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        <title>International Polarized Radiative Transfer intercomparisons</title>
        <description></description>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/</link>
        <image rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/lib/tpl/dokuwiki/images/favicon.ico" />
       <dc:date>2026-05-22T10:43:32+00:00</dc:date>
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                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a1_rayleigh&amp;rev=1426005581&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a2_lambert&amp;rev=1426005695&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a3_aerosol_spherical&amp;rev=1426005756&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a4_aerosol_spheroid&amp;rev=1426005777&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a5_water_cloud&amp;rev=1432039341&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a6_ocean1&amp;rev=1757592789&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:b1_rayleigh&amp;rev=1426007098&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:b2_absorption&amp;rev=1426007242&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:b2_absortpion&amp;rev=1414664071&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:b3_aerosol&amp;rev=1426007301&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:b4_cloud_ocean&amp;rev=1426007319&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:c1_stepcloud&amp;rev=1515414178&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:c2_cubiccloud&amp;rev=1515414164&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:c3_cumulus&amp;rev=1515414216&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d1_rayleigh&amp;rev=1764166576&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d2_lambert&amp;rev=1753136223&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d3_aerosol_spherical&amp;rev=1757939835&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d4_aerosol_spheroid&amp;rev=1771422643&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d5_water_cloud&amp;rev=1753136247&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d6_mixed&amp;rev=1753134423&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d6_ocean&amp;rev=1757924944&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e1_rayleigh&amp;rev=1753136263&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e2_absorption&amp;rev=1753136269&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e3_aerosol&amp;rev=1753136275&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e4_aerosol_stratos&amp;rev=1753136282&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e5_cirrus&amp;rev=1757527439&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e6_ocean_planet&amp;rev=1774026127&amp;do=diff"/>
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                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:intercomparisons&amp;rev=1771233512&amp;do=diff"/>
                <rdf:li rdf:resource="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:scoremip&amp;rev=1414664071&amp;do=diff"/>
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        <title>International Polarized Radiative Transfer</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/</link>
        <url>https://www.meteo.physik.uni-muenchen.de/~iprt/lib/tpl/dokuwiki/images/favicon.ico</url>
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    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a1_rayleigh&amp;rev=1426005581&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2015-03-10T16:39:41+00:00</dc:date>
        <title>intercomparisons:a1_rayleigh</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a1_rayleigh&amp;rev=1426005581&amp;do=diff</link>
        <description>Case A 1: Rayleigh scattering

The most simple setup contains only one layer with scattering (non-absorbing) molecules. The radiance should be calculated for various geometries to check whether polarization is included correctly, in particular for special directions (e.g. solar zenith angle 0° or viewing zenith angle 0°). This test also checks, whether the Rayleigh depolarization factor is correctly included.</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a2_lambert&amp;rev=1426005695&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2015-03-10T16:41:35+00:00</dc:date>
        <title>intercomparisons:a2_lambert</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a2_lambert&amp;rev=1426005695&amp;do=diff</link>
        <description>Case A2: Rayleigh atmosphere with Lambertian surface

Setup:

	*  similar to case A1, with small modifications
	*  surface albedo: 0.3
	*  optical thickness: 0.1
	*  Rayleigh depolarization factor: 0.03
	*  transmittance at bottom and reflectance at top of layer</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a3_aerosol_spherical&amp;rev=1426005756&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2015-03-10T16:42:36+00:00</dc:date>
        <title>intercomparisons:a3_aerosol_spherical</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a3_aerosol_spherical&amp;rev=1426005756&amp;do=diff</link>
        <description>Case A 3: Aerosol - spherical particles

Setup:

	*  typical water soluble aerosol for 50% relative humidity at 500 nm from OPAC database 
	*  aerosol optical thickness: 0.2
	*  aerosol optical properties: [netCDF], [ascii] 
The variable “phase” includes the phase matrix, as a function of the scattering angle (variable</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a4_aerosol_spheroid&amp;rev=1426005777&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2015-03-10T16:42:57+00:00</dc:date>
        <title>intercomparisons:a4_aerosol_spheroid</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a4_aerosol_spheroid&amp;rev=1426005777&amp;do=diff</link>
        <description>Case A 4: Aerosol - spheroidal particles

Setup:

	*  same settings as case A3 but for spheroidal aerosol particles 
	*  aerosol optical thickness: 0.2
	*  aerosol optical properties: [netCDF],[ascii] 
The variable “phase” includes the phase matrix, as a function of the scattering angle (variable</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a5_water_cloud&amp;rev=1432039341&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2015-05-19T12:42:21+00:00</dc:date>
        <title>intercomparisons:a5_water_cloud</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a5_water_cloud&amp;rev=1432039341&amp;do=diff</link>
        <description>Case A 5: Liquid water cloud

