@prefix ns0: <https://gcmd.earthdata.nasa.gov/kms#> .
@prefix skos: <http://www.w3.org/2004/02/skos/core#> .

<https://gcmd.earthdata.nasa.gov/kms/concept/8c25b822-ad70-4e0f-b453-97fe5a80ae1f>
  ns0:altLabel [ ] ;
  skos:broader <https://gcmd.earthdata.nasa.gov/kms/concept/af0968ce-ffe3-44a0-86de-2ec9b9a8fa5d> ;
  skos:prefLabel "ICRCCM"@en ;
  skos:inScheme <https://gcmd.earthdata.nasa.gov/kms/concepts/concept_scheme/projects> ;
  skos:definition """The fourth intercomparison is actually one of the earliest
      conducted by DOE. ICRCCM is a program co-sponsored by DOE, the
      World Meteorological Organization (WMO), and the International
      Radiation Commission (IRC). The late Fred Luther gave the best
      description of the rationale for the program: "Since the
      transfer of solar and longwave radiation is the prime physical
      process that drives the circulation of the atmosphere and its
      temperature structure, it is natural that an evaluation of the
      modeling of physical processes important to climate begin with
      radiation." (Luther 1984)

      Principal Findings:

1. Line-by-line models are in good agreement with each other to within
   a few W/m2 (usually within 1%) when arbitrary line width cutoffs
   are universally applied. The ICRCCM concluded that: "Uncertainties
   in the physics of line wings and in the proper treatment of the
   continuum make it impossible for line-by-line models to provide an
   absolute reference . . ." (Luther et al. 1988). Thus, no
   present-day model furnishes a reliable standard by which to judge
   other models, nor are appropriate data available.

2. There is no systematic difference between wide-band and narrow-band
   model results. However, there is a large variation among the band
   models. While average differences from line-by-line results range
   from 5 to 10%, the spread among the band models is several times
   larger.

3. Band model calculations of sensitivities to changes in absorbing
   constituents show poorer agreement with line-by-line results, and a
   much larger spread, than calculations of flux components. For
   example, when is doubled, the median band model sensitivities
   differ by up to 18% from line-by-line values, while their spread is
   an order of magnitude larger.

4. In cases of only and only, the spread in results among band models
   increases considerably compared to the case when all absorbing
   gases are included; this indicates that the success in the latter
   case is partly fortuitous because of the way absorbing bands
   overlap in the Earth's atmosphere.

5. For the longwave clear cases, with about 40 participants
   representing almost all the world's major modeling groups, ICRCCM
   revealed intermodel disagreements in fluxes and flux sensitivity to
   constituent changes ranging from 30 to 70% (Luther et
   al. 1988). The disagreements are worst for single absorbing gas
   atmospheres, indicating that the better agreement found in the
   all-gas cases is partly accidental. Subsequent ICRCCM calculations,
   involving cloudy longwave cases, and clear and cloudy shortwave
   cases, have revealed equally large or larger disagreements, ranging
   up to 20 to 30% in fluxes and up to 70% in flux sensitivity to
   constituent changes.

6. Comparisons are still in progress for vertical profiles of
   radiative heating rates. Disagreements in radiative heating rates
   are expected to be larger than for fluxes, because heating rate is
   the derivative of flux and taking derivatives magnifies errors

      For more information, link to
"http://www.arm.gov/docs/documents/project/er_0441/bkground_5/radcompar_9.html\""""@en ;
  a skos:Concept .

<https://gcmd.earthdata.nasa.gov/kms/concept/af0968ce-ffe3-44a0-86de-2ec9b9a8fa5d>
  skos:prefLabel "G - I"@en ;
  a skos:Concept ;
  skos:narrower <https://gcmd.earthdata.nasa.gov/kms/concept/8c25b822-ad70-4e0f-b453-97fe5a80ae1f> .

