., 32, 1164–1176, doi:10.1175/1520-0469(1975)032<1164:MBCOTA>2.0.CO;2.
  35. Sandor, B. J. and R. T. Clancy (2005), Water vapor variations in the Venus mesosphere from microwave spectra, Icarus, 177, 129–143, doi:10.1016/j.icarus.2005.03.020.
  36. Sandor, B. J., R. T. Clancy, G. Moriarty-Schieven, and F. P. Mills (2010), Sulfur chemistry in the Venus mesosphere from SO2 and SO microwave spectra, Icarus, 208, 49–60, doi:10.1016/j.icarus.2010.02.013.
  37. Sandor, B. and R. T. Clancy (2011), Venus 70–100 km Photochemistry: HCl, H2SO4, SO2, SO, ClO Sub-mm Observations Observations from the JCMT, , Presentation at 2011 VEXAG International Venus Workshop, Chantilly, Virginia, USA.
  38. Sandor, B. J. and R. T. Clancy (2012), Observations of HCl altitude dependence and temporal variation in the 70–100 km mesosphere of Venus, Icarus, 220, 618–626, doi:10.1016/j.icarus.2012.05.016.
  39. Sandor, B. J., R. T. Clancy, and G. Moriarty-Schieven (2012), Upper limits for H2SO4 in the mesosphere of Venus, Icarus, 217, 839–844, doi:10.1016/j.icarus.2011.03.032.
  40. Steele, H. M. and P. Hamill (1981), Effects of Temperature and Humidity on the Growth and Optical Properties of Sulphuric Acid-Water Droplets in the Stratosphere, J. Atmos. Sci., 12(6), 517–528, doi:10.1016/0021-8502(81)90054-9.
  41. Steffes, P. G. (1985), Laboratory measurements of the microwave opacity and vapor pressure of sulfuric acid vapor under simulated conditions for the middle atmosphere of Venus, Icarus, 64(3), 576–585, doi:10.1016/0019-1035(85)90077-6.
  42. Stratton, A. J. (1968), Optical and Radio Refraction on Venus, J. Atmos. Sci., 25, 666–667, doi:10.1175/1520-0469(1968)025<0666:OARROV>2.0.CO;2.
  43. Ulich, B.L., J.R. Cogdell, and J.H. Davis (1973), Planetary brightness temperature measurements at 8.6 mm and 3.1 mm wavelengths, Icarus, 19, 59–82, doi:10.1016/0019-1035(73)90139-5.
  44. Ward, D. B., G. E. Gull, and M. Harwit (1977), Far-infrared spectral observations of Venus, Mars, and Jupiter, Icarus, 30, 295–300, doi:10.1016/0019-1035(77)90162-2.
  45. Warnock, W. W. and J. R. Dickel (1972), Venus: Measurements of brightness temperatures in the 7-?15 cm wavelength range and theoretical radio and radar spectra for a two-layer subsurface model, Icarus, 17, 682–691, doi:10.1016/0019-1035(72)90032-2.
  46. Wilson, W. J., M. J. Klein, R. K. Kahar, S. Gulkis, E. T. Olsen, and P. T. P. Ho (1981), Venus I. Carbon monoxide distribution and molecular-line searches, Icarus, 45, 624–637, doi:10.1016/0019-1035(81)90029-4.