Study on the Transmission Characteristics of Polarized Laser in the Complicated Dust Environment on Mars

Table 2

The vertical distribution of the number concentration and effective radius of Martian dust particles corresponding to the three models [17, 18].

Height/km	Case 1: b = 0.10		Case 2: b = 0.25		Case 3: b = 0.40
	n/cm^3	reff/μm	n/cm^3	reff/μm	n/cm^3	reff/μm
0	1.31	1.76	2.26	1.90	5.56	2.05
1	1.18	1.75	2.06	1.88	5.09	2.03
2	1.07	1.74	1.88	1.87	4.67	2.01
3	0.97	1.73	1.71	1.85	4.28	1.99
4	0.87	1.72	1.56	1.84	3.93	1.97
5	0.79	1.71	1.43	1.82	3.62	1.94
6	0.72	1.70	1.30	1.80	3.34	1.91
7	0.65	1.68	1.19	1.78	3.08	1.88
8	0.59	1.67	1.09	1.75	2.86	1.85
9	0.53	1.65	1.00	1.73	2.65	1.81
10	0.48	1.64	0.92	1.70	2.47	1.78
11	0.43	1.62	0.85	1.67	2.31	1.74
12	0.39	1.60	0.78	1.64	2.16	1.69
13	0.36	1.58	0.72	1.61	2.04	1.65
14	0.33	1.55	0.68	1.57	1.94	1.60
15	0.30	1.53	0.64	1.54	1.86	1.55
16	0.27	1.50	0.60	1.49	1.79	1.50
17	0.25	1.47	0.56	1.45	1.72	1.44
18	0.23	1.44	0.52	1.41	1.65	1.38
19	0.20	1.41	0.48	1.36	1.56	1.33
20	0.18	1.38	0.44	1.32	1.47	1.27
21	0.16	1.34	0.40	1.26	1.40	1.20
22	0.14	1.29	0.38	1.20	1.32	1.14
23	0.13	1.25	0.35	1.15	1.25	1.08
24	0.12	1.20	0.33	1.09	1.20	1.02