The structure of the Uranian atmosphere - Constraints from the geometric albedo spectrum and H2 and CH4 line profiles

[1]  E. I. Robson,et al.  Submillimeter and millimeter observations of Uranus and Neptune , 1986 .

[2]  J. F. Appleby.  Radiative-convective equilibrium models of Uranus and Neptune , 1986 .

[3]  J. Pollack,et al.  Estimates of the bolometric albedos and radiation balance of Uranus and Neptune , 1986 .

[4]  S. Whitcomb,et al.  Far-infrared and submillimeter brightness temperatures of the giant planets , 1985 .

[5]  Bradford A. Smith,et al.  Spatial variability of aerosols in the atmosphere of Uranus. , 1985 .

[6]  R. Silverberg,et al.  Atmospheric temperature profiles of Uranus and Neptune , 1985 .

[7]  J. S. Neff,et al.  Absolute spectrophotometry of Titan, Uranus, and Neptune: 30,500–10,500 Å , 1984 .

[8]  J. Bergstralh,et al.  Properties of the upper tropospheres of Uranus and Neptune derived from observations at visible to near-infrared wavelengths , 1984 .

[9]  G. Orton,et al.  Temperature Structures and Infrared-Derived Properties of the Atmosphere of Uranus and Neptune , 1984 .

[10]  J. S. Neff,et al.  A Determination of the Bolometric Albedo of Uranus and Neptune , 1984 .

[11]  C. E. Keffer,et al.  Limits on the intramolecular relaxation rate for high vibrational overtones of methane , 1984 .

[12]  P. Gierasch,et al.  Global variation of the para hydrogen fraction in Jupiter's atmosphere and implications for dynamics on the outer planets , 1984 .

[13]  K. Baines.  Interpretation of the 6818.9-Å methane feature observed on Jupiter, Saturn, and Uranus☆ , 1983 .

[14]  William H. Smith,et al.  High-resolution observations of the 6815-Å band of methane in the major planets , 1983 .

[15]  G. Lockwood,et al.  The albedo of Uranus , 1983 .

[16]  V. G. Teifel.  Methane abundance in the atmosphere of Uranus , 1983 .

[17]  W. Smith,et al.  Line positions and strengths in the H/sub 2/ quadrupole spectrum , 1982 .

[18]  D. Hunten,et al.  Conversion of para and ortho hydrogen in the Jovian planets , 1982 .

[19]  G. Orton,et al.  Evidence for Thermal Inversions in the Lower Stratospheres of Uranus and Neptune. , 1981 .

[20]  J. Elias,et al.  Orbits of nine Uranian rings , 1981 .

[21]  A. R. Rivolo,et al.  Observations of Uranus, Neptune, and Titan by the International Ultraviolet Explorer , 1981 .

[22]  L. Wallace.  The structure of the Uranus atmosphere , 1980 .

[23]  U. Fink,et al.  Application of methane band-model parameters to the visible and near-infrared spectrum of Uranus , 1980 .

[24]  I. Shapiro,et al.  The geometric oblateness of Uranus , 1980 .

[25]  W. Smith,et al.  Determination of the H2 4-0 S/1/ quadrupole line strength and pressure shift , 1980 .

[26]  U. Fink,et al.  The infrared spectra of Uranus, Neptune, and Titan from 0.8 to 2.5 microns , 1979 .

[27]  W. Macy.  On the clouds of uranus , 1979 .

[28]  J. Morgan,et al.  Methane band limb-brightening on Uranus , 1979 .

[29]  J. Margolis,et al.  Intensity and pressure shift of the H2 /4,0/ S/1/ quadrupole line. [in giant planet atmospheres] , 1978 .

[30]  Lawrence P. Giver,et al.  Intensity measurements of the CH4 bands in the region 4350 A to 10,600 A , 1978 .

[31]  W. Cochran,et al.  Raman scattering in the atmospheres of the major planets , 1978 .

[32]  R. Goody.  The rotation of Uranus , 1977 .

[33]  U. Fink,et al.  Band model analysis of laboratory methane absorption spectra from 4500 to 10500 A , 1977 .

[34]  R. E. Danielson,et al.  A saturation model of the atmosphere of Uranus , 1977 .

[35]  L. Trafton.  The aerosol distribution in Uranus' atmosphere - Interpretation of the hydrogen spectrum , 1976 .

[36]  L. Lebofsky,et al.  Laboratory reflection spectra for the determination of chemical composition of icy bodies , 1976 .

[37]  E. Richard Cohen,et al.  Theory of line shape in pressure-induced absorption , 1976 .

[38]  A. McKellar.  The significance of pressure shifts for the interpretation of H2 quadrupole lines in planetary spectra , 1974 .

[39]  M. J. Price,et al.  Limb Brightening on Uranus: a Prediction , 1973 .

[40]  L. Wallace.  Rayleigh and Raman Scattering by H_{2} in a Planetary Atmosphere , 1972 .

[41]  A. Mckellar,et al.  Collision-induced spectra of hydrogen in the first and second overtone regions with applications to planetary atmospheres , 1971, Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences.

[42]  M. J. Price,et al.  The Atmosphere of Uranus , 1971 .

[43]  T. C. James.  Calculations of Collision Narrowing of the Quadrupole Lines in Molecular Hydrogen , 1969 .

[44]  G. E. Hunt,et al.  Discrete space theory of radiative transfer I. Fundamentals , 1969, Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences.

[45]  J. Poll,et al.  Quadrupole Transitions in the H2, HD and D2 Molecules , 1969 .

[46]  L. Trafton.  Model atmospheres of the major planets , 1967 .

[47]  L. Galatry,et al.  Simultaneous Effect of Doppler and Foreign Gas Broadening on Spectral Lines , 1961 .

[48]  G. Orton,et al.  New observational constraints on the temperature inversions of Uranus and Neptune , 1983 .

[49]  W. Hubbard,et al.  Internal structure of Uranus , 1982 .

[50]  William H. Smith.  On the ortho-para equilibrium of H2 in the atmospheres of the Jovian planets☆ , 1978 .

[51]  A. Ingersoll,et al.  Pioneer 10 and 11 and ground-based infrared data on Jupiter - The thermal structure and He-H2 ratio , 1976 .

[52]  A. Farkas,et al.  Orthohydrogen, Parahydrogen and Heavy Hydrogen , 1935, Nature.