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Estimating the Chromospheric Absorption of Transition Region Moss Emission

  • Authors: Bart De Pontieu, Viggo H. Hansteen, Scott W. McIntosh, and Spiros Patsourakos

De PONTIEU et al. 2009 The Astrophysical Journal 702 1016.

  • Provider: AAS Journals

Caption: Figure 6.

Histograms of the intensity in the two moss regions (marked as A and B in Figure 5) for Fe xii 195 Å observed with STEREO A (full line) and STEREO B (dashed line). Both regions are reduced in intensity by a factor of roughly 0.75 when viewed with STEREO B. This reduction in intensity is caused by Lyman continuum absorption of EUV emission by chromospheric plasma that occurs at similar heights as the EUV emission. Such absorption is increased when the region is viewed from the side, since the observable surface area of chromospheric plasma is increased.

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