Rossby wave instability does not require sharp resistivity gradients

W. Lyra; N. J. Turner; C. P. McNally

doi:10.1051/0004-6361/201424919

Rossby wave instability does not require sharp resistivity gradients

W. Lyra, N. J. Turner, C. P. McNally

Astrofysik og Planetforskning

35 Citationer (Scopus)

Originalsprog	Engelsk
Artikelnummer	A10
Tidsskrift	Astronomy & Astrophysics
Vol/bind	574
ISSN	0004-6361
DOI	https://doi.org/10.1051/0004-6361/201424919
Status	Udgivet - 1 feb. 2015

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10.1051/0004-6361/201424919

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@article{a1bdf040038b4eb18e38ab95e76e6670,

title = "Rossby wave instability does not require sharp resistivity gradients",

keywords = "accretion, accretion disks, planets and satellites: formation, instabilities, magnetohydrodynamics (MHD), turbulence, methods: numerical",

author = "W. Lyra and Turner, {N. J.} and McNally, {C. P.}",

year = "2015",

month = feb,

day = "1",

doi = "10.1051/0004-6361/201424919",

language = "English",

volume = "574",

journal = "Astronomy and Astrophysics Supplement Series",

issn = "0004-6361",

publisher = "E D P Sciences",

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TY - JOUR

T1 - Rossby wave instability does not require sharp resistivity gradients

AU - Lyra, W.

AU - Turner, N. J.

AU - McNally, C. P.

PY - 2015/2/1

Y1 - 2015/2/1

KW - accretion, accretion disks

KW - planets and satellites: formation

KW - instabilities

KW - magnetohydrodynamics (MHD)

KW - turbulence

KW - methods: numerical

U2 - 10.1051/0004-6361/201424919

DO - 10.1051/0004-6361/201424919

M3 - Journal article

SN - 0004-6361

VL - 574

JO - Astronomy and Astrophysics Supplement Series

JF - Astronomy and Astrophysics Supplement Series

M1 - A10

ER -

Rossby wave instability does not require sharp resistivity gradients

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