Comparison of cloud models for Brown Dwarfs

@inproceedings{ChHelling2007ComparisonOC,
  title={Comparison of cloud models for Brown Dwarfs},
  author={Ch.Helling and A.Ackerman and F.Allard and M.Dehn and P.Hauschildt and D.Homeier and K.Lodders and M.Marley and F.Rietmeijer and T.Tsuji and P.Woitke},
  year={2007}
}
  • Ch.Helling, A.Ackerman, +8 authors P.Woitke
  • Published 2007
  • Physics
  • A test case comparison is presented for different dust cloud model approaches applied in brown dwarfs and giant gas planets. We aim to achieve more transparency in evaluating the uncertainty inherent to theoretical modelling. We show in how far model results for characteristic dust quantities vary due to different assumptions. We also demonstrate differences in the spectral energy distributions resulting from our individual cloud modelling in 1D substellar atmosphere simulations. 

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