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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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