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Two-dimensional MHD model of gas flow dynamics near a young star with a jet and a protoplanetary disk. / Григорьев, Виталий Валерьевич; Демидова, Татьяна Валерьевна.

Astronomy at the epoch of multimessenger studies. Москва : Janus-K, 2022. стр. 142-144.

Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференцийстатья в сборнике материалов конференциинаучнаяРецензирование

Harvard

Григорьев, ВВ & Демидова, ТВ 2022, Two-dimensional MHD model of gas flow dynamics near a young star with a jet and a protoplanetary disk. в Astronomy at the epoch of multimessenger studies. Janus-K, Москва, стр. 142-144, ВСЕРОССИЙСКАЯ АСТРОНОМИЧЕСКАЯ КОНФЕРЕНЦИЯ — 2021, Москва, Российская Федерация, 23/08/21. <https://www.vak2021.ru/wp-content/uploads/2022/03/VAK_2021_proceedings.pdf>

APA

Vancouver

Григорьев ВВ, Демидова ТВ. Two-dimensional MHD model of gas flow dynamics near a young star with a jet and a protoplanetary disk. в Astronomy at the epoch of multimessenger studies. Москва: Janus-K. 2022. стр. 142-144

Author

BibTeX

@inproceedings{1a4cdbc3e07e470f993f5df568afb962,
title = "Two-dimensional MHD model of gas flow dynamics near a young star with a jet and a protoplanetary disk",
abstract = "Within the framework of a nonstationary MHD approach,the interaction of a jet, a partially ionized gas of the stellar corona, anda protoplanetary disk with a constant dipole magnetic eld of a youngstar of the T Tauri type on a two-dimensional axisymmetric computa-tional grid is considered. The model takes into account the degree ofgas ionization, optically thin cooling, anisotropic thermal conductivityand viscosity. Numerical modeling is performed using the free PLUTOpackage. The simulations were performed using the resources of the JointSuperComputer Center of the Russian Academy of Sciences.",
author = "Григорьев, {Виталий Валерьевич} and Демидова, {Татьяна Валерьевна}",
year = "2022",
language = "English",
pages = "142--144",
booktitle = "Astronomy at the epoch of multimessenger studies",
publisher = "Janus-K",
address = "Russian Federation",
note = "Всероссийская астрономическая конференция 2021 {"}Астрономия в эпоху многоканальных исследований{"}, ВАК-2021 ; Conference date: 23-08-2021 Through 28-08-2021",
url = "https://www.vak2021.ru/, https://www.vak2021.ru, https://www.vak2021.ru/timetable/",

}

RIS

TY - GEN

T1 - Two-dimensional MHD model of gas flow dynamics near a young star with a jet and a protoplanetary disk

AU - Григорьев, Виталий Валерьевич

AU - Демидова, Татьяна Валерьевна

PY - 2022

Y1 - 2022

N2 - Within the framework of a nonstationary MHD approach,the interaction of a jet, a partially ionized gas of the stellar corona, anda protoplanetary disk with a constant dipole magnetic eld of a youngstar of the T Tauri type on a two-dimensional axisymmetric computa-tional grid is considered. The model takes into account the degree ofgas ionization, optically thin cooling, anisotropic thermal conductivityand viscosity. Numerical modeling is performed using the free PLUTOpackage. The simulations were performed using the resources of the JointSuperComputer Center of the Russian Academy of Sciences.

AB - Within the framework of a nonstationary MHD approach,the interaction of a jet, a partially ionized gas of the stellar corona, anda protoplanetary disk with a constant dipole magnetic eld of a youngstar of the T Tauri type on a two-dimensional axisymmetric computa-tional grid is considered. The model takes into account the degree ofgas ionization, optically thin cooling, anisotropic thermal conductivityand viscosity. Numerical modeling is performed using the free PLUTOpackage. The simulations were performed using the resources of the JointSuperComputer Center of the Russian Academy of Sciences.

M3 - Conference contribution

SP - 142

EP - 144

BT - Astronomy at the epoch of multimessenger studies

PB - Janus-K

CY - Москва

T2 - Всероссийская астрономическая конференция 2021 "Астрономия в эпоху многоканальных исследований"

Y2 - 23 August 2021 through 28 August 2021

ER -

ID: 93735730