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Statistical Tracing of Magnetic Fields: Comparing and Improving the Techniques

  • Authors: Ka Ho Yuen, Junda Chen, Yue Hu, Ka Wai Ho, A. Lazarian, Victor Lazarian, Bo Yang, Blakesley Burkhart, Caio Correia, Jungyeon Cho, Bruno Canto, and J. R. De Medeiros

2018 The Astrophysical Journal 865 54.

  • Provider: AAS Journals

Caption: Figure 5.

Illustration showing the pipelines of PCAA. We first project the PPV cubes along either of the spatial directions (panel 1), in which we would call the compressed PPV cubes “PV tires” (panel 2) in which the covariance matrix S of the PV tires (panel 3, Equation (15)) can be computed. The eigenvalues of the covariance matrix (panel 4) contain the velocity information along this particular PV tire, and the ﹩{e}^{-1}﹩ lag of the autocorrelation functions of the eigenvectors and eigen-projections (panel 5, Equation (21)) tells us the characteristic velocities ﹩\delta {v}_{x,y}﹩ and length scales ﹩{L}_{x,y}﹩, respectively.

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