Fig. 10
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Example of a quiescent prominence, observed on June 22, 2010. Top row: Hinode/SOT observations in the Ca II H line (left) and the Hα line 0.0208 nm from the line centre (right). Images are aligned to show the same FOV of 103″ × 99″. Bottom row: SDO/AIA 17.1, 19.3, and 30.4 nm channel observations. Labels indicate arcseconds. Adapted from Gunár et al. (2018).
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