1) temporal correlated observation noise
时间相关观测噪声
2) correlated measurement noises
相关观测噪声
1.
For the multisensor systems with correlated measurement noises and different measurement matrices,two correlated measurement fusion steady-state Kalman filtering algorithms are presented by using the weighted least squares (WLS)method.
对于带相关观测噪声和带不同观测阵的多传感器系统,用加权最小二乘(Weighted least squares,WLS)法提出了两种相关观测融合稳态Kalman滤波算法。
2.
For the multisensor systems with correlated measurement noises and unknown noise statistics,the on-line noise statistics estimators are obtained by the correlation method.
对带相关观测噪声和未知噪声统计的多传感器系统,用相关方法得到噪声统计在线估值器。
3.
For the multi-sensor linear discrete time-varying stochastic control systems with correlated measurement noises and different measurement matrices,two weighted measurement fusion Kalman estimators are developed by using the weighted least squares(WLS)method.
对于带相关观测噪声和带不同观测阵的多传感器线性离散时变随机控制系统,用加权最小二乘法(WLS)提出了两种加权观测融合Kalman估值器,它们包括状态滤波、状态预报和状态平滑。
3) temporal correlation noise
时域相关噪声
1.
In distributed video coding (DVC) because the decoder cannot have access to the current frame,modeling the temporal correlation noise becomes a difficult task.
在分布式视频编码(DVC)中,由于解码端不能获取当前编码帧的信息,精确地对时域相关噪声进行建模变得更为困难。
4) noise correlation time
噪声关联时间
1.
The effective eigenvalue λ eff and the intensity correlation time T C of the system are derived for different noise correlation time τ.
对于不同的噪声关联时间τ ,求出了系统的有效本征值λeff和强度相关时间Tc。
5) correlated spatial noise fields
空间相关噪声场
6) spatial correlated noise
空间相关噪声
补充资料：时间
实际上，时间单位首先从天文观测来确定的，“1平太阳日或1天（1昼夜）”是以地球相对于太阳的自转周期为基准来计量的，一个平太阳日的1/86400为1秒；后来发现地球自转不均匀，1960年国际度量衡大会把时间基准改为以地球绕太阳公转周期，即规定为1900年地球公转周期（回归年）的1/31556925.9747为1秒；随着精确、稳定的原子钟制成，1967年国际度量衡大会规定国际单位制原子时的时间单位“秒（长）是两个超精细能级之间跃进所对应辐射9192631770个周期的持续时间”。
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