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Cited article:

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Why take the square root? An assessment of interstellar magnetic field strength estimation methods

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Thermal and Turbulent Properties of the Warm Neutral Medium in the Solar Neighborhood

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ROHSA: Regularized Optimization for Hyper-Spectral Analysis

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DHIGLS: DRAO H i INTERMEDIATE GALACTIC LATITUDE SURVEY

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https://doi.org/10.3847/1538-4357/834/2/126

The structure of the thermally bistable and turbulent atomic gas in the local interstellar medium

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A method for reconstructing the variance of a 3D physical field from 2D observations: application to turbulence in the interstellar medium

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