Abstract
Large-scale magnetic field regions are evolving on a time scale of many weeks and months and are also modified during the solar activity cycle. The position of the regions are compared in a pair of consecutive synoptic charts and the horizontal velocity field responsible for their position changes, is inferred. Besides the axially symmetric zonal and meridional drifts, relating to differential rotation and meridional circulation, also non-axially symmetric velocity structures were observed during the last three solar activity cycles. Changes of the position and spatial distribution, as well as temporal variations of the field strength, closely relate to the occurrence and variations of other forms of solar activity such as sunspots, filaments and prominences and coronal structures. In combination with 11-yr cyclic changes of the large-scale velocity field, a new global dynamic regime of the convection zone is described.
Similar content being viewed by others
References
Ambrož, P.: 2001a, Solar Phys. 198, 253.
Ambrož, P.: 2001b, Solar Phys. 199, 251.
Haber, D., Hindman, B. W., Toomre, J., Bogart, R. S., and Hill, F.: 2001, Proc. SOHI 10/GONG 2000 Workshop, ESA SP 464, 213.
Hathaway, D. H.: 1996, Astrophys. J. 460, 1027.
Howard, R. and LaBonte, B.: 1980, Astrophys. J. 239, L33.
Howe, R., Komm, R., and Hill, F.: 2000, Solar Phys. 192, 427.
Kosovichev, A. G. and 41 coauthors: 1997, Solar Phys. 170, 43.
November, L. J.: 1986, Appl. Optics 25, 392.
Snodgrass, H. B.: 1985, Astrophys. J. 291, 339.
Spruit, H. C.: 2003, Solar Phys. 213, 1.
Ulrich, R. K.: 2001, Astrophys. J. 560, 466.
Zhao, J. and Kosovichev, A. G.: 2001. Astrophys. J. 603, 776.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Ambrož, P. Long-Term Dynamics of the Large-Scale Magnetic Structures. Sol Phys 224, 61–68 (2004). https://doi.org/10.1007/s11207-005-3881-5
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1007/s11207-005-3881-5