A method to statistically characterize turbulent data with physically motivated parameters, illustrated on a centroid velocity map

no code implementations • 18 Jan 2021 • J. -B. Durrive, P. Lesaffre, T. Ghosh, B. Regaldo-Saint Blancard

Hence, thanks to this procedure, one may characterize statistically, and thus compare, various turbulent data.

Astrophysics of Galaxies Solar and Stellar Astrophysics Fluid Dynamics Plasma Physics