Solid‐state photochemistry as a formation mechanism for Titan's stratospheric C 4 N 2 ice clouds
Author:
Affiliation:
1. NASA Goddard Space Flight Center Greenbelt Maryland USA
2. Department of AstronomyUniversity of Maryland College Park Maryland USA
3. Division of Geological and Planetary SciencesCalifornia Institute of Technology Pasadena California USA
Funder
National Aeronautics and Space Administration
Publisher
American Geophysical Union (AGU)
Subject
General Earth and Planetary Sciences,Geophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016GL067795
Reference29 articles.
1. Titan’s aerosol and stratospheric ice opacities between 18 and 500μm: Vertical and spectral characteristics from Cassini CIRS
2. Particle size and abundance of HC3N ice in Titan’s lower stratosphere at high northern latitudes
3. Subsidence-induced methane clouds in Titan’s winter polar stratosphere and upper troposphere
4. Numerical simulations of the three-dimensional distribution of meteoric dust in the mesosphere and upper stratosphere
5. Numerical simulations of the three-dimensional distribution of polar mesospheric clouds and comparisons with Cloud Imaging and Particle Size (CIPS) experiment and the Solar Occultation For Ice Experiment (SOFIE) observations
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