1) bias-induced noise
偏磁感生噪声
2) induced noise
感应噪声，感生噪声
3) polarization noise
偏振噪声
1.
Based on the model mentioned above, a theoretic analysis on the optical path polarization is made, an expression of the highest polarization error is acquired, and furthermore, the influences of each apparatus on polarization noise are discussed.
在此基础上进行了光路偏振噪声的理论分析,通过计算得出最大偏振误差表达式,讨论了光路器件的性能对陀螺偏振噪声的影响,得出消光比是影响结果的关键因子,并阐述了主要有效措施。
2.
Zero drift and polarization noise are the main two hindrances in the development of fiber gyroscopes in China.
采用相干矩阵和琼斯矩阵建立了光纤陀螺光路传输系统的数学模型 ,在此基础上 ,进行了光路偏振噪声的理论分析。
3.
If has been proved theoretically that the deviation will induce phase noise in interferometer,if the error of the Faraday rotator angle is about ±5°,the amplitude of polarization-induced phase noise is related to the polarization noise in lead fiber and the state of polarization of the input light to interferometer,and it is less than 1.
理论分析法拉第旋转角有偏差时,引导光纤中的偏振态扰动(偏振噪声)会在干涉仪中引入相位噪声,该相位噪声水平与引导光纤中的偏振噪声水平和干涉仪输入光的偏振态有关。
4) noise bias
噪声偏差
1.
Because there are many kinds of noise, the noise bias terms are introduced in the iterative shift and add method for astronomical image reconstruction when working in real data.
当工作于实际数据时 ,由于存在着多种噪声 ,导致了天文像复原迭代位移叠加法中的噪声偏差项。
5) bias noise
偏压噪声
补充资料：磁感线
又称“磁力线”。描述磁场分布的假想曲线。该曲线上各点的切线方向就是相应各点的磁场方向。它分布的疏密程度表示磁场的强弱。磁感线可用在磁体周围洒铁屑等方法显示出来。磁感线是闭合曲线，在磁场中磁感线从磁体的n极到s极，在磁体内从s极到n极。
说明：补充资料仅用于学习参考，请勿用于其它任何用途。
参考词条