Possible suppression of magnetorotational instability by rapid radial flow

@article{43588,
   author = {Abramowicz, Marek and Horák, Jiří and Kluźniak, Włodek},
   article_location = {PL - Polská republika},
   article_number = {2},
   keywords = {accretion, accretion disks;magnetohydrodynamics (MHD);instabilities;black hole physics},
   language = {eng},
   issn = {0001-5237},
   journal = {Acta Astronomica},
   title = {Possible suppression of magnetorotational instability by rapid radial flow},
   url = {http://acta.astrouw.edu.pl/Vol63/n2/pdf/pap_63_2_8.pdf},
   volume = {63},
   year = {2013}
}

TY  - JOUR
ID  - 43588
AU  - Abramowicz, Marek - Horák, Jiří - Kluźniak, Włodek
PY  - 2013
TI  - Possible suppression of magnetorotational instability by rapid radial flow
JF  - Acta Astronomica
VL  - 63
IS  - 2
SP  - 267-273
EP  - 267-273
SN  - 00015237
KW  - accretion, accretion disks;magnetohydrodynamics (MHD);instabilities;black hole physics
UR  - http://acta.astrouw.edu.pl/Vol63/n2/pdf/pap_63_2_8.pdf
N2  - 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.
ER  - 

ABRAMOWICZ, Marek, Jiří HORÁK a Włodek KLU$\backslash$'ZNIAK. Possible suppression of magnetorotational instability by rapid radial flow. \textit{Acta Astronomica}. PL - Polská republika, 2013, roč.~63, č.~2, s.~267-273. ISSN~0001-5237.