Article ID Journal Published Year Pages File Type
10701519 Icarus 2012 23 Pages PDF
Abstract
► A new near-IR methane line list incorporates improved measurements at 80 K and 296 K. ► Line-by-line (LBL) outer planet transmission results are compared to band models. ► LBL results agree best with Karkoschka and Tomasko (Karkoschka, E., Tomasko, M. [2010]. Icarus 205, 309-319) model. ► LBL results are in error short of 1.26 μm and where CH3D line data are missing. ► A measured Uranus spectrum is used to define a far wing line shape for the H window.
Keywords
Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Space and Planetary Science
Preview
Comparison of line-by-line and band models of near-IR methane absorption applied to outer planet atmospheres
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