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 噪声改正
 noise correction
 Noise Correction in Power Spectrum and Image Reconstruction with Speckle Holography 功率谱噪声改正和斑点全息术象复原 短句来源
 “噪声改正”译为未确定词的双语例句
 After Characteristic of noise is studied in the wavelet domain, it is proposed that corrective technique of noise is based on wavelet transform and adaptation. 通过研究各类噪声在小波域的特征，提出了基于小波变换迭代回归的噪声改正方法，综合数据研究表明在加入5—10倍的噪声后，利用本文提出的方法改正后信号的相关性高，相关系数达0.91以上； 短句来源
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 Noise Correction in Power Spectrum and Image Reconstruction with Speckle Holography 功率谱噪声改正和斑点全息术象复原 短句来源 and noise group (N. G.) 和噪声组(N.G.) 短句来源 (2) Does the above mentioned the only source of Xu-duan or the other species, D. ,现改正为D. 短句来源 A recommended acceptable noise level can be determined from the teacheras response to the noise under investigation. 噪声调查； 短句来源 CCD image correcting technique was adopted to decrease CCD self-noise; 为了减小CCD引入的噪声,还采用了CCD图象改正技术; 短句来源

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 noise correction
 Noise correction for roughening analysis of magnetic flux profiles in YBa$_\mathsf{2}$Cu$_\mathsf{3}$O$_\mathsf{7-x}$ After noise correction, we find that the magnetic field profile is characterized by a roughness exponent $\alpha = 0.75(6)$. This dark current also degrades the performance of cameras containing these pixels by increasing the residual fixed pattern noise following fixed pattern noise correction. Although not exploited in this work, the features of the proposed model make it feasible for noise correction in 3-D PET. Expression intensities were prepared with default smoothing adjustments, noise correction, and quantile normalization in Microarray Suite. 更多
 TwokindsofnoisesinspeckledataarousedbythespeckleimagedetectingsystemofYunnanObservatory:recodingnoiseforspecklegrameandsystematicerorcousedbythediferenceofatmosphericseeingarediscussed.Pre-processingmethodstore-movethesenoisesaredescribed.Theresultsofexperimentsclearlyshowthatthepre-processingisefectiveanditisnecessarytoachievehighresolutionimagereconstructionforastronomicalobjects. 主要讨论了由云南天文台的斑点象探测系统引入斑点数据中的两种噪声：斑点图记录噪声和由大气视宁度差异引起的系统误差，叙述了用于克服噪声的预处理方法，噪声改正的实验结果表明：这些预处理对于实现天文目标的高分辨率象复原是有效的和必须的 In astronomical high resolution image reconstruction, Fourier modulus recovery is as important as the phase recovery of a object, because there are many kinds of complex noise in observations and the recovery of modulus or phase will become more difficult. To solve the problem of the noise of all kinds in the modulus recovery, some appropriate methods are provided. The experimental results of image reconstruction show that these methods are effective and necessary, they ensured the high precision modulus recovery.... In astronomical high resolution image reconstruction, Fourier modulus recovery is as important as the phase recovery of a object, because there are many kinds of complex noise in observations and the recovery of modulus or phase will become more difficult. To solve the problem of the noise of all kinds in the modulus recovery, some appropriate methods are provided. The experimental results of image reconstruction show that these methods are effective and necessary, they ensured the high precision modulus recovery. 在天文高分辨率像复原中 ,目标的傅里叶模复原与相位复原同样重要。由于观测数据中存在着多种复杂噪声 ,模和相位的复原将变得更加困难。本文针对在模复原中的各种噪声 ,提出相应的噪声改正方法 ,所给出的像复原实验表明 ,这些方法是有效的和必须的 ,它们保证了模的高精度复原
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