Influence of CO2 line profiles on radiative and radiative-convective equilibrium states of the Venus lower atmosphere

Journal of Geophysical Research: Planets

Volumn 115, Issue 6, 2010, Pages

  Takagi, M ^a   Suzuki, K ^b,c   Sagawa, H ^d   Baron, P ^c   Mendrok, J ^c,e   Kasai, Y ^c   Matsuda, Y ^b  

^a UNIVERSITY OF TOKYO   (Japan)

^b TOKYO GAKUGEI UNIVERSITY   (Japan)

^c NATIONAL INSTITUTE OF INFORMATION AND COMMUNICATIONS TECHNOLOGY   (Japan)

^d MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^e LULEÅ UNIVERSITY OF TECHNOLOGY   (Sweden)

Author keywords

[No Author keywords available]

Indexed keywords

POLLACHIUS POLLACHIUS;

EID: 77954482032     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/2009JE003488     Document Type: Article

References (31)

1. Bullock, M. A. (1997), The stability of climate on Venus, Ph.D. thesis, Univ. of Colo. at Boulder, Boulder.
2. Bullock, M. A., and D. H. Grinspoon (2001), The recent evolution of climate on Venus, Icarus, 150, 19-37.
3. Curtis, A. R. (1956), The computation of radiative heating rates in the atmosphere, Proc. R. Soc. London A, 236, 156-159.
4. Esposito, L. W., R. G. Knollenberg, M. Y. Marov, O. B. Toon, and R. P. Turco (1983), The clouds and hazes of Venus, in Venus, edited by D. M. Hunten et al., pp. 484-564, Univ. of Ariz. Press, Tucson.
5. 2, J. Quant. Spectrosc. Radiat. Transfer, 36, 265-270.
6. Goody, R. M., and Y. L. Yung (1996), Atmospheric Radiation: Theoretical Basis, 2nd ed., Oxford Univ. Press, New York.
7. Hollingsworth, J. L., R. E. Young, G. Schubert, C. Covey, and A. S. Grossman (2007), A simple-physics global circulation model for Venus: Sensitivity assessments of atmospheric superrotation, Geophys. Res. Lett., 34, L05202, doi:10.1029/2006GL028567. (Pubitemid 46864494)
8. Kamp, L. W., and F. W. Taylor (1990), Radiative transfer models of the night side of Venus, Icarus, 86, 510-529.
9. Kamp, L. W., F. W. Taylor, and S. B. Calcutt (1988), Structure of Venus's atmosphere from modeling of night-side spectra, Nature, 336, 360-362, doi:10.1038/336360a0.
10. Kido, A., and Y. Wakata (2008), Multiple equilibrium states appearing in a Venus-like atmospheric general circulation model, J. Meteorol. Soc. Jpn., 86, 969-979.
11. 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, 8039-8058, doi:10.1029/JA085iA13p08039.
12. Lee, C, S. R. Lewis, and P. L. Read (2007), Superrotation in a Venus general circulation model, J. Geophys. Res., 112, E04S11, doi:10.1029/ 2006JE002874. (Pubitemid 46957942)
13. Liou, K. N. (2002), An Introduction to Atmospheric Radiation, Int. Geo-phys. Ser., vol.84, 2nd ed., Academic, San Diego, Calif.
14. Matsuda, Y., and T. Matsuno (1978), Radiative-convective equilibrium of the Venusian atmosphere, J. Meteorol. Soc. Jpn., 56, 1-18.
15. Meadows, V. S., and D. Crisp (1996), Ground-based near-infrared observations of the Venus nightside: The thermal structure and water abundance near the surface, J. Geophys. Res., 101, 4595-4622, doi:10.1029/95JE03567.
16. Moskalenko, N. I., Y. A. Il'in, S. N. Parzhin, and L. V. Rodionov (1979), Pressure-induced IR radiation absorption in atmospheres, Atmos. Oceanic Phys., 15, 632-637.
17. Pollack, J. B., and R. Young (1975), Calculations of the radiative and dynamical state of the Venus atmosphere, J. Atmos. Sci., 32, 1025-1037.
18. Pollack, J. B., O. B. Toon, and R. Boese (1980), Greenhouse models of Venus' high surface temperature, as constrained by Pioneer Venus measurements, J. Geophys. Res., 85, 8223-8231, doi:10.1029/JA085iA13p08223.
19. Pollack, J. B., et al. (1993), Near-infrared light from Venus' nightside: A spectroscopic analysis, Icarus, 103, 1-42.
20. Schubert, G. (1983), General circulation and the dynamical state of the Venus atmosphere, in Venus, edited by D. M. Hunten et al., pp. 681-765, Univ. of Ariz. Press, Tucson.
21. Seiff, A. (1983), Thermal structure of the atmosphere of Venus, in Venus, edited by D. M. Hunten et al., pp. 215-279, Univ. of Ariz. Press, Tucson.
22. Seiff, A., et al. (1985), Models of the structure of the atmosphere of Venus from the surface to 100 kilometers altitude, Adv. Space Res., 5(11), 3-58, doi:10.1016/0273-1177(85)90197-8.
23. Staley, D. O. (1970), The adiabatic lapse rate in the Venus atmosphere, J. Atmos. Sci., 27, 219-223.
24. Takagi, M., and Y. Matsuda (1999), Interpretation of Thompson's mechanism for Venus' atmospheric super-rotation and its extension to the spherical geometry, J. Meteorol. Soc. Jpn., 77, 971-983.
25. Takagi, M., and Y. Matsuda (2005), Sensitivity of thermal tides in the Venus atmosphere to basic zonal flow and Newtonian cooling, Geophys. Res. Lett, 32, L02203, doi:10.1029/2004GL022060. (Pubitemid 40473015)
26. Takagi, M., and Y. Matsuda (2006), Dynamical effect of thermal tides in the lower Venus atmosphere, Geophys. Res. Lett., 33, L13102, doi:10.1029/2006GL026168. (Pubitemid 44945912)
27. Takagi, M., and Y. Matsuda (2007), Effects of thermal tides on the Venus atmospheric superrotation, J. Geophys. Res., 112, D09112, doi:10.1029/ 2006JD007901. (Pubitemid 47009838)
28. Tomasko, M. G., L. R. Doose, P. H. Smith, and A. P. Odell (1980), Measurements of the flux of sunlight in the atmosphere of Venus, J. Geophys. Res., 85, 8167-8186, doi:10.1029/JA085iA13p08167.
29. 2 absorption in the 23-pm region at room temperature: Far wings, allowed and collision-induced bands, Appl. Opt, 35, 4863-4870.
30. Urban, J., P. Baron, N. Lautie, N. Schneider, K. Dassas, P. Ricaud, and J. De La Noe (2004), Moliere (v5): A versatile forward-and inversion model for the millimeter and sub-millimeter wavelength range, J. Quant. Spectrosc. Radiat. Transfer, 83, 529-554.
31. Yamamoto, M., and M. Takahashi (2004), Dynamics of Venus' superrotation: The eddy momentum transport processes newly found in a GCM, Geophys. Res. Lett, 31, L09701, doi:10.1029/2004GL019518. (Pubitemid 39032616)