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SUMMARY:Simulation of nonrelativistic jets using a solution of the Grad-Sh
 afranov equation as the initial condition
DTSTART;VALUE=DATE-TIME:20181022T124000Z
DTEND;VALUE=DATE-TIME:20181022T151000Z
DTSTAMP;VALUE=DATE-TIME:20260808T124323Z
UID:indico-contribution-1331@cern.ch
DESCRIPTION:Speakers: Ilia Kalashnikov (National Research Nuclear Universi
 ty MEPhI)\nThere are several problems in the numerical simulation of jets 
 of young stars: the results of calculations depend very much on the initia
 l conditions\, most of which are unknown from observational data. Analytic
 al approaches\, based on the solution of the Grad-Shafranov equation\, can
  only provide a stationary one-dimensional picture of what is happening.\n
 \nThe purpose of this work is to combine the above two approaches\, using 
 the plasma configuration and its magnetic field\, obtained by solving the 
 Grad-Shafranov equation\, as the initial conditions for the magnetohydrody
 namic modeling of a jet. The dynamics of jet propagation through the surro
 unding space was investigated\, morphology similar to the morphology of th
 e observed jets was obtained. Also the stability of the solution of the Gr
 ad-Shafranov equation with finite perturbations was numerically investigat
 ed.\n\nhttps://indico.particle.mephi.ru/event/22/contributions/1331/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1331/
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