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Paper: The Decay of a Simulated Pore
Volume: 325, The Solar-B Mission and the Forefront of Solar Physics
Page: 57
Authors: Cameron, R.; Voegler, A.; Shelyag, S.; Schuessler, M.
Abstract: Using MURaM — Max-Planck Institut für Aeronomie University of Chicago Radiative Magnetohydrodynamics — an MHD code which includes radiative transfer and partial ionization, we have studied the decay phase of a solar pore. The simulations are sufficiently realistic in their treatment of the photosphere to allow a direct comparison with observations, both current and those of upcoming missions such as Solar-B. As well as discussing the structure and decay of pores, we show the formation of shallow, field aligned, convective rolls which are an important feature of our solutions.
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