Published July 28, 2022
| Version v1
Journal article
Open
The Kelvin-Helmholtz instability in astrospheres.
Authors/Creators
- 1. Space Research Institute (IKI) Russian Academy of Sciences, Moscow, Russia
Description
Videos are isolines of the Mach number in the entire flow area versus time. You can observe the evolution of the Kelvin-Helmholtz instability.
Video_1 shows the flow with the parameter \(\chi = 1.6\) and \(M_\infty = 3\). It's almost a steady stream.
Video_2 shows the flow with the parameter \(\chi = 17\) and \(M_\infty = 3\). There is a very strong instability.
Files
Files
(16.5 MB)
| Name | Size | Download all |
|---|---|---|
|
md5:fe400d71b76c5c178332d5605db78eee
|
2.6 MB | Download |
|
md5:b9090ee4708237fefc6cfdcd3f375977
|
13.8 MB | Download |