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                <identifier>oai:data.mendeley.com/m5pscpthph.1</identifier>
                <datestamp>2017-07-17T23:18:29Z</datestamp>
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            <metadata><oai_dc:dc xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
    <dc:creator>Thelen, Alexander</dc:creator>
    <dc:title>ALMA Titan Emission Angles</dc:title>
    <dc:publisher>Mendeley Data</dc:publisher>
    <dc:description>Emission angles for radiative transfer modeling (NEMESIS, see Irwin et al., 2008) of ALMA data. Files correspond to retrieved temperature profiles found in &apos;ALMA Titan Temperature Retrievals&apos; (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.</dc:description>
    <dc:subject>Radiative Transfer</dc:subject>
    <dc:subject>Planet Atmosphere</dc:subject>
    <dc:subject>Radio Astronomy</dc:subject>
    <dc:type>Dataset</dc:type>
    <dc:identifier>doi:10.17632/m5pscpthph.1</dc:identifier>
    <dc:identifier>oai:data.mendeley.com/m5pscpthph.1</dc:identifier>
    <dc:rights>Creative Commons Attribution 4.0 International</dc:rights>
    <dc:rights>http://creativecommons.org/licenses/by/4.0</dc:rights>
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    <dc:date>2017-07-17T23:18:29Z</dc:date>
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