It is a basic feature of the Babcock-Leighton model of the solar cycle that the polar fieId reversal is due to the diffusive decay and poleward drift of the active region fields. The flux from follower regions moves preferentially polewards in each hemisphere, where it cancels with, and then replace
The reversal of the solar polar magnetic fields
โ Scribed by P. R. Wilson; P. S. McIntosh; H. B. Snodgrass
- Publisher
- Springer
- Year
- 1990
- Tongue
- English
- Weight
- 507 KB
- Volume
- 127
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
Some theoretical difficulties confronting the current model of the polar magnetic reversal by cancellation with the flux remnants of decaying active regions are discussed. It is shown that the flux transport equation does not adequately describe the essential physical consequences of the transport of large-scale fields, linked to deep subsurface toroids, over distances comparable with the solar radius. The possibility that subsurface reconnections may release these fields to form U-loops is discussed but it is shown that, in this event, the loops will quickly rise to the surface. Mechanisms whereby the flux may escape through the surface are considered.
๐ SIMILAR VOLUMES
Poleward migration of the magnetic neutral line on the Sun has been calculated for the periods 1945-1950 and 1955-1981 using synoptic charts based on Hc~ observations. Epochs of sign reversal of the solar magnetic field at latitudes 50 ~ to 90 ~ have been determined for these periods. During the cyc
Poleward migration of the magnetic neutral line on the Sun has been computed for the period 1904-1940 using synoptic charts based on Hot observations and the epochs of sign reversal of the solar magnetic field at latitudes 50 ~ to 90 ~ have been determined for this period. During the cycles 16 and 1