Statistical tracing of magnetic fields: comparing and improving the techniques

Magnetohydrodynamic turbulence displays velocity anisotropies that reflect the direction of the magnetic field. This anisotropy has led to the development of a number of statistical techniques for studying magnetic fields in the interstellar medium. In this paper, we review and compare three techni...

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Detalhes bibliográficos
Principais autores: Martins, Bruno Leonardo Canto, Yuen, Ka Ho, Chen, Junda, Hu, Yue, Ho, Kai Wa, Lazarian, A., Lazarian, Victor, Yang, Bo, Burkhart, Blaskesley, Correia, Caio, Cho, Jungyeon, Medeiros, J. R. de
Formato: article
Idioma:English
Publicado em: IOP Publishing
Assuntos:
ISM: general
ISM: magnetic fields
ISM: structure
Magnetohydrodynamics (MHD)
Methods: numerical
Endereço do item:https://repositorio.ufrn.br/jspui/handle/123456789/29403
http://dx.doi.org/10.3847/1538-4357/aada88
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https://repositorio.ufrn.br/jspui/handle/123456789/29403
http://dx.doi.org/10.3847/1538-4357/aada88

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