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@ARTICLE{Funke:22367,
      author       = {Funke, B. and López-Puertas, M. and Garda-Comas, M. and
                      Kaufmann, M. and Stiller, G.P.},
      title        = {{GRANANDA}: {A} {G}eneric {RA}diative tra{N}sfer {A}n{D}
                      non-{LTE} population},
      journal      = {Journal of quantitative spectroscopy $\&$ radiative
                      transfer},
      volume       = {113},
      issn         = {0022-4073},
      address      = {New York, NY [u.a.]},
      publisher    = {Elsevier},
      reportid     = {PreJuSER-22367},
      pages        = {1771 - 1817},
      year         = {2012},
      note         = {We would like to acknowledge the enormous effort of Alain
                      Barbe, Claude Camy-Peiret, and Jean-Marie Flaud for
                      improving and supplying spectroscopic data that are crucial
                      for the non-LIE studies. We give special thanks to
                      Jean-Marie Flaud for providing the spectroscopic data for
                      many of the O<INF>3</INF> and NO<INF>2</INF> hot bands in
                      addition to those in HITRAN2008. We also thank F.J.
                      Martin-Torres for useful advices during the early
                      development of the algorithm, and Miguel A. Lopez-Valverde,
                      Sergio Gil-Lopez, Mariliza Koukouli and Diego
                      Bermejo-Pantaleon for useful comments and suggestions. The
                      IAA team was partially supported by the Spanish MCINN under
                      projects AYA2008-03498/ESP, AYA2011-23552, "ASTROMOL"
                      CSD2009-00038, and EC FEDER funds.},
      abstract     = {We present in this paper the Generic RAdiative traNsfer AnD
                      non-LTE population Algorithm (GRANADA). This model is able
                      to compute non-LIE populations for vibrational, rotational,
                      spin (i.e., NO and OH), and electronic (i.e., O-2) states in
                      a given planetary atmosphere. The model is very flexible and
                      can be used for computing very accurate non-LIE populations
                      or for calculating reasonably accurate but at high speed
                      non-LIE populations in order to implement it into non-LIE
                      remote sensing retrievals. We describe the model in detail
                      and present an update of the non-LIE collisional processes
                      and their rate coefficients for the most important molecules
                      in Earth's atmosphere. In addition, we have applied the
                      model to the most important atmospheric infrared emitters
                      including 13 species (H2O, CO2, O-3, N2O, CO, CH4, O-2, NO,
                      NO2, HNO3, OH, N-2, and HCN) and 460 excited vibrational or
                      electronic energy levels. Non-LIE populations for all these
                      energy levels have been calculated for 48 reference
                      atmospheres expanding from the surface up to 200 km,
                      including seasonal (January, April, July and October),
                      latitudinal (75 degrees S, 45 degrees S, 10 degrees S, 10
                      degrees N, 45 degrees N, 75 degrees N) and diurnal (day and
                      night) coverages. The effects of the most recent updates of
                      the non-LIE collisional parameters on the non-LIE
                      populations are briefly described. This climatology is
                      available online to the community and it can be used for
                      estimating non-LTE effects at specific conditions and for
                      testing and validation studies. (C) 2012 Elsevier Ltd. All
                      rights reserved.},
      keywords     = {J (WoSType)},
      cin          = {IEK-7},
      ddc          = {530},
      cid          = {I:(DE-Juel1)IEK-7-20101013},
      pnm          = {Atmosphäre und Klima},
      pid          = {G:(DE-Juel1)FUEK491},
      shelfmark    = {Spectroscopy},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000306615400004},
      doi          = {10.1016/j.jqsrt.2012.05.001},
      url          = {https://juser.fz-juelich.de/record/22367},
}