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MAGNETIC UPFLOW EVENTS IN THE QUIET-SUN PHOTOSPHERE. I. OBSERVATIONS

  • Authors: S. Jafarzadeh, L. Rouppe van der Voort, and J. de la Cruz Rodríguez

2015 The Astrophysical Journal 810 54.

  • Provider: AAS Journals

Caption: Figure 2.

Examples of far-blue-wing Stokes V (top left), in-line Stokes V (top right), far-red-wing Stokes V (bottom left), and Stokes I continuum (bottom right) images from the Fe I 6302 Å line. The Stokes V images are saturated to the same scale. The blue and red circles mark detected magnetic upflow/downflow events (MUEs/MDEs), respectively. Both events are of either polarities and absolute values of their signals are only used for detection purposes. On the upper panels: one of the MUEs is magnified, the red arrows indicate two examples of apparent MUE candidates that do not meet signal threshold criterion, and the yellow arrows mark an example where the MUE visually shows strong signals in both images.

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