Swirling astrophysical flows – efficient amplifiers of Alfvén waves!?

DOI10.1051/0004-6361:20021753zbMath1026.76062arXivastro-ph/0212132OpenAlexW3099650057WikidataQ68845266 ScholiaQ68845266MaRDI QIDQ4707267

Swadesh M. Mahajan, Gianluigi Bodo, Andria D. Rogava, Silvano Massaglia

Publication date: 8 July 2003

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0212132

zbMATH Keywords

parametric instabilityastrophysical plasmasAlfvén turbulenceamplification of Alfvén wavesdifferentially rotating magnetized plasmashelical steady flowsincompressible linear perturbationstime-dependent spatial Fourier transforms

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Stability and instability of magnetohydrodynamic and electrohydrodynamic flows (76E25) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

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