Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-23T16:37:53.932Z Has data issue: false hasContentIssue false
  • English
  • Français

The structure and evolution of global solar magnetic fields

Published online by Cambridge University Press:  26 August 2011

Duncan H. Mackay
Duncan H. Mackay*
Affiliation:
School of Mathematics and Statistics, University of St Andrews, St Andrews, Fife, KY16 8HB email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

This review will discuss both observational and theoretical aspects of the Sun's global magnetic field. First recent observations will be described, along with the main physical processes leading to the time evolution and structure of the global field. Following this, recent theoretical models of both the global surface and coronal magnetic field will be presented. The application of these models to the structure of the corona, formation of solar filaments, the onset of CMEs and finally the origin and variation of the Sun's open flux will be discussed.

Keywords

Sun: activitysun: coronasun: magnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S273: The Physics of Sun and Star Spots , August 2010 , pp. 290 - 297
Copyright
Copyright © International Astronomical Union 2011

References

Antiochos, S. K., DeVore, C. R., & Klimchuk, J. A. 1999, Astrophys. J., 510, 485CrossRefGoogle Scholar
Balogh, A., Smith, E. J., Tsurutani, B. T., Southwood, D. J., Forsyth, R. J., & Horbury, T. S. 1995, Science, 268, 1007CrossRefGoogle Scholar
Barnes, G. 2007, Astrophys. J. Lett., 670, L53CrossRefGoogle Scholar
Baumann, I., Schmitt, D., & Schüssler, M. 2006, Astron. Astrophys, 446, 307CrossRefGoogle Scholar
Cook, G. R., Mackay, D. H., & Nandy, D. 2009, Astrophys. J., 704, 1021CrossRefGoogle Scholar
Cremades, H., St.Cyr, O. C. 2007, Advances in Space Research, 40, 1042CrossRefGoogle Scholar
Downs, C., Roussev, I. I., van der Holst, B., Lugaz, N., Sokolov, I. V., & Gombosi, T. I. 2010, Astrophys. J., 712, 1219CrossRefGoogle Scholar
Fisk, L. A. & Zurbuchen, T. H. 2006, Journal of Geophysical Research (Space Physics), 111, 9115Google Scholar
Forbes, T. G., et al. 2006, Space Science Reviews, 123, 251CrossRefGoogle Scholar
Hathaway, D. H. 2010, Living Reviews in Solar Physics, 7, 1CrossRefGoogle Scholar
Lin, J., Soon, W., & Baliunas, S. L., 2003, New Astronomy Review, 47, 53CrossRefGoogle Scholar
Lionello, R., Linker, J. A., & Mikić, Z. 2009, Astrophys. J., 690, 902CrossRefGoogle Scholar
Lockwood, M., Stamper, R., & Wild, M. N. 1999, Nature, 399, 437CrossRefGoogle Scholar
Lockwood, M., Rouillard, A. P., & Finch, I. D. 2009, Astrophys. J., 700, 937CrossRefGoogle Scholar
Mackay, D. H., Jardine, M., Cameron, A. C., Donati, J.-F., & Hussain, G. A. J. 2004, Mon. Not. Roy. Astron. Soc., 354, 737CrossRefGoogle Scholar
Mackay, D. H. & van Ballegooijen, A. A. 2006, Astrophys. J., 641, 577CrossRefGoogle Scholar
Mackay, D. H., Karpen, J. T., Ballester, J. L., Schmieder, B., & Aulanier, G. 2010, Space Science Reviews, 151, 333CrossRefGoogle Scholar
Martin, S. F., Bilimoria, R., & Tracadas, P. W. 1994, Solar Surface Magnetism, 303Google Scholar
Riley, P. 2007, Astrophys. J. Lett., 667, L97CrossRefGoogle Scholar
Rušin, V., et al. 2010, Astron. Astrophys, 513, A45CrossRefGoogle Scholar
Schatten, K. H., Wilcox, J. M., & Ness, N. F. 1969, Solar Phys., 6, 442CrossRefGoogle Scholar
Schrijver, C. J. 2001, Astrophys. J., 547, 475CrossRefGoogle Scholar
Schrijver, C. J. & Title, A. M. 2001, Astrophys. J., 551, 1099CrossRefGoogle Scholar
Schüssler, M. & Baumann, I. 2006, Astron. Astrophys, 459, 945CrossRefGoogle Scholar
Sheeley, N. R. Jr. 2005, Living Reviews in Solar Physics, 2, 5CrossRefGoogle Scholar
Tandberg-Hanssen, E. 1995, Astrophysics and Space Science Library, 199CrossRefGoogle Scholar
van Ballegooijen, A. A. & Martens, P. C. H. 1989, Astrophys. J., 343, 971CrossRefGoogle Scholar
van Ballegooijen, A. A., Priest, E. R., & Mackay, D. H. 2000, Astrophys. J., 539, 983CrossRefGoogle Scholar
Yang, W. H., Sturrock, P. A., & Antiochos, S. K. 1986, Astrophys. J., 309, 383CrossRefGoogle Scholar
Yeates, A. R., Mackay, D. H., & van Ballegooijen, A. A. 2007, Solar Phys., 245, 87CrossRefGoogle Scholar
Yeates, A. R., Mackay, D. H., & van Ballegooijen, A. A. 2008, Solar Phys., 247, 103CrossRefGoogle Scholar
Yeates, A. R. & Mackay, D. H. 2009, Solar Phys., 254, 77CrossRefGoogle Scholar
Yeates, A. R. & Mackay, D. H. 2009, Astrophys. J., 699, 1024CrossRefGoogle Scholar
Yeates, A. R., Attrill, G. D. R., Nandy, D., Mackay, D. H., Martens, P. C. H., & van Ballegooijen, A. A. 2010, Astrophys. J., 709, 1238CrossRefGoogle Scholar
Yeates, A. R., Mackay, D. H., van Ballegooijen, A. A., & Constable, J. A. 2010, arXiv:1006.4011Google Scholar
Wang, Y.-M., Nash, A. G., & Sheeley, N. R. Jr. 1989, Science, 245, 712CrossRefGoogle Scholar