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Organisation of potential vorticity on the mesoscale during deep moist convection
Author(s) -
Chris Weijenborg,
Petra Friederichs,
Andreas Hense
Publication year - 2015
Publication title -
tellus. series a, dynamic meteorology and oceanography
Language(s) - English
Resource type - Journals
eISSN - 1600-0870
pISSN - 0280-6495
DOI - 10.3402/tellusa.v67.25705
Subject(s) - mesoscale meteorology , potential vorticity , wind shear , geology , atmospheric sciences , convection , vorticity , storm , meteorology , hydrostatic equilibrium , severe weather , climatology , environmental science , wind speed , vortex , physics , quantum mechanics
Potential vorticity (PV) and its conservation principle elegantly describe large-scale atmospheric dynamics. On the mesoscale, however, PV has received less attention. We describe the characteristics of PV on the convective weather scale (≈10 km) as simulated by the non-hydrostatic numerical weather prediction model COSMO-DE. Two weather cases with a different synoptic background are analysed, on 5 June 2011 and 22 June 2011. Composites of PV and other quantities like wind velocity around storm updrafts are calculated to test consistency of PV anomalies associated with storm updrafts.For the frontal case on 22 June bands of positive and negative PV form approximately along the direction of the wind shear. A possible explanation of these elongated PV bands is the preferential generation of new cells downshear of old cells in an atmosphere with moderate to high vertical wind shear. The PV dipoles are much less consistent in direction in the 5 June case with localised deep convection. For both cases, the wind anomalies around the convective PV anomalies are consistent with the flow around synoptic PV anomalies. The coherent PV anomalies around storm updrafts motivate the use of PV-thinking on smaller scales

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