Figure 3 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 3.

Offsets of images observed by different instruments with respect to MDI. Positive values in the parentheses show that image shifts to east or south, while negative values to west or north. The error bars are also plotted, both in the east–west and the north–south directions.

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