MHD simulations show CNM clouds are elongated along the local magnetic field with lower disorder per column density than the WNM, explaining the f_CNM-polarization trend for low-cloud-count sightlines.
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3 Pith papers cite this work, alongside 5 external citations. Polarity classification is still indexing.
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astro-ph.GA 3years
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UNVERDICTED 3representative citing papers
Observational modeling of GWA and LAB survey spectra yields 19.8% CNM, 32.5% UNM and 47.8% WNM, in agreement with the TIGRESS-NCR simulation under fixed spin-temperature boundaries.
Reviews SKA techniques for reconstructing 3D magnetic field vectors in the ISM but presents no new data or derivations.
citing papers explorer
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Phase-dependent magnetic coherence in the turbulent interstellar medium
MHD simulations show CNM clouds are elongated along the local magnetic field with lower disorder per column density than the WNM, explaining the f_CNM-polarization trend for low-cloud-count sightlines.
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Gas Phase Distribution in the Neutral ISM: A Comparison between Observation and Numerical Simulation
Observational modeling of GWA and LAB survey spectra yields 19.8% CNM, 32.5% UNM and 47.8% WNM, in agreement with the TIGRESS-NCR simulation under fixed spin-temperature boundaries.
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3D Magnetic Field Vectors in Space: Bubbles, Clouds, and Filaments
Reviews SKA techniques for reconstructing 3D magnetic field vectors in the ISM but presents no new data or derivations.