File:High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere (SVSa000107 details).jpg
High_Resolution_2-D_Numerical_Simulation_of_Emergence_of_Magnetic_Flux_Through_the_Solar_Atmosphere_(SVSa000107_details).jpg (720 × 528 pixels, file size: 90 KB, MIME type: image/jpeg)
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DescriptionHigh Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere (SVSa000107 details).jpg |
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 domainPublic domainfalsefalse |
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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current | 21:31, 10 March 2024 | 720 × 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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