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American Astronomical Society, Astrophysical Journal, 1(751), p. 26, 2012

DOI: 10.1088/0004-637x/751/1/26

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Turbulent Magnetic Field Amplification from Spiral SASI Modes: Implications for Core-Collapse Supernovae and Proto-Neutron Star Magnetization

Journal article published in 2012 by Eirik Endeve ORCID, Christian Y. Cardall, Reuben D. Budiardja, Samuel W. Beck, Alborz Bejnood, Ross J. Toedte, Anthony Mezzacappa, John M. Blondin
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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