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Windmiller, Julia Miriam (2017): Organization of tropical convection. Dissertation, LMU München: Fakultät für Physik

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Figure

Fig. 1.1.: Satellite image of the eastern pacific part of the ITCZ which appears as a horizontal bandof bright white clouds just north of the equator
Fig. 1.2.: Snapshots of a shallow cumulus cloud field in an atmospheric model simulation, showing(a) the synthetic cloud albedo and (b) the moisture deviation in the sub-cloud layer (color)and cloud contours (black lines; 0.001 g m−2 and 1.0 g m−2 isolines of liquid water path)(Seifert and Heus, 2013).
Fig. 1.3.: Schematic radar echo of a squall line. A line of deep convective cells with high radarreflectivity, marked by the dark gray or black cells at the leading edge of the squall line,with trailing stratiform precipitation with weaker radar reflectivity, marked by the light grayregion (Houze Jr, 1993).
Fig. 1.8.: Two successive snapshots of temperature perturbations [K] at a height of 50 m in an atmo-spheric model simulation of deep convection performed by Tompkins (2001b)
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Outline

Idealized models of convection Percolation Method Discussion Spatial evolution of self-aggregation in RCE simulations Proposed mechanisms causing self-aggregation Comparison of coarsening and self-aggregation in RCE simulations Conclusion Limitations Understanding Convection

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