ALMA Titan Emission Angles

Published: 17 July 2017| Version 1 | DOI: 10.17632/m5pscpthph.1
Alexander Thelen


Emission angles for radiative transfer modeling (NEMESIS, see Irwin et al., 2008) of ALMA data. Files correspond to retrieved temperature profiles found in 'ALMA Titan Temperature Retrievals' (Thelen et al., 2017). Each file contains emission angles for the matching temperature profile obtained by modeling CO lines from 2012, 2013, 2014, or 2015. Files are denoted by region: disk-averaged (DA) or north (N), center (C), and south (S). Each file contains the radius of each annulus (km), the tangent altitude (x-2575 km) where available (km), the emission angle (deg), and the weighting of that emission angle in the radiative transfer model; weightings add to unity. Thelen et al., 2017.



Radiative Transfer, Planet Atmosphere, Radio Astronomy