Structuring the hot advective accretion flow, as a result interaction of plasma with magnetic field
High Energy Astrophysical Phenomena
2014-08-19 v1
Abstract
We present a magneto-hydrodynamic model developed for investigations of advective non-stationary, asymmetric Keplerian accretion disks in the normal magnetic field. The introduced model allows us to trace the evolution in different fixed moments and to get detailed description of the self-structuring of the disk. We have introduced "meeting coefficients" that define the feedback. It determines the impact from nonlinear effects have over the structure of the flow. We have obtained solutions for the radial structure of the disk for two crucial moments of its evolution.
Keywords
Cite
@article{arxiv.1408.4011,
title = {Structuring the hot advective accretion flow, as a result interaction of plasma with magnetic field},
author = {Krasimira Yankova and Lachezar Filipov},
journal= {arXiv preprint arXiv:1408.4011},
year = {2014}
}
Comments
23 pages, 5 figures, 40th COSPAR Scientific Assembly Moscow, Russia, 2-10 August 2014