Correlation of near-infrared albedo and 5-micron brightness variations in Jupiter's atmosphere

Advances in Space Research

Volumn 29, Issue 2, 2002, Pages 285-290

  Irwin, P G J ^a   Calcutt, S B ^a   Weir, A L ^a   Taylor, F W ^a   Carlson, R W ^b  

^a UNIVERSITY OF OXFORD   (United Kingdom)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

AMMONIA; ATMOSPHERIC STRUCTURE; CLOUDS; OPACITY; SPECTROMETRY;

MICRON BRIGHTNESS;

PLANETARY SURFACE ANALYSIS;

PLANETARY ATMOSPHERE;

EID: 0036160408     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(01)00579-8     Document Type: Article

References (17)

1. Jupiter's cloud structure from Galileo imaging data
2. Study of the deep cloud structure in the equatorial region of Jupiter from Voyager infrared and visible data
3. Retrieval of ammonia abundances and cloud opacities on Jupiter from Voyager IRIS spectra
4. Models of the millimeter-centimeter spectra of the giant planets
5. Jupiter's zone-belt structure at radio wavelengths. II Comparison of observations with model calculations
6. The origin of belt/zone contrasts in the atmosphere of Jupiter and their correlation with 5-micron opacity
7. -1
8. Cloud structure and atmospheric composition of Jupiter retrieved from Galileo NIMS real-time spectra
9. -1 from exponential sum fitting to band-modelled spectra
10. Spectrophotometry of the Jovian planets and Titan at 300 - 1000 nm wavelength: The methane spectrum
11. Study of the ammonia ice cloud layer in the equatorial region of Jupiter from the infrared interferometric experiment on Voyager
12. Matrix operator theory of radiative transfer. 1: Rayleigh scattering
13. -1 for remote sounding of the atmosphere of Jupiter
14. Clouds, aerosols, and photochemistry in the Jovian atmosphere
15. 2 pairs in the first overtone band at temperatures from 20 to 500 K