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
Edition
Acta Astronomica, PL - Polská republika, 2013, 0001-5237
Other information
Type of outcome
Article in a journal
Field of Study
10308 Astronomy
Confidentiality degree
is not subject to a state or trade secret
Impact factor
Impact factor: 1.955
Organization unit
Faculty of Philosophy and Science in Opava
EID Scopus
2-s2.0-84881266743
Keywords in English
accretion, accretion disks;magnetohydrodynamics (MHD);instabilities;black hole physics
Tags
International impact, Reviewed
Links
EE2.3.20.0071, research and development project.
In the original language
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.
Displayed: 10/2/2026 09:57