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. 2017 Sep 4;292(9):130. doi: 10.1007/s11207-017-1161-9

Figure 6.

Figure 6

Variation in brightness temperatures across the FOV in non-isothermal large-scale prominence models. The isobaric pressure is 0.1dyncm2 and the FOV is orientated vertically in the solar atmosphere, with the positive x-axis directed radially away from the Sun.