HAL (France)open access
Coexisting Tayler instability-driven dynamos in radiative zones: New dynamo solution and its impacts on stellar physics
Dynamo, 2, Stars magnetic field, 0, 1, Stars interiors, Method numerical, Magnetohydrodynamics MHD
This document is indexed with metadata only — full text is not available in the archive for this record.
Open the official source ↗
Record · ID 652728
Conceptio Open Knowledge Archive — every document is proof-bundled with source, license, and retrieval metadata.