莱斯衰减
噪音(视频)
高斯噪声
震级(天文学)
分布(数学)
高斯分布
信噪比(成像)
强度(物理)
信号(编程语言)
核磁共振
计算机科学
物理
人工智能
数学
算法
图像(数学)
光学
数学分析
解码方法
量子力学
衰退
天文
程序设计语言
作者
Hákon Guðbjartsson,Samuel Patz
标识
DOI:10.1002/mrm.1910340618
摘要
Abstract The image intensity in magnetic resonance magnitude images in the presence of noise is shown to be governed by a Rician distribution. Low signal intensities (SNR < 2) are therefore biased due to the noise. it is shown how the underlying noise can be estimated from the images and a simple correction scheme is provided to reduce the bias. the noise characteristics in phase images are also studied and shown to be very different from those of the magnitude images. Common to both, however, is that the noise distributions are nearly Gaussian for SNR larger than two.
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