Extending Velocity Channel Analysis for Studying Turbulence Anisotropies
Dinesh Kandel, Alex Lazarian, Dmitri Pogosyan

TL;DR
This paper extends the velocity channel analysis method to study turbulence anisotropies in magnetized media, revealing how different MHD modes influence observed anisotropy and demonstrating applicability to various observational setups.
Contribution
It introduces an analytical extension of VCA to analyze anisotropies from magnetic fields and distinguishes contributions from different MHD modes in spectroscopic data.
Findings
Anisotropy in thick channels reflects density field anisotropy.
Fast modes produce opposite anisotropy compared to Alfven and slow modes.
Method applicable to interferometric observations and absorption lines.
Abstract
We extend the velocity channel analysis (VCA), introduced by Lazarian & Pogosyan, of the intensity fluctuations in the velocity slices of position-position-velocity (PPV) spectroscopic data from Doppler broadened lines to study statistical anisotropy of the underlying velocity and density that arises in a turbulent medium from the presence of magnetic field. In particular, we study analytically how the anisotropy of the intensity correlation in the channel maps changes with the thickness of velocity channels. In agreement with the earlier VCA studies we find that the anisotropy in the thick channels reflects the anisotropy of the density field, while the relative contribution of density and velocity fluctuations to the thin velocity channels depends on the density spectral slope. We show that the anisotropies arising from Alfven, slow and fast magnetohydrodynamical modes are different,…
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