K H Baines
Affiliation: NASA Ames Research Center
- Clouds, hazes, and the stratospheric methane abundance in NeptuneK 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...
- Jupiter cloud composition, stratification, convection, and wave motion: a view from new horizonsD 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...
- Release of volatiles from a possible cryovolcano from near-infrared imaging of TitanC 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...
- Composition and physical properties of Enceladus' surfaceRobert 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...
- Evidence for a polar ethane cloud on TitanC 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...