Tracing the magnetic field and magnetohydrodynamic turbulence mode in the Cygnus Loop

Open Access

Fig. 8.

Distribution of correlation function for $I + Q \propto B_{x}^{2}$ $Mathematical equation: $ I+Q \propto B_{x}^{2} $$ (left panel) and $I - Q \propto B_{y}^{2}$ $Mathematical equation: $ I-Q \propto B_{y}^{2} $$ (right panel) for the central region. We draw dashed white lines to depict the direction of the mean magnetic-field component in the plane of sky (B_⊥), which is also the reference axis for estimating the anisotropy in both the v direction (B_⊥) and the h direction.

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