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- W2108966901 abstract "In this paper, we use our recent technique for estimating the turbulent component of the magnetic field to derive the structure functions of the unpolarized emission as well as that of the Stokes Q and U parameters of the polarized emission. The solutions for the structure functions to 350 μm SHARP polarization data of OMC-1 allow the determination of the corresponding turbulent correlation length scales. The estimated values for these length scales are 94 ± 01, 73 ± 01, 126 ± 02 (or 20.5 ± 0.2, 16.0 ± 0.2, and 27.5 ± 0.4 mpc at 450 pc, the adopted distance for OMC-1) for the Stokes Q and U parameters, and for the unpolarized emission N, respectively. Our current results for Q and U are consistent with previous results obtained through other methods and may indicate presence of anisotropy in magnetized turbulence. We infer a weak coupling between the dust component responsible for the unpolarized emission N and the magnetic field B from the significant difference between their turbulent correlation length scales." @default.
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- W2108966901 date "2012-03-20" @default.
- W2108966901 modified "2023-09-26" @default.
- W2108966901 title "CHARACTERIZATION OF TURBULENCE FROM SUBMILLIMETER DUST EMISSION" @default.
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- W2108966901 doi "https://doi.org/10.1088/0004-637x/749/1/45" @default.
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