Magnetic Flux Transport on the Sun

Although most of the magnetic flux observed on the sun originates in the low-latitude sunspot belts, this flux is gradually dispersed over a much wider range of latitudes by supergranular convective motions and meridional circulation. Numerical simulations show how these transport processes interact...

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Veröffentlicht in:	Science (American Association for the Advancement of Science) 1989-08, Vol.245 (4919), p.712-718
Hauptverfasser:	Y.-M. Wang, Nash, A. G., Sheeley, N. R.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Diameter, figure, rotation, mass Earth, ocean, space Exact sciences and technology Interplanetary magnetic fields Magnetic fields Magnetic flux Magnetism Meridional flow Polar regions Rotation Solar magnetic field Solar magnetic fields Solar Physics Solar rotation Solar system Sun Sun-spots Sunspot cycle Sunspots
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