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DCMIP2016: The tropical cyclone test case

  • Justin L. Willson
  • , Kevin A. Reed
  • , Christiane Jablonowski
  • , James Kent
  • , Peter H. Lauritzen
  • , Ramachandran Nair
  • , Mark A. Taylor
  • , Paul A. Ullrich
  • , Colin M. Zarzycki
  • , David M. Hall
  • , Don Dazlich
  • , Ross Heikes
  • , Celal Konor
  • , David Randall
  • , Thomas Dubos
  • , Yann Meurdesoif
  • , Xi Chen
  • , Lucas Harris
  • , Christian Kühnlein
  • , Vivian Lee
  • Abdessamad Qaddouri, Claude Girard, Marco Giorgetta, Daniel Reinert, Hiroaki Miura, Tomoki Ohno, Ryuji Yoshida
  • Stony Brook University
  • University of Michigan, Ann Arbor
  • University of South Wales
  • Met Office
  • Sandia National Laboratories, New Mexico
  • University of California at Davis
  • Pennsylvania State University
  • University of Colorado Boulder
  • NVIDIA
  • Colorado State University
  • Ecole Polytechnique
  • National Oceanic and Atmospheric Administration
  • CAS - Institute of Atmospheric Physics
  • European Centre for Medium-Range Weather Forecasts
  • Université Laval and Environment and Climate Change Canada
  • Max Planck Institute for Meteorology
  • Deutscher Wetterdienst
  • The University of Tokyo
  • Yokohama National University

Research output: Contribution to journalArticlepeer-review

2 Scopus citations

Abstract

This paper describes and analyzes the Reed-Jablonowski (RJ) tropical cyclone (TC) test case used in the 2016 Dynamical Core Model Intercomparison Project (DCMIP2016). This intermediate-complexity test case analyzes the evolution of a weak vortex into a TC in an idealized tropical environment. Reference solutions from nine general circulation models (GCMs) with identical simplified physics parameterization packages that participated in DCMIP2016 are analyzed in this study at 50gkm horizontal grid spacing, with five of these models also providing solutions at 25gkm grid spacing. Evolution of minimum surface pressure (MSP) and maximum 1gkm azimuthally averaged wind speed (MWS), the wind-pressure relationship, radial profiles of wind speed and surface pressure, and wind composites are presented for all participating GCMs at both horizontal grid spacings. While all TCs undergo a similar evolution process, some reach significantly higher intensities than others, ultimately impacting their horizontal and vertical structures. TCs simulated at 25gkm grid spacings retain these differences but reach higher intensities and are more compact than their 50gkm counterparts. These results indicate that dynamical core choice is an essential factor in GCM development, and future work should be conducted to explore how specific differences within the dynamical core affect TC behavior in GCMs.

Original languageEnglish
Pages (from-to)2493-2507
Number of pages15
JournalGeoscientific Model Development
Volume17
Issue number7
DOIs
StatePublished - Apr 3 2024

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