Fig. 7

Sketch of the vertically infinite 2D prominence fine structure model used for analysis of Area1 a), 1D horizontal-slab filament model b), and a general 3D model c). Dotted arrows indicate the incident radiation from the solar surface, while the dash-dotted lines show the directions of the infinite dimensions. Colour highlights the observed surfaces. An LOS drawn in panel c) shows the representative direction towards the observer for Area3.
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