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Formation Heights of Extreme Ultraviolet Lines in an Active Region Derived by Correlation of Doppler Velocity and Magnetic Field

  • Authors: Y. Guo, M. D. Ding, M. Jin, and T. Wiegelmann

GUO et al. 2009 The Astrophysical Journal 696 1526.

  • Provider: AAS Journals

Caption: Figure 2.

Top left: the FOV of the magnetic field observed by SOT/SP from 20:30 to 21:33 UT on 2006 December 12. The dashed square denotes the FOV in which the NLFFF extrapolation is performed. Bottom left: the three-dimensional magnetic field extrapolated by the NLFFF model for the dashed square shown in the top left panel. Top right: the FOV of MDI magnetogram for potential field extrapolation observed at 20:51 UT on 2006 December 12. The dashed square is the similar to that in the top left panel. Bottom right: the three-dimensional magnetic field extrapolated by the potential field model. Note that only the region in the dashed square is shown.

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