K H Baines

Summary

Affiliation: NASA Ames Research Center
Country: USA

Publications

  1. ncbi Clouds, hazes, and the stratospheric methane abundance in Neptune
    K H Baines
    Jet Propulsion Laboratory, California Institute of Technology, Pasadena 91109, USA
    Icarus 109:20-39. 1994
  2. ncbi Jupiter cloud composition, stratification, convection, and wave motion: a view from new horizons
    D C Reuter
    NASA Goddard Space Flight Center, Code 693, Greenbelt, MD 20771, USA
    Science 318:223-5. 2007
  3. ncbi Release of volatiles from a possible cryovolcano from near-infrared imaging of Titan
    C Sotin
    Laboratoire de Planétologie et Géodynamique, UMR CNRS 6112, Universite de Nantes, Nantes, 44100, France
    Nature 435:786-9. 2005
  4. ncbi Composition and physical properties of Enceladus' surface
    Robert H Brown
    Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA
    Science 311:1425-8. 2006
  5. ncbi Evidence for a polar ethane cloud on Titan
    C A Griffith
    Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, 85721 USA
    Science 313:1620-2. 2006

Collaborators

Detail Information

Publications5

  1. ncbi Clouds, hazes, and the stratospheric methane abundance in Neptune
    K H Baines
    Jet Propulsion Laboratory, California Institute of Technology, Pasadena 91109, USA
    Icarus 109:20-39. 1994
    ..The factor-of-10 reduction in fCH4,s below that assumed by Pryor et al. implies decreased gas absorption and consequently a decrease in the forward-scattering component of tropospheric aerosols...
  2. ncbi Jupiter cloud composition, stratification, convection, and wave motion: a view from new horizons
    D C Reuter
    NASA Goddard Space Flight Center, Code 693, Greenbelt, MD 20771, USA
    Science 318:223-5. 2007
    ..Both of these phenomena serve as probes of atmospheric dynamics below the visible cloud tops...
  3. ncbi Release of volatiles from a possible cryovolcano from near-infrared imaging of Titan
    C Sotin
    Laboratoire de Planétologie et Géodynamique, UMR CNRS 6112, Universite de Nantes, Nantes, 44100, France
    Nature 435:786-9. 2005
    ..We propose that the structure is a dome formed by upwelling icy plumes that release methane into Titan's atmosphere...
  4. ncbi Composition and physical properties of Enceladus' surface
    Robert H Brown
    Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA
    Science 311:1425-8. 2006
    ..Upper limits of 140 kelvin (for a filled pixel) are derived for the temperatures in the tiger stripes...
  5. ncbi Evidence for a polar ethane cloud on Titan
    C A Griffith
    Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, 85721 USA
    Science 313:1620-2. 2006
    ..Preferential condensation of ethane, perhaps as ice, at Titan's poles during the winters may partially explain the lack of liquid ethane oceans on Titan's surface at middle and lower latitudes...