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Geophysical Fluid Dynamics Laboratory Princeton, New Jersey Convective Vertical Velocities and Microphysics: Contrasts between 2D and 3D CSRMs Leo Donner.

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Presentation on theme: "Geophysical Fluid Dynamics Laboratory Princeton, New Jersey Convective Vertical Velocities and Microphysics: Contrasts between 2D and 3D CSRMs Leo Donner."— Presentation transcript:

1 Geophysical Fluid Dynamics Laboratory Princeton, New Jersey Convective Vertical Velocities and Microphysics: Contrasts between 2D and 3D CSRMs Leo Donner (GFDL, Princeton University) Vaughan Phillips (Princeton University) GCSS WG4 Broomfield, CO October 2003

2 Geophysical Fluid Dynamics Laboratory Princeton, New Jersey Motivation CSRMs emerging as crucial component of multi-scale modeling framework for AGCMs, aka “superparameterization” 2D CSRMs have been employed in pioneering superparameterization studies Convective vertical velocities increasingly recognized as important for microphysics and radiation interactions

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13 Geophysical Fluid Dynamics Laboratory Princeton, New Jersey 2D

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21 Geophysical Fluid Dynamics Laboratory Princeton, New Jersey 2D > 3D SW Reflection: Microphysical Aspects Less cloud liquid,cloud ice, and snow in 3D More graupel in 3D Behavior holds for GATE, TOGA-COARE, and ARM A Precipitating stratiform fractional area less in 3D in all cases except ARM A 2D(y) Microphysics linked to convective vertical velocities, which differ sharply in 2 and 3D

22 Geophysical Fluid Dynamics Laboratory Princeton, New Jersey 2D > 3D SW Reflection: Dynamic Aspects Cumulus vertical velocities higher in 3D than 2D for GATE, TOGA-COARE, ARM Convective mass flux greater in 3D than 2D for GATE and TOGA-COARE, and, for vertical velocities > 5 m s -1, for ARM A Stratiform mass flux less in melting layer for GATE, ARM, and TOGA-COARE


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