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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 2.

Example of an angular structure function. Panel (a) shows hypothetical turbulent (triple-dot-broken curve) and ordered (dot-broken curve) contributions to the total angular structure function langΔΦ 2(ℓ) rang plotted in panel (b) (solid curve). Panel (c) presents the same information as panel (b) but displayed as a function of ℓ 2 instead of ℓ. The total angular structure function is subtracted from a Taylor series fit obtained from its values at ℓ ⩾ 6'' (dot-broken curve in panels (b) and (c)) to get the turbulent autocorrelation function shown in panel (d). The correlation length characterizing turbulence is represented by δ.

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