An analysis of Pluto occultation light curves using an atmospheric radiative–conductive model
- 31 January 2011
- journal article
- Published by Elsevier BV in Icarus
- Vol. 211 (1), 804-818
- https://doi.org/10.1016/j.icarus.2010.08.018
Abstract
No abstract availableKeywords
This publication has 34 references indexed in Scilit:
- Analysis of Stellar Occultation Data. II. Inversion, with Application to Pluto and TritonThe Astronomical Journal, 2003
- The recent expansion of Pluto's atmosphereNature, 2003
- Rovibrational Relaxation of Methane in CH4−N2 Mixtures: Time-Resolved IR−IR Double-Resonance Measurements at 193 K and Kinetic ModelingThe Journal of Physical Chemistry A, 2003
- On the Seasonality of the Hadley CellJournal of the Atmospheric Sciences, 2003
- A Numerical Method for Calculating Stellar Occultation Light Curves from an Arbitrary Atmospheric ModelPublications of the Astronomical Society of the Pacific, 1997
- PROBING PLANETARY ATMOSPHERES WITH STELLAR OCCULTATIONSAnnual Review of Earth and Planetary Sciences, 1996
- Seasonal Nitrogen Cycles on PlutoIcarus, 1996
- Modeling Pluto-Charon Mutual Events. II. CCD Observations With the 60 in. Telescope at Palomar MountainThe Astronomical Journal, 1995
- Analysis of stellar occultation data for planetary atmospheres. I - Model fitting, with application to PlutoThe Astronomical Journal, 1992
- Pluto's atmosphereIcarus, 1989