Magnetorotational instability in Keplerian disks: a nonlocal approach-Reference-Cited by-同舟云学术

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Magnetorotational instability in Keplerian disks: a nonlocal approach

Published:2023-09 Issue:12 Volume:66 Page:1262-1276
ISSN:1063-7869
Container-title:Physics-Uspekhi
language:en
Short-container-title:Phys. Usp.

Author:

Shakura Nikolai I.¹²,Postnov Konstantin A.¹²,Kolesnikov Dmitrii A.¹³,Lipunova Galina V.¹⁴

Affiliation:

1. Lomonosov Moscow State University, Shternberg State Astronomical Institute, Universitetskii prosp. 13, Moscow, 119889, Russian Federation

2. Kazan Federal University, ul. Kremlyovskaya 18, Kazan, 420008, Russian Federation

3. Tel-Aviv University, Raymond and Beverly Sackler School of Physics and Astronomy, Tel-Aviv, Israel

4. Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, Bonn, 53121, Germany

Publisher

Uspekhi Fizicheskikh Nauk (UFN) Journal

Subject

General Physics and Astronomy

Reference30 articles.

1. Advective accretion disks and related problems including magnetic fields

2. The Standard Model of Disc Accretion

3. Magnetic fields in the accretion disks for various inner boundary conditions

4. Flares in accretion disk coronae

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Eigenvalue Problem Describing Magnetorotational Instability in Outer Regions of Galaxies;Mathematics;2024-03-04

2. Role of Biermann Battery Mechanism in Appearance of Magnetic Fields in Accretion Discs;Astronomy Reports;2024-03

3. Flute Instability Effects for Disk Accretion onto Neutron Stars with Strong Magnetic Fields;Astronomy Letters;2023-12

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