Fig. 5 from The Effects of Noise and Sampling on the Spectral Correlation Function

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The Effects of Noise and Sampling on the Spectral Correlation Function

Authors: Paolo Padoan, Erik W. Rosolowsky, and Alyssa A. Goodman

Padoan, Rosolowsky, & Goodman 2001 The Astrophysical Journal 547 862.

Provider: AAS Journals

Caption: Fig. 5.

(a) Normalized SCF vs. Q for the MHD model (two top panels), and the Heiles cloud 2 data (two bottom panels). The normalized SCF is obtained by dividing the SCF by the analytic function ﹩1-1/ Q﹩. (b) Histograms of the normalized SCF plotted in the left panels. Only points from the left panels with ﹩Q> 2﹩ are used, since spectra with ﹩Q< 2﹩ are dominated by noise.

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