Sustained turbulence and magnetic energy in non-rotating shear flows

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Standard

Sustained turbulence and magnetic energy in non-rotating shear flows. / Nauman, Farrukh; Blackman, Eric G.

I: Physical Review E, Bind 95, Nr. 3, 033202, 23.07.2017.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Harvard

Nauman, F & Blackman, EG 2017, 'Sustained turbulence and magnetic energy in non-rotating shear flows', Physical Review E, bind 95, nr. 3, 033202. https://doi.org/10.1103/PhysRevE.95.033202

APA

Nauman, F., & Blackman, E. G. (2017). Sustained turbulence and magnetic energy in non-rotating shear flows. Physical Review E, 95(3), [033202]. https://doi.org/10.1103/PhysRevE.95.033202

Vancouver

Nauman F, Blackman EG. Sustained turbulence and magnetic energy in non-rotating shear flows. Physical Review E. 2017 jul. 23;95(3). 033202. https://doi.org/10.1103/PhysRevE.95.033202

Author

Nauman, Farrukh ; Blackman, Eric G. / Sustained turbulence and magnetic energy in non-rotating shear flows. I: Physical Review E. 2017 ; Bind 95, Nr. 3.

Bibtex

@article{c257e1a602cd4ce6997c50c5debd91d1,
title = "Sustained turbulence and magnetic energy in non-rotating shear flows",
abstract = "From numerical simulations, we show that non-rotating magnetohydrodynamic shear flows are unstable to finite amplitude velocity perturbations and become turbulent, leading to the growth and sustenance of magnetic energy, including large scale fields. This supports the concept that sustained magnetic energy from turbulence is independent of the driving mechanism for large enough magnetic Reynolds numbers.",
keywords = "physics.plasm-ph, astro-ph.GA, astro-ph.SR",
author = "Farrukh Nauman and Blackman, {Eric G.}",
note = "5 pages, 5 figures, under review in PRL",
year = "2017",
month = jul,
day = "23",
doi = "10.1103/PhysRevE.95.033202",
language = "English",
volume = "95",
journal = "Physical Review E",
issn = "2470-0045",
publisher = "American Physical Society",
number = "3",

}

RIS

TY - JOUR

T1 - Sustained turbulence and magnetic energy in non-rotating shear flows

AU - Nauman, Farrukh

AU - Blackman, Eric G.

N1 - 5 pages, 5 figures, under review in PRL

PY - 2017/7/23

Y1 - 2017/7/23

N2 - From numerical simulations, we show that non-rotating magnetohydrodynamic shear flows are unstable to finite amplitude velocity perturbations and become turbulent, leading to the growth and sustenance of magnetic energy, including large scale fields. This supports the concept that sustained magnetic energy from turbulence is independent of the driving mechanism for large enough magnetic Reynolds numbers.

AB - From numerical simulations, we show that non-rotating magnetohydrodynamic shear flows are unstable to finite amplitude velocity perturbations and become turbulent, leading to the growth and sustenance of magnetic energy, including large scale fields. This supports the concept that sustained magnetic energy from turbulence is independent of the driving mechanism for large enough magnetic Reynolds numbers.

KW - physics.plasm-ph

KW - astro-ph.GA

KW - astro-ph.SR

U2 - 10.1103/PhysRevE.95.033202

DO - 10.1103/PhysRevE.95.033202

M3 - Journal article

C2 - 28415182

VL - 95

JO - Physical Review E

JF - Physical Review E

SN - 2470-0045

IS - 3

M1 - 033202

ER -

ID: 172897569