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    "title": "High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere",
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            "description": "Descriptive image reads, \"Ideal MHD in a model photosphere/corona:<br /> Structured spatial mesh: resolution (nx, ny) = (300, 500)<br />Flux-Corrected-Transport, 4th order spatial differences.<br />Predictor-Corrector time advance.<br />Periodic in x, hard wall at bottom.<br />Characteristic outflow-no inflow at top.<br />Initial condition:<br />A sheet of magnetic flux suffers a velocity perturbation;<br />the ratio of specific heasts is 1.05,<br />(ct. Shibata et al., 1989 APJ 345 584).\"",
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