Figure 5 from Formation Heights of Extreme Ultraviolet Lines in an Active Region Derived by Correlation of Doppler Velocity and Magnetic Field

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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 5.

Correlation heights vs. log T _max for Regions 1–3. The magnetic field is extrapolated with the NLFFF model except for the top right panel, in which the potential field model is used. The dotted lines are the linear fitting of the height–log T _max relationship.

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