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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 1.

EIS He ii 256 Å velocity maps fitted by a single Gaussian curve (left panel) and double Gaussian curves (middle panel). The velocities that exceed 40/ −40 km s −1 have been set to the top color (red/blue) in order to make the velocity field pattern stand out. The Ca ii H image (right panel) shows that it has similar configurations with the He ii 256 Å velocity maps. The Ca ii H image observed by SOT/BFI is created artificially to match the EIS map in time. See text for details.

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