Molecular nitrogen and methane density retrievals from Cassini UVIS dayglow observations of Titan’s upper atmosphere
- 1 February 2015
- journal article
- Published by Elsevier BV in Icarus
- Vol. 247, 301-312
- https://doi.org/10.1016/j.icarus.2014.10.008
Abstract
No abstract availableKeywords
Funding Information
- National Aeronautics and Space Administration (13AV62I)
This publication has 48 references indexed in Scilit:
- The mesosphere and lower thermosphere of Titan revealed by Cassini/UVIS stellar occultationsIcarus, 2011
- Titan airglow spectra from Cassini Ultraviolet Imaging Spectrograph (UVIS): EUV analysisGeophysical Research Letters, 2007
- POAM III retrieval algorithm and error analysisJournal of Geophysical Research: Atmospheres, 2002
- The EUV airglow of Titan: Production and loss ofJournal of Geophysical Research, 2001
- A new reference spectrum for the EUV irradiance of the quiet Sun: 2. Comparisons with observations and previous modelsJournal of Geophysical Research, 1998
- POAM II retrieval algorithm and error analysisPublished by American Geophysical Union (AGU) ,1997
- Analytical representation of g factors for rapid, accurate calculation of excitation rates in the dayside thermosphereJournal of Geophysical Research, 1997
- EUVAC: A solar EUV Flux Model for aeronomic calculationsJournal of Geophysical Research, 1994
- Ultraviolet spectroscopy and remote sensing of the upper atmosphereSpace Science Reviews, 1991
- Observational, reference and model data on solar EUV, from measurements on AE‐EGeophysical Research Letters, 1981