An advanced thermal roughness model for airless planetary bodies - Implications for global variations of lunar hydration and mineralogical mapping of Mercury with the MERTIS spectrometer

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Table 5

Best fit parameters for twelve EPF measurements of Diviner channels four and seven.

		Channel four (8.25 µm)		Channel seven (25 – 41 µm)
No.	A_dh		w		w
01	0.099	37	0.11	35	0.18
02	0.097	28	0.17	29	0.18
03	0.090	34	0.26	34	0.20
04	0.080	37	0.12	31	0.16
05	0.070	28	0.00	28	0.00
06	0.075	19	0.42	19	0.16
07	0.061	29	0.17	32	0.15
08	0.042	34	0.20	36	0.17
09	0.053	34	0.20	27	0.19
10	0.054	29	0.11	26	0.13
11	0.041	28	0.18	27	0.18
12	0.028	26	0.31	27	0.23
	0.066	30.250	0.188	29.250	0.161

Notes. See Table 2 for locations and geometries. The directional hemispherical albedo A_dh is derived from M³ measurements beforehand. The roughness and the single scattering albedo w are inferred via a simple grid search. The last row provides the average values.

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