The retrieval of cloud structure maps in the equatorial region of Jupiter using a principal component analysis of Galileo/NIMS data

Icarus

Volumn 156, Issue 1, 2002, Pages 52-63

  Irwin, P G J ^a   Dyudina, U ^b  

^a UNIVERSITY OF OXFORD   (United Kingdom)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Atmosphere; Clouds; Image processing; Jupiter

Indexed keywords

EID: 0036261636     PISSN: 00191035     EISSN: None     Source Type: Journal    
DOI: 10.1006/icar.2001.6773     Document Type: Article

References (14)

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2. Spectral detection of ammonia ice in the turbulent clouds of Jupiter by Galileo/NIMS
3. Jupiter's cloud structure from Galileo imaging data
4. Interpretation of NIMS and SSI images on the jovian cloud structure
5. Observation of moist convection in Jupiter's atmosphere
6. Moist convection as an energy source for large-scale motions in Jupiter's atmosphere
7. Cloud structure and atmospheric composition of Jupiter retrieved from Galileo NIMS real-time spectra
8. The origin of belt/zone contrasts in the atmosphere of Jupiter and their correlation with 5-μm opacity
9. Jovian winds from Voyager 2. Part I: Zonal mean circulation
10. Galileo images of lightning on Jupiter
11. Matrix operator theory of radiative transfer. 1: Rayleigh scattering
12. Retrieval of atmospheric temperature and composition from remote sensing measurements of thermal radiation
13. Inverse Methods for Atmospheric Sounding
14. Proximate humid and dry regions in Jupiter's atmosphere indicate complex local meteorology