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posted on 2020-10-05, 03:41 authored by Hiroaki Matsui, Yangguang Liao, Takumi Kera, Yuto Katoh, Magali I. Billen, Louise KelloggLouise Kellogg
The present study is a parallel in-situ visualization for geodynamo simulations using a open-source dynamo code Calypso. Calypso solves magnetohydrodynamic (MHD) simulations in a rotating shell on a massively parallel computing environment. We develop a parallel volume rendering modules for scalar component and line integral convolution (LIC) modules for vector fields on an unstructured grid, and performed these visualization modules and numerical simulation concurrently.


NSF awards EAR-1550901