Rossby wave instability does not require sharp resistivity gradients

Research output: Contribution to journal › Journal article › Research › peer-review

Standard

Rossby wave instability does not require sharp resistivity gradients. / Lyra, W.; Turner, N. J.; McNally, C. P.

In: Astronomy & Astrophysics, Vol. 574, A10, 02.02.2015.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Lyra, W, Turner, NJ & McNally, CP 2015, 'Rossby wave instability does not require sharp resistivity gradients', Astronomy & Astrophysics, vol. 574, A10. https://doi.org/10.1051/0004-6361/201424919

APA

Lyra, W., Turner, N. J., & McNally, C. P. (2015). Rossby wave instability does not require sharp resistivity gradients. Astronomy & Astrophysics, 574, [A10]. https://doi.org/10.1051/0004-6361/201424919

Vancouver

Lyra W, Turner NJ, McNally CP. Rossby wave instability does not require sharp resistivity gradients. Astronomy & Astrophysics. 2015 Feb 2;574. A10. https://doi.org/10.1051/0004-6361/201424919

Author

Lyra, W. ; Turner, N. J. ; McNally, C. P. / Rossby wave instability does not require sharp resistivity gradients. In: Astronomy & Astrophysics. 2015 ; Vol. 574.

Bibtex

@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 = "2",
doi = "10.1051/0004-6361/201424919",
language = "English",
volume = "574",
journal = "Astronomy & Astrophysics",
issn = "0004-6361",
publisher = "E D P Sciences",

}

RIS

TY - JOUR

T1 - Rossby wave instability does not require sharp resistivity gradients

AU - Lyra, W.

AU - Turner, N. J.

AU - McNally, C. P.

PY - 2015/2/2

Y1 - 2015/2/2

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

VL - 574

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

SN - 0004-6361

M1 - A10

ER -

ID: 154444372