Accurate and efficient Jones-Worland spectral transforms for planetary applications


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Date

2021-07

Publication Type

Conference Paper

ETH Bibliography

yes

Citations

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Data

Abstract

Spectral transforms between physical space and spectral space are needed for fluid dynamical calculations in the whole sphere, representative of a planetary core. In order to construct a representation that is everywhere smooth, regular and differentiable, special polynomials called Jones-Worland polynomials, based on a type of Jacobi polynomial, are used for the radial expansion, coupled to spherical harmonics in angular variables. We present an exact, efficient transform that is partly based on the FFT and which remains accurate in finite precision. Application is to high-resolution solutions of the Navier-Stokes equation, possibly coupled to the heat transfer and induction equations. Expected implementations would be in simulations with P3 degrees of freedom, where P may be greater than 103. Memory use remains modest at high spatial resolution, indeed typically P times lower than competing algorithms based on quadrature.

Publication status

published

Editor

Book title

PASC '21: Proceedings of the Platform for Advanced Scientific Computing Conference

Journal / series

Volume

Pages / Article No.

16

Publisher

Association for Computing Machinery

Event

Platform for Advanced Scientific Computing Conference (PASC 2021)

Edition / version

Methods

Software

Geographic location

Date collected

Date created

Subject

Spectral method; Computational fluid dynamics; HPC

Organisational unit

03734 - Jackson, Andrew / Jackson, Andrew check_circle

Notes

Funding

833848 - Unravelling Earth’s magnetic history and processes UEMHP (EC)
165641 - Understanding planetary magnetic fields from theoretical, numerical and analogue models (SNF)

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