J 2013

Possible suppression of magnetorotational instability by rapid radial flow

ABRAMOWICZ, Marek, Jiří HORÁK and Włodek KLUŹNIAK

Basic information

Original name

Possible suppression of magnetorotational instability by rapid radial flow

Authors

ABRAMOWICZ, Marek, Jiří HORÁK and Włodek KLUŹNIAK

Edition

Acta Astronomica, PL - Polská republika, 2013, 0001-5237

Other information

Language

English

Type of outcome

Článek v odborném periodiku

Field of Study

10308 Astronomy

Confidentiality degree

není předmětem státního či obchodního tajemství

References:

Organization unit

Faculty of Philosophy and Science in Opava

UT WoS

000323396300008

Keywords in English

accretion, accretion disks;magnetohydrodynamics (MHD);instabilities;black hole physics

Tags

Tags

International impact, Reviewed

Links

EE2.3.20.0071, research and development project.
Změněno: 15/4/2021 10:50, Mgr. Pavlína Jalůvková

Abstract

V originále

By investigating the magnetorotational instability (MRI) in a region of rapidly varying accretion-disk thickness, e.g., in the ISCO region, we find a limit to the applicability of a recent finding by Balbus (2012) that the MRI is present also in the region of Rayleigh-unstable flow.