Journal cover Journal topic
Atmospheric Chemistry and Physics An interactive open-access journal of the European Geosciences Union
doi:10.5194/acp-2017-51
© Author(s) 2017. This work is distributed
under the Creative Commons Attribution 3.0 License.
Research article
07 Feb 2017
Review status
This discussion paper is under review for the journal Atmospheric Chemistry and Physics (ACP).
Scale dependence of cirrus heterogeneity effects. Part I: MODIS thermal infrared channels
Thomas Fauchez1,2, Steven Platnick2, Kerry Meyer3,2, Céline Cornet4, Frédéric Szczap5, and Tamás Várnai6,2 1Universities Space Research Association (USRA), Columbia, MD, USA
2NASA Goddard Space Flight Center, Greenbelt, MD, USA
3Goddard Earth Sciences Technology and Research, Universities Space Research Association, Columbia, MD, USA
4Laboratoire d'Optique Atmosphèrique, UMR 8518, Université Lille 1, Villeneuve d'Ascq, France
5Laboratoire de Météorologie Physique, UMR 6016, Université Blaise Pascal, Clermont Ferrand, France
6University of Maryland Baltimore County: Joint Center for Earth Systems Technology and the Department of Physics, Baltimore, MD, USA
Abstract. This paper presents a study on the impact of cirrus cloud heterogeneities on MODIS simulated thermal infrared (TIR) brightness temperatures (BT) at the top of the atmosphere (TOA) as a function of spatial resolution from 50 m to 10 km. A realistic 3-D cirrus field is generated by the 3DCLOUD model, and 3-D thermal infrared radiative transfer (RT) is simulated with the 3DMCPOL code. According to previous studies, differences between 3-D BT computed from a heterogeneous pixel and 1-D RT computed from a homogeneous pixel are considered dependent, at nadir, on two effects: (i) the optical thickness horizontal heterogeneity leading to the homogeneous plane parallel bias (PPHB) and the (ii) horizontal radiative transport (HRT) leading to the independent pixel approximation error (IPAE). A unique but realistic cirrus case is simulated and, as expected, the PPHB impacts mainly the low spatial resolution results (above 250 m) with averaged values up to 5–7 K while the IPAE impacts mainly the high spatial resolution results (below 250 m) with average values up to 1–2 K. A sensitivity study has been performed in order to extend these results to various cirrus optical thicknesses and heterogeneities by sampling the cirrus in several ranges of parameters. For four optical thickness classes and four optical heterogeneity classes, we have found that, for nadir observations, the spatial resolution where the combination of PPHB and HRT effects is the smallest, falls between 100 m and 250 m. These spatial resolutions appear thus to be the best choice to retrieve cirrus optical properties with the smallest cloud heterogeneity related total bias in the thermal infrared. For off-nadir observations, the average total effect is increased and the minimum is shifted to coarser spatial resolutions.

Citation: Fauchez, T., Platnick, S., Meyer, K., Cornet, C., Szczap, F., and Várnai, T.: Scale dependence of cirrus heterogeneity effects. Part I: MODIS thermal infrared channels, Atmos. Chem. Phys. Discuss., doi:10.5194/acp-2017-51, in review, 2017.
Thomas Fauchez et al.
Thomas Fauchez et al.
Thomas Fauchez et al.

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This paper presents a study on the impact of cirrus cloud horizontal heterogeneity on simulated thermal infrared brightness temperatures at the top of the atmosphere for spatial resolutions ranging from 50 m to 10 km. The cirrus is generated by the 3DCLOUD code and the radiative transfer by the 3DMCPOL code. Brightness temperatures are mostly impacted by the horizontal transport effect and plane parallel bias at high and coarse spatial resolutions, respectively, with a minimum around 100 m–250 m.
This paper presents a study on the impact of cirrus cloud horizontal heterogeneity on simulated...
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