Fig. 5
Thermal profiles over the polar night region as a function of effective latitude (−45°, −60°, and −75°), for thermal inertia values of 5, 12, 22, 37, and 60 J m-2 K-1 s-0.5, which are hereafter compared with MIRO SMM and MM brightness temperatures. The emission depths (Le) for a regolith with lunar-like dielectric properties are indicated for both wavelengths.
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