File:High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere (SVSa000107 details).jpg

Captions

Captions

Descriptive image reads, "Ideal MHD in a model photosphere/corona: Structured spatial mesh: resolution (nx, ny) = (300, 500)Flux-Corrected-Transport, 4th order spatial differences.Predictor-Corrector time advance.Periodic in x, hard wall at bottom.

Summary edit

Description
English: Descriptive image reads, "Ideal MHD in a model photosphere/corona: Structured spatial mesh: resolution (nx, ny) = (300, 500)Flux-Corrected-Transport, 4th order spatial differences.Predictor-Corrector time advance.Periodic in x, hard wall at bottom.Characteristic outflow-no inflow at top.Initial condition:A sheet of magnetic flux suffers a velocity perturbation;the ratio of specific heasts is 1.05,(ct. Shibata et al., 1989 APJ 345 584)."
Date 21 May 1996 (upload date)
Source High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere
Author NASA's Scientific Visualization Studio - Liam Krauss, Dan Spicer, M. L. Rilee, R. Sudan
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Keyword
InfoField
Space science

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current21:31, 10 March 2024Thumbnail for version as of 21:31, 10 March 2024720 × 528 (90 KB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://svs.gsfc.nasa.gov/vis/a000000/a000100/a000107/a000107_details.jpg via Commons:Spacemedia

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