Fig. 7


Subsurface temperature distribution at different depths d′ (along the MIRO line of sight) at the respective MIRO observation time. Stars show the same selected surface points as in Fig. 2, and circles refer to 1 FWHM and 2 FWHM beam widths of the SubMM and MM channel. The horizontal axes of these plots are aligned with those of the respective spots in Fig. 2.

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