A Comprehensive Three-dimensional Radiative Magnetohydrodynamic Simulation of a Solar Flare (Nature Astronomy, 2018)

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Abstract/Contents

Abstract
In this repository are 3D and 2D simulation snapshots of the radiative magnetohydrodynamics simulation of a flare as description in Cheung et al. (2018, Nature Astronomy). IDL and Python scripts for reading the cubes are also provided. See README.txt.

Description

Type of resource software, multimedia
Date created January 24, 2018

Creators/Contributors

Author Cheung, Mark Chun Ming
Author Rempel, Matthias
Author Chintzoglou, Georgios
Author Chen, Feng
Author Testa, Paola
Author Martinez-Sykora, Juan
Author Sainz Dalda, Alberto
Author DeRosa, Marc Lyle
Author Malanushenko, Anna
Author Hansteen, Viggo
Author De Pontieu, Bart
Author Carlsson, Mats
Author Gudiksen, Boris
Author McIntosh, Scott William

Subjects

Subject Hansen Experimental Physics Laboratory
Subject NASA
Subject Heliophysics
Subject Astrophysics
Subject Radiative Transfer
Subject Solar Flares
Subject Magnetohydrodynamics
Subject Computational Fluid Dynamics
Subject Solar Corona
Subject Solar Convection Zone
Subject Magnetic Reconnection
Genre Dataset

Bibliographic information

Access conditions

Use and reproduction
User agrees that, where applicable, content will not be used to identify or to otherwise infringe the privacy or confidentiality rights of individuals. Content distributed via the Stanford Digital Repository may be subject to additional license and use restrictions applied by the depositor.
License
This work is licensed under a Creative Commons Attribution 3.0 Unported license (CC BY).

Preferred citation

Preferred Citation
Cheung, Mark C. M., Rempel, Matthias et al., A Comprehensive, Three-dimensional Radiative MHD Simulation of a Solar Flare (Nature Astronomy, 2018). Stanford Digital Repository. Available at: https://purl.stanford.edu/dv883vb9686

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