TL;DR
This paper introduces a high-order numerical method combining space-time tensor formalism, flux reconstruction, and exponential integration to efficiently solve the shallow-water equations on a rotated cubed-sphere grid, enabling larger time steps and improved accuracy.
Contribution
It develops new multistep exponential propagation methods of orders 4, 5, and 6 for high-order time integration of shallow-water equations on the sphere.
Findings
Methods achieve high-order accuracy in time.
Significantly larger time steps are possible.
Validated with standard benchmark tests.
Abstract
A novel numerical approach to solving the shallow-water equations on the sphere using high-order numerical discretizations in both space and time is proposed. A space-time tensor formalism is used to express the equations of motion covariantly and to describe the geometry of the rotated cubed-sphere grid. The spatial discretization is done with the direct flux reconstruction method, which is an alternative formulation to the discontinuous Galerkin approach. The equations of motion are solved in differential form and the resulting discretization is free from quadrature rules. It is well known that the time step of traditional explicit methods is limited by the phase velocity of the fastest waves. Exponential integration is employed to enable integrations with significantly larger time step sizes and improve the efficiency of the overall time integration. New multistep-type exponential…
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