An advective solar-type dynamo without the $\sf \alpha$ effect

DOI10.1051/0004-6361/200912614zbMath1183.85012arXiv0910.2614OpenAlexW3124429055WikidataQ68677751 ScholiaQ68677751MaRDI QIDQ3551073

Norbert Seehafer, V. V. Pipin

Publication date: 8 April 2010

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

Full work available at URL: https://arxiv.org/abs/0910.2614

zbMATH Keywords

magnetohydrodynamics (MHD)Sun: magnetic fieldsstars: magnetic fields

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (2)

Helicity–vorticity turbulent pumping of magnetic fields in the solar convection zone ⋮ The WKB approximation for the interface dynamo

This page was built for publication: An advective solar-type dynamo without the $\sf \alpha$ effect