Confinement of Magnetic Fields Below the Solar Convection Zone

Autor:	Nicholas H. Brummell
Rok vydání:	2020
Předmět:	Physics Work (thermodynamics) Turbulence Laminar flow Tachocline Astrophysics::Cosmology and Extragalactic Astrophysics Mechanics Rotation Magnetic field Physics::Fluid Dynamics Dipole Convection zone Physics::Space Physics Astrophysics::Earth and Planetary Astrophysics
Zdroj:	Astrophysics and Space Science Proceedings ISBN: 9783030553357
DOI:	10.1007/978-3-030-55336-4_31
Popis:	Confining the primordial dipole magnetic field below the convection zone affords the possibility of a serendipitous solution that fits many of the observed qualities of the solar interior rotation profile. Gough and McIntyre [6] pointed this out and derived a laminar balanced model that operates on the slow Eddington-Sweet timescale for this purpose. An interesting question is, what is the role of turbulence? Does the presence of turbulence help or hinder? In the spirit of Michael Thompson’s love of tachocline dynamics, we survey some recent work on these issues.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::1820c83d37c8fa96cdc78d690b6bcc38 https://doi.org/10.1007/978-3-030-55336-4_31 Zobrazit plný text záznamu