Speaker
Mr.
Ilya Kalashnikov
(National Research Nuclear University MEPhI)
Description
One of the most interesting properties of astrophysical jets is that they propagates along the axis of rotation of the accretion disk on the distances, which are many times greater than its diameter.
Using $Z$-Pinch facilities for laboratory simulation of astrophysical jets seems very logical. The Plasma focus is supposed to be a very suitable device for simulation of astrophysical jets.
Results of MHD simulations of jet propagation and its compare with known properties of the laboratory and young stellar object's jets are presented.
Primary author
Mr.
Ilya Kalashnikov
(National Research Nuclear University MEPhI)
Co-authors
Prof.
Valery Chechetkin
(Keldysh Institute of Applied Mathematics)
Dr.
Viacheslav Krauz
(National Research Centre Kurchatov Institute)
