On the water abundance in the atmosphere of Jupiter

[1]  Harold C. Urey,et al.  Abundances of the elements , 1956 .

[2]  JOHN S. Lewis,et al.  Atmospheric and cloud structures of the Jovian planets , 1973 .

[3]  P. Gierasch,et al.  Infrared Observations of the Jovian System from Voyager 1 , 1979, Science.

[4]  T. Encrenaz,et al.  The abundance of water on Jupiter from the voyager IRIS data at 5 μm , 1982 .

[5]  A. Chédin,et al.  The tropospheric gas composition of Jupiter's north equatorial belt /NH3, PH3, CH3D, GeH4, H2O/ and the Jovian D/H isotopic ratio , 1982 .

[6]  D. Raine.  Essays in Nuclear Astrophysics , 1983 .

[7]  Gordon L. Bjoraker,et al.  The abundance and distribution of water vapor in Jupiter's atmosphere , 1986 .

[8]  Sushil K. Atreya,et al.  Book-Review - Atmospheres and Ionospheres of the Outer Planets and Their Satellites , 1986 .

[9]  T. Geballe,et al.  The Origin and Vertical Distribution of Carbon Monoxide in Jupiter , 1988 .

[10]  N. Grevesse,et al.  Abundances of the elements: Meteoritic and solar , 1989 .

[11]  T. Geballe,et al.  The abundance of AsH3 in Jupiter , 1990 .

[12]  W. Smythe,et al.  Near-Infrared Mapping Spectrometer experiment on Galileo , 1992 .

[13]  B. Ragent,et al.  Results of the Galileo Probe Nephelometer Experiment , 1996, Science.

[14]  T. Encrenaz,et al.  First results of ISO-SWS observations of Jupiter , 1996 .

[15]  M. Lemmon,et al.  Solar and Thermal Radiation in Jupiter's Atmosphere: Initial Results of the Galileo Probe Net Flux Radiometer , 1996, Science.

[16]  Frank S. Milos,et al.  Structure of the Atmosphere of Jupiter: Galileo Probe Measurements , 1996, Science.

[17]  M. Roos-Serote.  Spectro-imagerie infrarouge de venus et jupiter : interpretation des observations de nims/galileo , 1997 .

[18]  R. West,et al.  Jupiter's Cloud Structure from Galileo Imaging Data☆ , 1998 .

[19]  T. Encrenaz,et al.  Cloud structure and atmospheric composition of Jupiter retrieved from Galileo near‐infrared mapping spectrometer real‐time spectra , 1998 .

[20]  W. Folkner,et al.  Ammonia abundance in Jupiter's atmosphere derived from the attenuation of the Galileo probe's radio signal , 1998 .

[21]  M. Lemmon,et al.  Galileo probe measurements of thermal and solar radiation fluxes in the Jovian atmosphere , 1998 .

[22]  G. Orton,et al.  The clouds of Jupiter: Results of the Galileo Jupiter Mission Probe Nephelometer Experiment , 1998 .

[23]  G. Orton,et al.  Evolution and persistence of 5‐μm hot spots at the Galileo probe entry latitude , 1998 .

[24]  T. Encrenaz,et al.  Analysis of Jupiter north equatorial belt hot spots in the 4–5 μm range from Galileo/near‐infrared mapping spectrometer observations: Measurements of cloud opacity, water, and ammonia , 1998 .

[25]  D. Hunten,et al.  The composition of the Jovian atmosphere as determined by the Galileo probe mass spectrometer. , 1998, Journal of geophysical research.

[26]  T. Encrenaz,et al.  A comparison of the atmospheres of Jupiter and Saturn: deep atmospheric composition, cloud structure, vertical mixing, and origin. , 1999, Planetary and space science.

[27]  T. Encrenaz,et al.  Constraints on the Tropospheric Cloud Structure of Jupiter from Spectroscopy in the 5-μm Region: A Comparison between Voyager/IRIS, Galileo/NIMS, and ISO/SWS Spectra☆ , 1999 .

[28]  P. Irwin,et al.  The clouds of Jupiter , 1999 .

[29]  G. Orton,et al.  A Dynamical Model of Jupiter's 5-Micron Hot Spots , 1999 .

[30]  Imke de Pater,et al.  A low-temperature origin for the planetesimals that formed Jupiter , 1999, Nature.

[31]  Ashwin R. Vasavada,et al.  Galileo Images of Lightning on Jupiter , 1999 .

[32]  P. Gierasch,et al.  A Detection of Water Ice on Jupiter with Voyager IRIS , 2000 .

[33]  P. Drossart,et al.  Proximate humid and dry regions in Jupiter's atmosphere indicate complex local meteorology , 2000, Nature.

[34]  T. Dowling,et al.  Nonlinear simulations of Jupiter's 5-micron hot spots. , 2000, Science.

[35]  A large age for the pulsar B1757-24 from an upper limit on its proper motion , 2000, Nature.

[36]  Galileo Imaging Team,et al.  Observation of moist convection in Jupiter's atmosphere , 2000, Nature.

[37]  Erratum: Enrichments in Volatiles in Jupiter: A New Interpretation of the Galileo Measurements , 2001 .

[38]  R. Carlson,et al.  The Origin of Belt/Zone Contrasts in the Atmosphere of Jupiter and Their Correlation with 5-μm Opacity , 2001 .

[39]  R. Wimmer–Schweingruber.  Joint SOHO/ACE workshop "Solar and Galactic Composition" , 2001 .

[40]  H. Holweger.  Photospheric Abundances: Problems, Updates, Implications , 2001, astro-ph/0107426.

[41]  S. B. Calcutt,et al.  Atmospheric Composition and Cloud Structure in Jovian 5-μm Hotspots from Analysis of Galileo NIMS Measurements , 2001 .

[42]  J. Lunine,et al.  Enrichments in Volatiles in Jupiter: A New Interpretation of the Galileo Measurements , 2001 .

[43]  K. Baines,et al.  Fresh Ammonia Ice Clouds in Jupiter: I. Spectroscopic Identification, Spatial Distribution, and Dynamical Implications , 2002 .

[44]  Michael H. Wong,et al.  Composition and origin of the atmosphere of Jupiter—an update, and implications for the extrasolar giant planets , 2003 .