Fifth Workshop on Numerical Modeling in MHD and Plasma Physics: Methods, Tools, and Outcomes

Дата: 
с 12/10/2022 по 14/10/2022
Место проведения: 
Virtual hosted in Novosibirsk, Russia
Примечание: 

Institute of Computational Mathematics and Mathematical Geophysics

of Siberian Branch of Russian Academy of Sciences

holds

Fifth Workshop on Numerical Modeling in MHD and Plasma Physics:

Methods, Tools, and Outcomes

 

Virtual hosted in Novosibirsk, Russia

October 12-14, 2022

 

Conference web-site       http://conf.nsc.ru/mhd2022/en       

 

E-mail                                   mhd2022@sscc.ru

 

Topics

  • Numerical methods for MHD equations
  • Particle-in-cell method
  • High performance computing
  • Computational Fluid Dynamics
  • Computational Physics of Plasma
  • Computational Astrophysics

 

Important dates

            Abstracts deadline    July                  25

Notification of acceptance     August             1

Papers deadline                    September       1

Registration fee deadline      October           1

 

Agenda

Over the years, the work on projects of controlled thermonuclear fusion has been progressing. The ultimate purpose is the implementation of a thermonuclear reactor, which will become an ecologically conscious way of solving the energy problem of mankind. А large number of particle accelerators and colliders have been developed and constructed. The natural processes taking place in supernovae, interstellar medium, and galaxies are the main incentive in thermonuclear fusion. A workshop on numerical modeling in MHD and plasma physics is organized in the era of "big data". Observations with telescopes such as ALMA and results of experiments on colliders such as LHC generate huge sets of data. It is necessary not only to process the data, but also to explain the underlying physical processes with comparable quality. The problem of modeling the plasma in cosmos and laboratory is many-sided. For modeling it is necessary to create computational algorithms based on co-design, simulation study, and assessment of the energy efficiency, which satisfy simultaneously the conditions of high computational accuracy, scalability, and efficiency.  The main goal of the workshop is a close and intensive interaction of specialists in the field of numerical methods and parallel computations. The workshop will allow us to formulate current and future requirements for computational models and discuss applications of numerical methods to the problems of plasma physics and astrophysics. The workshop results will be published in the conference proceedings. Conferences and workshops are important life components of the scientific community, therefore, despite all the coronavirus limitations, we hold the traditional workshop on numerical solutions of MHD equations and plasma physics. Considering the current situation, we organize the workshop using virtual conferences. We hope that this format of the conferences will be quite effective and perhaps in the future will provide an opportunity to participate in events, held by scientific centers in the world.        

 

Program committee

            Edouard Audit

            Atomic Energy and Alternative Energies Commission, Gif-sur-Yvette, France

 

            Dmitry Bisikalo

            Institute of Astronomy of RAS, Moscow, Russia

 

            Marina Boronina

            Institute of Computational Mathematics and Mathematical Geophysics of SB RAS,

            Novosibirsk, Russia

 

            Konstantin Brushlinsky

            Keldysh Institute of Applied Mathematics of RAS, Moscow, Russia

 

            Igor Chernykh

            Institute of Computational Mathematics and Mathematical Geophysics of SB RAS,

            Novosibirsk, Russia

 

            Galina Dudnikova

            Institute of Computational Mathematics and Mathematical Geophysics of SB RAS,

            Novosibirsk, Russia

 

            Mikhail Fedoruk

            Novosibirsk State University, Novosibirsk, Russia

 

            Boris Glinskiy

            Institute of Computational Mathematics and Mathematical Geophysics of SB RAS,

            Novosibirsk, Russia

 

            Vladislav Izmodenov

            Space Research Institute of RAS, Moscow, Russia

 

            Andrey Kozlov

            Keldysh Institute of Applied Mathematics of RAS, Moscow, Russia

           

Igor Kulikov               vice-chair

            Institute of Computational Mathematics and Mathematical Geophysics of SB RAS,

            Novosibirsk, Russia

 

            Galina Lazareva

            Peoples' Friendship University of Russia, Moscow, Russia

 

            Vladimir Lukin

            Keldysh Institute of Applied Mathematics of RAS, Moscow, Russia

 

            Mikhail Marchenko

            Institute of Computational Mathematics and Mathematical Geophysics of SB RAS,

            Novosibirsk, Russia

 

            Sergey Moiseenko

            Space Research Institute of RAS, Moscow, Russia

 

            Boris Rybakin

            Lomonosov Moscow State University, Moscow, Russia

 

            Eugeny Stepin

            Keldysh Institute of Applied Mathematics of RAS, Moscow, Russia

 

            Aleksei Taiurskii

            Keldysh Institute of Applied Mathematics of RAS, Moscow, Russia

 

            Alexander Tutukov

            Institute of Astronomy of RAS, Moscow, Russia

 

            Eduard Vorobyov

            University of Vienna, Vienna, Austria

 

Vitaly Vshivkov         chair

            Institute of Computational Mathematics and Mathematical Geophysics of SB RAS,

            Novosibirsk, Russia

           

Victor Zhukov

            Keldysh Institute of Applied Mathematics of RAS, Moscow, Russia

 

Abstract submission

            The abstract in English (one page) should be mailed to contact e-address

            mhd2022@sscc.ru

 

Proceedings

            Lobachevskii Journal of Mathematics           (Web of Science / Scopus)

 

Registration fee

            5000    Russian rubles