The purpose of this test is to check whether the forward scattering peak and features of the phase matrix like the rainbow can be simulated. For this reason simulations in the principal plane and almucanter plane respectively are performed with an angular resolution of 1°.</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a6_ocean1&amp;rev=1757592789&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2025-09-11T12:13:09+00:00</dc:date>
        <title>intercomparisons:a6_ocean1</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:a6_ocean1&amp;rev=1757592789&amp;do=diff</link>
        <description>Case A6: Ocean surface

Setup:

	*  Ocean reflectance matrix by Mishchenko's code ocean.shadow.f (uses anti-clockwise convention for azimuth angle!)
	*  refractive index of water (1.33 + 0i)
	*  wind speed 2m/s
	*  scattering optical thickness (Rayleigh) of layer: 0.1</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:b1_rayleigh&amp;rev=1426007098&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2015-03-10T17:04:58+00:00</dc:date>
        <title>intercomparisons:b1_rayleigh</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:b1_rayleigh&amp;rev=1426007098&amp;do=diff</link>
        <description>Case B 1: Rayleigh scattering, standard atmosphere

In this case it shall be tested whether the coupling between model layers is correctly included.

Setup:

	*  model atmosphere with 30 layers, optical thicknesses provided in . The file includes 2 columns where the first is the altitude of the layer boundaries in km, and the second is the layer optical thickness (e.g. the value for 0 km corresponds to the optical thickness for the layer from 0 to 1 km).</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:b2_absorption&amp;rev=1426007242&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2015-03-10T17:07:22+00:00</dc:date>
        <title>intercomparisons:b2_absorption</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:b2_absorption&amp;rev=1426007242&amp;do=diff</link>
        <description>Case B2: Rayleigh scattering and molecular absorption

This test checks whether molecular absorption is correct. The setup is the same as for case B1 but with molecular absorption and at a different wavelength.

Setup:

	*  model atmosphere with 30 layers, scattering optical thicknesses provided in</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:b2_absortpion&amp;rev=1414664071&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2014-10-30T10:14:31+00:00</dc:date>
        <title>intercomparisons:b2_absortpion</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:b2_absortpion&amp;rev=1414664071&amp;do=diff</link>
        <description>Case B2: Rayleigh scattering and molecular absorption

This test checks whether molecular absorption is correct. The setup is the same as for case B1 but with molecular absorption.

Setup:

	*  model atmosphere with 30 layers, scattering optical thicknesses provided in</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:b3_aerosol&amp;rev=1426007301&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2015-03-10T17:08:21+00:00</dc:date>
        <title>intercomparisons:b3_aerosol</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:b3_aerosol&amp;rev=1426007301&amp;do=diff</link>
        <description>Case B3: Aerosol profile

This test case includes a standard atmosphere with Rayleigh scattering and molecular absorption (as case B2). Aerosol with a specified optical thickness profile is added. The aerosol optical properties are the same as in case A4 (spheroidal particles)</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:b4_cloud_ocean&amp;rev=1426007319&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2015-03-10T17:08:39+00:00</dc:date>
        <title>intercomparisons:b4_cloud_ocean</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:b4_cloud_ocean&amp;rev=1426007319&amp;do=diff</link>
        <description>Case B4: Standard atmosphere with cloud layer and underlying ocean surface

This test case includes a standard atmosphere with Rayleigh scattering (as case B1). A cloud layer and an ocean surface is added.

Setup:

	*  model atmosphere with 30 layers, scattering optical thicknesses provided in</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:c1_stepcloud&amp;rev=1515414178&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2018-01-08T12:22:58+00:00</dc:date>
        <title>intercomparisons:c1_stepcloud</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:c1_stepcloud&amp;rev=1515414178&amp;do=diff</link>
        <description>Case C 1: Step cloud

This test case has been adopted from phase 1 of the I3RC project (see &lt;http://i3rc.gsfc.nasa.gov/input/step_cloud/README.txt&gt;)

Setup:

[Definition of step cloud]

	*  simple 1D step cloud
		*  32 pixels along the x-direction, first 16 have optical depth of 2, remaining have optical thickness of 18.
		*  size of field is set to 0.5 km, i.e. all pixels have a width of 0.5/32 km</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:c2_cubiccloud&amp;rev=1515414164&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2018-01-08T12:22:44+00:00</dc:date>
        <title>intercomparisons:c2_cubiccloud</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:c2_cubiccloud&amp;rev=1515414164&amp;do=diff</link>
        <description>Case C 2: Cubic cloud

Setup:

[Definition of cubic cloud]

