Studying Astrophysical Turbulence: Progress Report on Statistical Tools

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I shall discuss two techniques of studying astrophysical turbulence using observations of fluctuations of the profiles of Doppler-broaderned spectral lines. These techniques are Velocity Channel Analysis (VCA) and Velocity Coordinate Spectrum (VCS). While VCA is a well-established technique by now, VCS is a relatively new development. I shall show results obtained (in collaboration with A. Chepurnov) of using the two techniques to the same data sets. Unlike earlier studies, where I concentrated on the assymptotics, I shall show the results obtained where entire information was used. The results obtained by VCA and VCS assuringly correspond to each other and indicate interesting deviations from Kolmogorov behavior.

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