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Well-balanced second-order approximation of the compressible atmospheric Euler equations
Abstract
We introduce a second-order approximation to the compressible atmospheric Euler equations with gravity that is invariant domain preserving and well-balanced with respect to stratified rest states, including isentropic and isothermal equilibria. The approximation is built upon discrete auxiliary states derived from a hydrostatic reconstruction of the density and potential temperature. These auxiliary states, together with an affine shift of the numerical state, provide local bounds needed for maintaining well-balancing and invariant domain preserving properties of the method. The numerical method is then verified and validated with analytic solutions, well-balancing tests, and typical benchmark problems for atmospheric flows.
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BibTeX
@misc{farris2026wellbalanced,
title = {{Well-balanced second-order approximation of the compressible atmospheric Euler equations}},
author = {Crystal Farris and Matthias Maier and Eric J. Tovar},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2606.19764},
eprint = {2606.19764},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2606.19764},
}
RIS
TY - UNPB
TI - Well-balanced second-order approximation of the compressible atmospheric Euler equations
AU - Crystal Farris
AU - Matthias Maier
AU - Eric J. Tovar
PY - 2026
DA - 2026/10/31
PB - arXiv
DO - 10.48550/arxiv.2606.19764
UR - https://arxiv.org/abs/2606.19764
AB - We introduce a second-order approximation to the compressible atmospheric Euler equations with gravity that is invariant domain preserving and well-balanced with respect to stratified rest states, including isentropic and isothermal equilibria. The approximation is built upon discrete auxiliary states derived from a hydrostatic reconstruction of the density and potential temperature. These auxiliary states, together with an affine shift of the numerical state, provide local bounds needed for maintaining well-balancing and invariant domain preserving properties of the method. The numerical method is then verified and validated with analytic solutions, well-balancing tests, and typical benchmark problems for atmospheric flows.
ER -