Uranus' (3-0) H2 quadrupole line profiles
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference35 articles.
1. Radiative-convective equilibrium models of Uranus and Neptune;Appleby;Icarus,1986
2. The structure of the Uranian atmosphere: Constraints from the geometric albedo spectrum and H2 and CH4 line profiles;Baines;Icarus,1986
3. Spatial variability of aerosols in the atmosphere of Uranus;Baines;Bull. Amer. Astron. Soc.,1985
4. H2 pressure-induced lines in the spectra of the major planets;Belton;Astrophys. J.,1973
5. Quadrupole transitions in the H2, HD and D2 molecules;Birnbaum;J. Atmos. Sci.,1969
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5. H2Quadrupole and \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $\mathrm{H}\,^{+}_{3}$ \end{document} Emission from Uranus: The Uranian Thermosphere, Ionosphere, and Aurora;The Astrophysical Journal;1999-10-20
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