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MEG Source Detection Revisited

机译:再探MEG源

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摘要

Magnetoencephalography (MEG) is a multi-channel imaging technique. It uses an array composed of a large number of Superconducting Quantum Interference Device (SQUID) to measure the magnetic fields produced by the primary electric currents inside the brain. The measured spatio-temporal magnetic fields are then used to estimate the locations and strengths of these electric currents, often known as MEG sources. The estimated quantities are finally superimposed with the images generated by magnetic resonance imaging (MRI). The combination of information from MEG and MRI forms the magnetic source image (MSI).A great variety of signal processing and modeling techniques such as Inverse problem, Subspace approach, Independent component analysis (ICA) method, and Beamforming (BF) are used to estimate these sources. The first three approaches require the number of sources be detected a priori. Several shortcomings exist in the currently used methods for detecting the source number. First, the source detection is completed only after - not before - MSI is generated. Secondly, the detection methods are somewhat subjective.In order to provide a solution to the problem of detecting MEG source number for all these approaches, a novel method is developed. The covariance matrix of MEG measurements over all channels is decomposed into the signal and the noise subspaces. The number of sources is shown to be equal to the dimension of the signal subspace. The selection of this dimension is translated into a problem of determining the order of the underlying statistics. This statistical identification is resolved by using Information theoretic criteria which are derived based on Kullback-Leibler divergence. Because the method utilizes originally acquired MEG measurements and implemented before magnetic source images are generated, it is an entirely data-driven approach, more efficient, and less likely to be subjective.
机译:脑磁图(MEG)是一种多通道成像技术。它使用由大量超导量子干扰设备(SQUID)组成的阵列来测量由大脑内部一次电流产生的磁场。然后,将测得的时空磁场用于估算这些电流(通常称为MEG源)的位置和强度。最后,将估计量与由磁共振成像(MRI)生成的图像叠加。来自MEG和MRI的信息的组合形成了磁源图像(MSI)。 大量的信号处理和建模技术(例如反问题,子空间方法,独立分量分析(ICA)方法和波束成形(BF))用于估算这些来源。前三种方法要求先验检测源的数量。当前用于检测源编号的方法中存在一些缺点。首先,仅在生成MSI之后(而不是之前)才完成源检测。其次,检测方法有些主观。 为了提供针对所有这些方法的检测MEG源编号的问题的解决方案,开发了一种新颖的方法。所有通道上MEG测量的协方差矩阵都分解为信号和噪声子空间。源的数量显示为等于信号子空间的尺寸。选择此维度会转化为确定基础统计数据顺序的问题。通过使用基于Kullback-Leibler散度得出的信息理论标准来解决此统计标识。因为该方法利用了最初获取的MEG测量值,并且在生成磁源图像之前实施了该方法,所以它是一种完全由数据驱动的方法,效率更高,主观上也不太可能。

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