1 code implementation • 7 Feb 2013 • Ue-Li Pen, Yuri Levin
In this picture, the parts of warm ionized interstellar medium that are responsible for the scintillations are relatively quiescent, with scintillation and scattering resulting from weak waves propagating along magnetic domain boundary current sheets, which are both expected from helicity conservation and have been observed in numerical simulations.
Astrophysics of Galaxies
