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提高白天观测星体信噪比的方法研究
Improvement of signal to noise ratio in astronomical objects detection in daytime
【摘要】 为提高对天体目标的检测概率,对多种可提高探测器检测概率的途径进行了研究。研究结果表明:光谱滤波技术能有效提高信噪比。为得到大的探测对比度和信噪比,需合理选取探测系统视场,应保证目标像所占像素个数不小于2×2;还应令系统在不加衰减器的情况下,电荷耦合器件(CCD)接近饱和并保证CCD不饱和。结合探测系统视场的选取,利用形态学方法对图像进行处理,将大大提高探测信噪比,从而大大提高检测概率。
【Abstract】 Detection for a faint astronomical object in daytime is an extremely complex issue because of low target-background-contrast and low signal-to-noise ratio. Some ways to improve the detection probability is studied in this paper. The results show, spectral filtering technology is an effective way to improve signal-to-noise ratio. The reasonable choice of field of view is helpful to get higher signal-to-noise ratio and contrast. With the reasonable choice of field of view and the effective application of morphology-based detection algorithm, the detection efficiency could be greatly improved.
【Key words】 Faint astronomical objects; Detection efficiency; Daytime; Image processing; Signal-to-noise ratio;
- 【文献出处】 强激光与粒子束 ,High Power Laser & Particle Beams , 编辑部邮箱 ,2003年12期
- 【分类号】P161
- 【被引频次】51
- 【下载频次】494