Helical dynamo growth and saturation at modest versus extreme magnetic Reynolds numbers-Reference-Cited by-同舟云学术

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Helical dynamo growth and saturation at modest versus extreme magnetic Reynolds numbers

Published:2024-01-19 Issue:1 Volume:109 Page:
ISSN:2470-0045
Container-title:Physical Review E
language:en
Short-container-title:Phys. Rev. E

Author:

Zhou Hongzhe^ORCID,Blackman Eric G.

Funder

Shanghai Jiao Tong University

China Postdoctoral Science Foundation

Isaac Newton Institute for Mathematical Sciences

Engineering and Physical Sciences Research Council

National Science Foundation

U.S. Department of Energy

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevE.109.015206/fulltext

Reference48 articles.

1. THE STELLAR-ACTIVITY-ROTATION RELATIONSHIP AND THE EVOLUTION OF STELLAR DYNAMOS

2. Magnetic fields in spiral galaxies

3. Efficient generation of jets from magnetically arrested accretion on a rapidly spinning black hole

4. Long-term GRMHD simulations of neutron star merger accretion discs: implications for electromagnetic counterparts

5. Hydromagnetic Dynamo Models.

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