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Paper: Flux Emergence and Pore Formation: What ATST can See
Volume: 463, 2nd ATST-EAST Workshop in Solar Physics: Magnetic Fields from the Photosphere to the Corona
Page: 83
Authors: Stein, R. F.; Nordlund, Å.
Abstract: Pores form spontaneously in flux emergence simulations where minimally structured (uniform, untwisted, horizontal) magnetic field rises from a depth of 20 Mm. With 1 kG incident field pores formed after about a turnover time (2 days). To compare what ATST will see with current telescopes a very high resolution (6 km) magneto-convection simulation was carried out with an initially uniform, vertical field. Stokes V-profiles were compared for the simulation and as modified for the diffraction pattern for the ATST and the SST.
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