no code implementations • 11 Dec 2020 • Yue Hu, Siyao Xu, A. Lazarian
We demonstrate that the anisotropic structure functions of turbulent velocities can be used to estimate both the orientation and strength of magnetic fields.
Astrophysics of Galaxies
no code implementations • 10 Feb 2021 • Siyao Xu, Yue Hu
The interstellar turbulence is magnetized and thus anisotropic.
Astrophysics of Galaxies
no code implementations • 4 Mar 2021 • Mi-Xiang Lan, Hao-Bing Wang, Siyao Xu, Siming Liu, Xue-Feng Wu
Therefore, we conclude that the energy dependence of PD can be used to distinguish these two models for the GRB prompt emission.
High Energy Astrophysical Phenomena