The decay of the large-scale solar magnetic field

In the absence of new bipolar sources of flux, the large-scale magnetic field at the solar photosphere decays as a result of differential rotation, meridional flow, and supergranular diffusion. The rotational shear quickly winds up the nonaxisymmetric components of the field, increasing their latitu...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Solar physics 1987-01, Vol.112 (1), p.17-35
1. Verfasser:	DE VORE, C. R
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Earth, ocean, space Exact sciences and technology Photosphere, granulation Solar physics Solar system
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!