Bernal M P, Burr G W, Coufal H, Quintanilla M
Appl Opt. 1998 Aug 10;37(23):5377-85. doi: 10.1364/ao.37.005377.
We investigate the effects of interpixel cross talk and detector noise on the areal storage density of holographic data storage. A numerical simulation is used to obtain the bit-error rate (BER) as a function of hologram aperture, pixel fill factors, and additive Gaussian intensity noise. We consider the effect of interpixel cross talk at an output pixel from all possible configurations of its 12 closest-neighbor pixels. Experimental verification of this simulation procedure is shown for several fill-factor combinations. The simulation results show that areal density is maximized when the aperture coincides with the zero order of the spatial light modulator (SLM) (Nyquist sampling condition) and the CCD fill factor is large. Additional numerical analysis including finite SLM contrast and fixed-pattern noise show that, if the fixed-pattern noise reaches 6% of the mean signal level, the SLM contrast has to be larger than 6:1 to maintain high areal density. We also investigate the improvement of areal density when error-prone pixel combinations are forbidden by using coding schemes. A trade-off between an increase in areal density and the redundancy of a coding scheme that avoids isolated-on pixels occurs at a code rate of approximately 83%.
我们研究了像素间串扰和探测器噪声对全息数据存储面密度的影响。通过数值模拟获得误码率(BER)与全息图孔径、像素填充因子和加性高斯强度噪声的函数关系。我们考虑了输出像素与其12个最邻近像素的所有可能配置下像素间串扰的影响。针对几种填充因子组合展示了该模拟过程的实验验证。模拟结果表明,当孔径与空间光调制器(SLM)的零级重合(奈奎斯特采样条件)且CCD填充因子较大时,面密度最大。包括有限SLM对比度和固定图案噪声的额外数值分析表明,如果固定图案噪声达到平均信号电平的6%,则SLM对比度必须大于6:1才能维持高面密度。我们还研究了通过使用编码方案禁止易出错像素组合时面密度的提高情况。在大约83%的码率下,面密度增加与避免孤立亮像素的编码方案冗余之间存在权衡。