TY - JOUR
T1 - The influence of terrain on the convective environment and associated convective morphology from an idealized modeling perspective
AU - Mulholland, Jake P.
AU - Nesbitt, Stephen W.
AU - Trapp, Robert J.
AU - Peters, John M.
N1 - Funding Information:
Acknowledgments. We are indebted to George Bryan for his creation, development, and support of CM1. The authors thank the Servicio Meteorológico Nacional, Argentina, for their efforts during RELAMPAGO. J. Mulholland would like to thank Chuan-Chieh Chang, Geoffrey Marion, Benjamin Vega-Westhoff, Tzu-shun Lin, Itinderjot Singh, and Kevin Gray for computing assistance and Robert Rauber, Deanna Hence, Hugh Morrison, Christopher Nowotarski, Jana Houser, Bowen Pan, Bruno Ribeiro, Johana Lambert, and Janice Mulholland for many thought-provoking and fruitful discussions. The authors thank the main editor, Louis Wicker, and three anonymous reviewers for their constructive reviews that greatly improved the manuscript. Computational resources were provided by the Computational and Information Systems Lab at the National Center for Atmospheric Research and the University of Illinois at Urbana–Champaign Keeling supercomputing cluster. Support for this work was made possible by National Science Foundation (NSF) Grants AGS-1661799 for J. Mulholland and S. Nesbitt and AGS-1661800 for R. Trapp. J. Peters efforts were supported by NSF Grants AGS-1928666 and partially supported by NSF Grants AGS-1841674 and Department of Energy Atmospheric System Research (DOE ASR) Grant DE-SC0000246356.
Publisher Copyright:
© 2020 American Meteorological Society. For information regarding reuse of this content and general copyright information, consult the AMS Copyright Policy (www.ametsoc.org/PUBSReuseLicenses).
PY - 2020
Y1 - 2020
N2 - Orographic deep convection (DC) initiation and rapid evolution from supercells to mesoscale convective systems (MCSs) are common near the Sierras de Córdoba, Argentina, which was the focal point of the Remote Sensing of Electrification, Lightning, and Mesoscale/Microscale Processes with Adaptive Ground Observations (RELAMPAGO) field campaign. This study used an idealized numerical model with elongated north-south terrain similar to that of the Sierras de Córdoba to address how variations in terrain height affected the environment and convective morphology. Simulations used a thermodynamic profile from a RELAMPAGO event that featured both supercell and MCS storm modes. Results revealed that DC initiated earlier in simulations with higher terrain, owing both to stronger upslope flows and standing mountain waves. All simulations resulted in supercell formation, with higher-terrain supercells initiating closer to the terrain peak and moving slower off the terrain. Higher-terrain simulations displayed increases in both low-level and deep-layer wind shear along the eastern slopes of the terrain that were related to the enhanced upslope flows, supporting stronger and wider supercell updrafts/downdrafts and a wider swath of heavy rainfall. Deeper and stronger cold pools from these wider and stronger higher-terrain supercells led to surging outflow that reduced convective available potential energy accessible to deep convective updrafts, resulting in quicker supercell demise off the terrain. Lower-terrain supercells moved quickly off the terrain, merged with weaker convective cells, and resulted in a quasi-organized MCS. These results demonstrate that terrain-induced flow modification may lead to substantial local variations in convective morphology.
AB - Orographic deep convection (DC) initiation and rapid evolution from supercells to mesoscale convective systems (MCSs) are common near the Sierras de Córdoba, Argentina, which was the focal point of the Remote Sensing of Electrification, Lightning, and Mesoscale/Microscale Processes with Adaptive Ground Observations (RELAMPAGO) field campaign. This study used an idealized numerical model with elongated north-south terrain similar to that of the Sierras de Córdoba to address how variations in terrain height affected the environment and convective morphology. Simulations used a thermodynamic profile from a RELAMPAGO event that featured both supercell and MCS storm modes. Results revealed that DC initiated earlier in simulations with higher terrain, owing both to stronger upslope flows and standing mountain waves. All simulations resulted in supercell formation, with higher-terrain supercells initiating closer to the terrain peak and moving slower off the terrain. Higher-terrain simulations displayed increases in both low-level and deep-layer wind shear along the eastern slopes of the terrain that were related to the enhanced upslope flows, supporting stronger and wider supercell updrafts/downdrafts and a wider swath of heavy rainfall. Deeper and stronger cold pools from these wider and stronger higher-terrain supercells led to surging outflow that reduced convective available potential energy accessible to deep convective updrafts, resulting in quicker supercell demise off the terrain. Lower-terrain supercells moved quickly off the terrain, merged with weaker convective cells, and resulted in a quasi-organized MCS. These results demonstrate that terrain-induced flow modification may lead to substantial local variations in convective morphology.
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U2 - 10.1175/JAS-D-19-0190.1
DO - 10.1175/JAS-D-19-0190.1
M3 - Article
AN - SCOPUS:85091169394
SN - 0022-4928
VL - 77
SP - 3929
EP - 3949
JO - Journal of the Atmospheric Sciences
JF - Journal of the Atmospheric Sciences
IS - 11
ER -