Submitted by whawkins on April 14, 2016 - 10:25am
Dr. Matthias Rempel is a Senior Scientist in the High Altitude Observatory at the National Center for Atmospheric Research. His research area is solar physics, with special emphasis on theoretical modeling of the solar interior and the solar photosphere.
Numerical simulations of sunspot decay: On the penumbra – Evershed flow – moat flow connection
Submitted by whawkins on September 10, 2014 - 9:25am
Sunspots are the most prominent manifestations of magnetic field in the visible layers of the solar atmosphere. Their origin is a dynamo process operating in the solar convection zone.
Numerical simulations of quiet Sun magnetism
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