Energetics of turbulence generated by chiral MHD dynamos-Reference-Cited by-同舟云学术

Energetics of turbulence generated by chiral MHD dynamos

Published:2018-09-12 Issue:1-2 Volume:113 Page:107-130
ISSN:0309-1929
Container-title:Geophysical & Astrophysical Fluid Dynamics
language:en
Short-container-title:Geophysical & Astrophysical Fluid Dynamics

Author:

Schober J.¹,Brandenburg A.²³⁴,Rogachevskii I.²⁵,Kleeorin N.²⁵

Affiliation:

1. Laboratoire d'Astrophysique, EPFL , Sauverny, Switzerland

2. Nordita, KTH Royal Institute of Technology and Stockholm University , Stockholm, Sweden

3. Laboratory for Atmospheric and Space Physics, JILA and Department of Astrophysical and Planetary Sciences, University of Colorado , Boulder, CO, USA

4. Department of Astronomy, Stockholm University , Stockholm, Sweden

5. Department of Mechanical Engineering, Ben-Gurion University of the Negev , Beer-Sheva, Israel

Funder

Marie Skłodowska-Curie

NSF Astrophysics

Research Council of Norway

European Research Council

Publisher

Informa UK Limited

Subject

Geochemistry and Petrology,Mechanics of Materials,Geophysics,Astronomy and Astrophysics,Computational Mechanics

Link

https://www.tandfonline.com/doi/pdf/10.1080/03091929.2018.1515313

Reference44 articles.

1. Universality of Transport Properties in Equilibrium, the Goldstone Theorem, and Chiral Anomaly

2. Transport coefficients in high temperature gauge theories (I): leading-log results

3. Decay Laws for Three-Dimensional Magnetohydrodynamic Turbulence

4. Dynamic Nonlinearity in Large‐Scale Dynamos with Shear

5. Self-Consistent Evolution of Magnetic Fields and Chiral Asymmetry in the Early Universe

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