Turbulence Parameters from Statistics of Spectral Line Data Cubes

Details Turbulence Parameters from Statistics of Spectral Line Data Cubes Turbulence Parameters from Statistics of Spectral Line Data Cubes

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..300e&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Statistics

Ism: General, Magnetic Fields, Mhd, Turbulence

Scientific paper

In a previous work, Lazarian & Pogosyan (2000) developed a technique to obtain information on interstellar turbulence by studying the emissivity statistics in velocity channel maps. Here we use MHD simulations to extend previous tests of the method and study anisotropies in two-point statistics, which reveal the direction of the magnetic field.

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