HOW FAR CAN MINIMAL MODELS EXPLAIN THE SOLAR CYCLE?

A physically consistent model of magnetic field generation by convection in a rotating spherical shell with a minimum of parameters is applied to the Sun. Despite its unrealistic features the model exhibits a number of properties resembling those observed on the Sun. The model suggests the importanc...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	The Astrophysical journal 2012-04, Vol.749 (1), p.1-5
Hauptverfasser:	SIMITEV, R. D, BUSSE, F. H
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy ASTROPHYSICS, COSMOLOGY AND ASTRONOMY AXIAL SYMMETRY CONVECTION Convection modes Earth, ocean, space Exact sciences and technology MAGNETIC FIELDS MAGNETOHYDRODYNAMICS Mathematical models Rotating Rotating generators SOLAR CYCLE Solar cycles Spherical shells SUN SUNSPOTS
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!