Longitudinal variability of methane and ammonia bands on Jupiter

[1]  D. Deming,et al.  Heterodyne Observations of 12mum Emission from the Jovian South Polar Region. , 1981 .

[2]  R. Cess,et al.  A Saturnian stratospheric seasonal climate model , 1979 .

[3]  Bradford A. Smith,et al.  The Jupiter System Through the Eyes of Voyager 1 , 1979, Science.

[4]  J. Hansen,et al.  Jupiter's Atmospheric Composition and Cloud Structure Deduced from Absorption Bands in Reflected Sunlight , 1978 .

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

[6]  L. Trafton.  Saturn: Long-term variation of H2 and CH4 absorptions , 1977 .

[7]  J. Bergstralh,et al.  Interpretation of spatial and temporal variations of hydrogen quadrupole absorptions in the Jovian atmosphere observed during the 1972 apparition , 1977 .

[8]  J. Westphal,et al.  The vertical cloud structure of Jupiter from 5 μm measurements , 1977 .

[9]  William H. Smith,et al.  Spatially resolved spectroscopy of Jupiter. I - H2 quadrupole 4-0 S/1/ line , 1976 .

[10]  J. Bergstralh,et al.  Structure of the visible Jovian clouds , 1974, Nature.

[11]  J. Bergstralh.  An Observational Test of Absorption Line Formation Models in the Jovian Atmosphere . , 1972 .

[12]  Larry A. Lebofsky,et al.  Lunar spectral types. , 1971 .

[13]  R. N. Griffin,et al.  Determination of extraterrestrial solar spectral irradiance from a research aircraft. , 1969, Applied optics.

[14]  T. Owen,et al.  The visible bands of ammonia - Band strengths, curves of growth, and the spatial distribution of ammonia on Jupiter , 1980 .

[15]  R. A. Stokes,et al.  Variation of Jupiter's CH4 and NH3 bands with position on the planetary disk , 1974 .

[16]  J. Bergstralh,et al.  ANALYSIS OF SPECTROSCOPIC OBSERVATIONS OF JUPITER AND THE VARIABILITY OF THE STRUCTURE OF THE VISIBLE CLOUDS , 1974 .