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Emission Measure Distribution for Diffuse Regions in Solar Active Regions

  • Authors: Srividya Subramanian, Durgesh Tripathi, James A. Klimchuk, and Helen E. Mason

Subramanian et al. 2014 The Astrophysical Journal 795 76.

  • Provider: AAS Journals

Caption: Figure 1.

Fe XV intensity image of AR 10961 tracked from close to the center of the Sun (2007 August 1) to the limb (2007 August 8). All the images have been plotted with the same field of view of 297'' ×197'' in order to help us track any AR structure through the solar rotation. Though all the AR data have been plotted with the same y-axis scale, the scalings in the x-axis are different. This is because the apparant heliographic longitude (the solar X coordinate) of the AR changes vastly over the solar rotation, unlike the latitude (the solar Y coordinate).

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