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Solar Surface Magneto-Convection

Simulation showing up and down streamlines near the solar surface

Vertical cut through a 48-megameter-wide simulation domain showing vertical velocity (red upward, blue downward) and streamlines near the solar surface (top of frame). Diverging upflows sweep downflows toward each other at the boundaries of the larger, deeper-lying upflows.
Credit: NASA Science Mission Directorate, Principle Investigator, Robert Stein




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Last Updated: August 20, 2009