The Linear Fitting Method for Model of PIN Array Receiver in Space Optical Communication

Table 1

Comparison between Newton-Raphson and proposed methods.

Temperature/°C	Light intensity/(mW/cm^2)			Error /%
		25	100		17.75	17.68	0.39
61.81	62.51			1.13
35	80	16.32	16.30	0.12
		45.76	46.05	0.6
50	60	14.87	14.61	1.7
		32.37	32,65	0.86
60	40	13.25	13.01	1.81
		20.10	20.31	1.04
70	20	11.82	11.79	0.25
		10.03	10.46	4.28