	*  simple cubic cloud
		*  domain: 7×7 km in x-y-plane, 5 km in z direction
		*  cubic cloud 1x1x1 km in domain center: x: 3-4km, y: 3-4km, z: 2-3km
		*  70×70 pixels along x-y direction
		*  periodic boundary conditions</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:c3_cumulus&amp;rev=1515414216&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2018-01-08T12:23:36+00:00</dc:date>
        <title>intercomparisons:c3_cumulus</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:c3_cumulus&amp;rev=1515414216&amp;do=diff</link>
        <description>Case C3: Cumulus cloud

Setup:

[Definition of cumulus cloudfield]

	*  Cumulus cloud field from LES model (same as used in I3RC project,  depending on LWC):

   , the format of the ascii file is as follows: 
    Nx Ny Nz flag
    dx dy z1 z2 z3 .... 
    ix iy iz ext Reff
      ...</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d1_rayleigh&amp;rev=1764166576&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2025-11-26T14:16:16+00:00</dc:date>
        <title>intercomparisons:d1_rayleigh</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d1_rayleigh&amp;rev=1764166576&amp;do=diff</link>
        <description>Case D1: Rayleigh scattering

The most simple setup contains only one layer with scattering (non-absorbing) molecules. Radiance shall be calculated for various sun-observer geometries, for twilight conditions and for limb observation geometries. We use the same model setup as for case A1, only change from plane-parallel to spherical geometry.</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d2_lambert&amp;rev=1753136223&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2025-07-21T22:17:03+00:00</dc:date>
        <title>intercomparisons:d2_lambert</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d2_lambert&amp;rev=1753136223&amp;do=diff</link>
        <description>Case D2: Rayleigh scattering layer above Lambertian surface

This case includes the same setup as case D1 but with smaller optical thickness and a Lambertian surface below the Rayleigh scattering layer. 

Setup:

	*  optical thickness of layer: 0.1
	*</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d3_aerosol_spherical&amp;rev=1757939835&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2025-09-15T12:37:15+00:00</dc:date>
        <title>intercomparisons:d3_aerosol_spherical</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d3_aerosol_spherical&amp;rev=1757939835&amp;do=diff</link>
        <description>Case D3: Aerosol layer (spherical)

This case includes the same setup as case D1 but including spherical aerosol particles instead of molecules, the same as in case A3.

Setup:

	*  no molecules
	*  typical water soluble aerosol for 50% relative humidity at 500 nm from OPAC database</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d4_aerosol_spheroid&amp;rev=1771422643&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2026-02-18T13:50:43+00:00</dc:date>
        <title>intercomparisons:d4_aerosol_spheroid</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d4_aerosol_spheroid&amp;rev=1771422643&amp;do=diff</link>
        <description>Case D4: Aerosol layer (spheroid)

This case includes the same setup as case D1 but including spheroidal aerosol particles instead of molecules.

Setup:

	*  no molecules
	*  aerosol optical thickness: 0.2
	*  aerosol optical properties: [netCDF],[ascii] 
The variable</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d5_water_cloud&amp;rev=1753136247&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2025-07-21T22:17:27+00:00</dc:date>
        <title>intercomparisons:d5_water_cloud</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d5_water_cloud&amp;rev=1753136247&amp;do=diff</link>
        <description>Case D5: Liquid water cloud layer

This case includes the same setup as case D1 but including liquid cloud droplets.

Setup:

	*  cloud optical thickness: 5
	*  effective radius: 10 m
	*  cloud optical properties: [netCDF],[ascii] 
The variable “phase” includes the phase matrix, as a function of the scattering angle (variable</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d6_mixed&amp;rev=1753134423&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2025-07-21T21:47:03+00:00</dc:date>
        <title>intercomparisons:d6_mixed</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d6_mixed&amp;rev=1753134423&amp;do=diff</link>
        <description>Case DX: Mixed particle types

This case includes the same setup as case D1 but including a mixture of molecules, spherical and spheroidal aerosol particles. The aerosol optical properties are the same as defined in cases D3 and D4. 

Setup:

	*  Molecular optical thickness: 0.5</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d6_ocean&amp;rev=1757924944&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2025-09-15T08:29:04+00:00</dc:date>
        <title>intercomparisons:d6_ocean</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:d6_ocean&amp;rev=1757924944&amp;do=diff</link>
        <description>Case D6: Ocean surface

This case includes the same setup as case D1 but including an ocean surface (reflectance matrix). 

Setup:

	*  Ocean reflectance matrix by Mishchenko's code ocean.shadow.f (uses anti-clockwise convention for azimuth angle!)
	*  refractive index of water (1.33 + 0i)</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e1_rayleigh&amp;rev=1753136263&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2025-07-21T22:17:43+00:00</dc:date>
        <title>intercomparisons:e1_rayleigh</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e1_rayleigh&amp;rev=1753136263&amp;do=diff</link>
        <description>Case E1: Rayleigh scattering, US standard atmosphere

In this case we include the US standard atmosphere, the corresponding Rayleigh scattering optical thickness profile is provided for 450nm. 

