A computer program for calculating the structure of magnetohydrodynamical shocks in interstellar clouds
收藏NIAID Data Ecosystem2026-03-11 收录
下载链接：
https://elsevier.digitalcommonsdata.com/datasets/2653cn4wxz
下载链接
链接失效反馈官方服务：
资源简介：
Abstract
The program solves for the stationary-state profile of a shock propagating in the interstellar medium under the influence of a magnetic field. The number densities of a given set of atomic and molecular species are computed point by point through the shock. Heavy molecules of the polycyclic aromatic hydrocarbon type, for example, may be included amongst the molecular species.
Title of program: MHD
Catalogue Id: ABLS_v1_0
Nature of problem
Shocks are known to be generated in the interstellar medium, for example, in regions of star formation. The structure of the shocks is modified by the interstellar magnetic field. The continuous or C-type shocks which are anticipated in such regions change the physical and chemical state of the gas. Chemical changes to the degree of ionization impinge, in turn, on the shock structure, and so the magnetohydrodynamical (MHD) and chemical rate equations need to be solved simultaneously. The column ...
Versions of this program held in the CPC repository in Mendeley Data
ABLS_v1_0; MHD; 10.1016/0010-4655(90)90143-O
This program has been imported from the CPC Program Library held at Queen's University Belfast (1969-2019)
创建时间：
2019-11-11
