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- W4385706670 abstract "Abstract We perform numerical simulations of supersonic magnetohydrodynamic (MHD) turbulence and calculate Fourier power spectra of E - and B -modes arising from dust polarization. We pay close attention to the ratio of E -mode to B -mode spectra (a.k.a. E/B power asymmetry) on small spatial scales. We find that the ratio depends on the strength of the mean magnetic field: the stronger the mean magnetic field, the smaller the ratio. More precisely speaking, the ratio scales with the Alfvén Mach number M A , the rms velocity divided by the Alfvén speed of the mean magnetic field, when it lies in the range 1 ≲ M A ≲ 30. This result implies that we can use the E/B power asymmetry to constrain the strength of the mean magnetic field in supersonic and super-Alfvénic MHD turbulence." @default.
- W4385706670 created "2023-08-10" @default.
- W4385706670 creator A5018242289 @default.
- W4385706670 date "2023-08-01" @default.
- W4385706670 modified "2023-10-18" @default.
- W4385706670 title "Obtaining the Strength of the Magnetic Field from E- and B-Modes of Dust Polarization" @default.
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- W4385706670 doi "https://doi.org/10.3847/1538-4357/ace10a" @default.
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