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Characterizing Magnetized Turbulence in M51

  • Authors: Martin Houde, Andrew Fletcher, Rainer Beck, Roger H. Hildebrand, John E. Vaillancourt, and Jeroen M. Stil

Houde et al. 2013 The Astrophysical Journal 766 49.

  • Provider: AAS Journals

Caption: Figure 3.

Orientation of the Gaussian ellipsoid characterizing our idealization of magnetized turbulence in the ( v 1, v 2, u) coordinate system. The v 1 and v 2 axes define the plane of the sky, while the line of sight points along the negative u-axis. The inclination angle relative to the line of sight of the ellipsoid symmetry axis (and of B 0) is given by α, while the angle β defines the orientation of its projection on the plane of the sky.

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