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BATS-R-US (Block-Adaptive-Tree Solarwind Roe Upwind Scheme)

Product or Programme · All products and programmes
Evidence · 3 claims (3 for) · 1 study (1 design), q2 · 0 of 1 report an effect size · 3 claims rest on one study

Description

A three-dimensional global magnetohydrodynamics simulation code developed by the University of Michigan and made publicly runnable through NASA's Community Coordinated Modeling Center.

Components

  • BATS-R-US global MHD simulations run through NASA's Community Coordinated Modeling Center as a public undergraduate lab resource: BATS-R-US (Block-Adaptive-Tree-Solarwind-Roe-Upwind-Scheme) solves the 3D magnetohydrodynamics equations in finite volume form using Roe's Approximate Riemann Solver on an adaptive grid. Students run it on NASA supercomputers at the CCMC, where simulation runs can be requested by the public and results explored and visualized through a standard web browser. The authors note the CCMC resources allow access to powerful simulations without local supercomputer hardware or installing and maintaining simulation codes, and that thorough documentation makes explaining run requests relatively easy. (Crumley et al. (2007))

Claims

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Key Sources

  • Crumley, Palczewski, and Kaster. (2007). Examining the Location of the Magnetopause in an Undergraduate Lab. https://arxiv.org/abs/0706.1985. doi:10.48550/arxiv.0706.1985
Page metadata
Field Value
type product
id bats-r-us-block-adaptive-tree-solarwind-roe-upwind-scheme
title BATS-R-US (Block-Adaptive-Tree Solarwind Roe Upwind Scheme)
description A three-dimensional global magnetohydrodynamics simulation code developed by the University of Michigan and made publicly runnable through NASA's Community Coordinated Modeling Center.
status review
moved_from element/bats-r-us-ccmc-public-simulation-resource
product_kind software
generated by process:sweep-kinds on 2026-10-10
trust unverified — no one has confirmed this page's content
sources 1 — crumley-2007

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