Setup:

	*  model atmosphere US-standard, scattering optical thickness provided in file</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e2_absorption&amp;rev=1753136269&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2025-07-21T22:17:49+00:00</dc:date>
        <title>intercomparisons:e2_absorption</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e2_absorption&amp;rev=1753136269&amp;do=diff</link>
        <description>Case E2: Rayleigh scattering and absorption, US standard atmosphere

In this case we include the US standard atmosphere, the corresponding Rayleigh scattering optical thickness and molecular absorption profiles are provided at 320nm. 

Setup:

	*  model atmosphere US-standard, scattering optical thickness provided in file</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e3_aerosol&amp;rev=1753136275&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2025-07-21T22:17:55+00:00</dc:date>
        <title>intercomparisons:e3_aerosol</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e3_aerosol&amp;rev=1753136275&amp;do=diff</link>
        <description>Case E3: US standard atmosphere and tropospheric aerosol layer

In this case we include the US standard atmosphere, the corresponding Rayleigh scattering optical thickness and molecular absorption profiles are provided at 450 nm.
In addition an aerosol layer is added between 0 and 3km altitude.</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e4_aerosol_stratos&amp;rev=1753136282&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2025-07-21T22:18:02+00:00</dc:date>
        <title>intercomparisons:e4_aerosol_stratos</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e4_aerosol_stratos&amp;rev=1753136282&amp;do=diff</link>
        <description>Case E4: US standard atmosphere and two aerosol layers

In this case we include the US standard atmosphere, the corresponding Rayleigh scattering optical thickness and molecular absorption profiles are provided at 450 nm.
In addition two aerosol layers are added: desert dust in the troposphere and sulfate in the stratosphere.</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e5_cirrus&amp;rev=1757527439&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2025-09-10T18:03:59+00:00</dc:date>
        <title>intercomparisons:e5_cirrus</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e5_cirrus&amp;rev=1757527439&amp;do=diff</link>
        <description>Case E5: US standard atmosphere and cirrus cloud

In this case we include the US standard atmosphere, the corresponding Rayleigh scattering optical thickness and molecular absorption profiles are provided at 450 nm.
In addition we include a cirrus cloud layer.</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e6_ocean_planet&amp;rev=1774026127&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2026-03-20T17:02:07+00:00</dc:date>
        <title>intercomparisons:e6_ocean_planet</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:e6_ocean_planet&amp;rev=1774026127&amp;do=diff</link>
        <description>Case E6: Planet with US standard atmosphere and ocean surface

In this case we include the US standard atmosphere, the corresponding Rayleigh scattering optical thickness and molecular absorption profiles are provided at 450 nm.
Below we add a water surface described by a bidirectional reflectance distribution function including the specular reflection.</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:intercomparison_studies&amp;rev=1414664071&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2014-10-30T10:14:31+00:00</dc:date>
        <title>intercomparisons:intercomparison_studies</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:intercomparison_studies&amp;rev=1414664071&amp;do=diff</link>
        <description>Line-by-line calculations (GOSAT spectra)

This intercomparison is part of the SWIR Carbon Observation Retrieval
Model Intercomparison Project (SCORE-MIP). The objectives of SCOREMIP
are to intercompare radiative transfer codes and retrieval methods used
for</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:intercomparisons&amp;rev=1771233512&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2026-02-16T09:18:32+00:00</dc:date>
        <title>intercomparisons:intercomparisons</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:intercomparisons&amp;rev=1771233512&amp;do=diff</link>
        <description>IPRT polarized radiative transfer model intercomparison

General conventions:

	*  For all cases normalized radiances are compared (i.e. Stokes vector components devided by the extraterrestrial irradiance). 
	*  The viewing azimuth angle is defined clockwise</description>
    </item>
    <item rdf:about="https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:scoremip&amp;rev=1414664071&amp;do=diff">
        <dc:format>text/html</dc:format>
        <dc:date>2014-10-30T10:14:31+00:00</dc:date>
        <title>intercomparisons:scoremip</title>
        <link>https://www.meteo.physik.uni-muenchen.de/~iprt/doku.php?id=intercomparisons:scoremip&amp;rev=1414664071&amp;do=diff</link>
        <description>SWIR Carbon Observation Retrieval Model Intercomparison Project (SCORE-MIP)

Hartmut Boesch, Andre Butz, Yukio Yoshida, and Claudia Emde

Comparison of scalar and vector radiative transfer codes

Objective: Radiative transfer intercomparisons of scalar and
vector RT codes for synchronized layer properties for the SWIR
spectral range.</description>
    </item>
</rdf:RDF>
