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Title: A Low Mach Number Model for Moist Atmospheric Flows

Journal Article · · Journal of the Atmospheric Sciences
 [1];  [1];  [1]
  1. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Center for Computational Sciences and Engineering

A low Mach number model for moist atmospheric flows is introduced that accurately incorporates reversible moist processes in flows whose features of interest occur on advective rather than acoustic time scales. Total water is used as a prognostic variable, so that water vapor and liquid water are diagnostically recovered as needed from an exact Clausius–Clapeyron formula for moist thermodynamics. Low Mach number models can be computationally more efficient than a fully compressible model, but the low Mach number formulation introduces additional mathematical and computational complexity because of the divergence constraint imposed on the velocity field. Here in this paper, latent heat release is accounted for in the source term of the constraint by estimating the rate of phase change based on the time variation of saturated water vapor subject to the thermodynamic equilibrium constraint. Finally, the authors numerically assess the validity of the low Mach number approximation for moist atmospheric flows by contrasting the low Mach number solution to reference solutions computed with a fully compressible formulation for a variety of test problems.

Research Organization:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR)
Grant/Contract Number:
AC02-05CH11231
OSTI ID:
1407268
Journal Information:
Journal of the Atmospheric Sciences, Vol. 72, Issue 4; ISSN 0022-4928
Publisher:
American Meteorological SocietyCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 8 works
Citation information provided by
Web of Science

References (13)

Low Mach Number Modeling of Type Ia Supernovae. I. Hydrodynamics journal February 2006
Low Mach Number Modeling of Type Ia Supernovae. II. Energy Evolution journal October 2006
Low Mach Number Modeling of Type Ia Supernovae. III. Reactions journal September 2008
Low Mach Number Modeling of Stratified Flows book January 2014
The conditions for dynamical similarity of motions of a frictionless perfect-gas atmosphere journal April 1953
Non-precipitating cumulus convection and its parameterization journal January 1973
Asymptotics, structure, and integration of sound-proof atmospheric flow equations journal May 2009
Conservative Split-Explicit Time Integration Methods for the Compressible Nonhydrostatic Equations journal August 2007
Maestro: an Adaptive low mach Number Hydrodynamics Algorithm for Stellar Flows journal May 2010
A moist pseudo-incompressible model journal June 2014
The Dry-Entropy Budget of a Moist Atmosphere journal December 2008
A non-hydrostatic mesoscale model: A NON-HYDROSTATIC MESOSCALE MODEL journal April 1976
Energy Conservation and Gravity Waves in Sound-Proof Treatments of Stellar Interiors. ii. Lagrangian Constrained Analysis journal August 2013

Cited By (3)

MAESTROeX: A Massively Parallel Low Mach Number Astrophysical Solver journal December 2019
A review on regional convection‐permitting climate modeling: Demonstrations, prospects, and challenges text January 2015
MAESTROeX: A Massively Parallel Low Mach Number Astrophysical Solver text January 2019

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