The brightness temperature of Mercury at mm-wavelengths

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Table 4:

Mercury: $\langle T_{\rm B}\rangle$ and $\Delta T_{\rm B}$ as a function of frequency/wavelength, for cosine approximations irrespective of Mercury's surface regions.
Frequency	Wavelength	$\langle T_{\rm B}\rangle$	$\Delta T_{\rm B}$	$\Omega$	Ref.
$\nu$ (GHz)	$\lambda$ [mm]	[K]	[K]	[ $\hbox {$^\circ $ }$ ]
8	37.5	380 $\pm$ 4	55 $\pm$ 3	32 $\pm$ 4	1
10.7	28	374 $\pm$ 4	42 $\pm$ 5	36 $\pm$ 7	2
90.0	3.3	359 $\pm$ 4	147 $\pm$ 6	17 $\pm$ 2	2
90	3.5-2.6	317 $\pm$ 3	137 $\pm$ 4	17.6	3
142.8	2.1	350 $\pm$ 20	150 $\pm$ 15	20	4, in 2
150	1.9-2.1	295 $\pm$ 19	176 $\pm$ 23	17.5	3
230	1.2-1.4	278 $\pm$ 10	154 $\pm$ 15	8.2	3

Ref. 1: Klein (1970), Eq. (1); 2: Epstein & Andrew (1985); 3: this paper; 4: Davis (in 2).

Source LaTeX | All tables | In the text

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