Abstract
Historical data of the geomagnetic activity records in St. Petersburg since 1841 do not show any ‘doubling’ of the total magnetic field at the Sun as claimed recently by Lockwood et al. (1999). However, recurrent patterns of the geomagnetic activity variations display ‘secular’ trend of the solar wind near ecliptic plane resulting from gradual change of the topological structure of the solar corona (Ponyavin, 1997). By comparing geomagnetic and eclipse observations we found ‘typical’ coronal shapes, which correspond better to periods of extremely low and high geomagnetic activity level rather than standard sunspot activity referencing as ‘Corona at Solar Maximum or Minimum’. Using geomagnetic records as proxies it has been suggested that the maximum of the sunspot activity was in July 2000.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Ahluwalia, H. S.: 1998, J. Geophys. Res. 103, 12103–12109.
Bruckner, Ed.: 1890, Geographische Abhandlungen 4 (2), 153–484.
Clough, H. W.: 1905, Astrophys. J. 22, 42–75.
Koutchmy, S., Belmandi, M., Coulter, R. L., et al.: 1994, Astron. Astrophys. 281, 249–257.
Lockwood, M., Stamper, R., and Wild, M. N.: 1999, Nature 399, 437–439.
Loucif, M. L. and Koutchmy, S.: 1989, Astron. Astrophys. Suppl. Ser. 77, 45–66.
Ponyavin, D. I.: 1995, Space Sci. Rev. 72, 185–188.
Ponyavin, D. I.: 1997, Proceedings 31st ESLAB Symposium `Correlated phenomena at the Sun, in the Heliosphere and in Geospace’ 97,ESTEC, Noordwijk, The Netherlands, 22–25 September 1997, ESA SP-415, pp. 481–483.
Ponyavin, D. I.: 1999, in V. S. Semenov, H. K. Biernat, M. V. Kubyshkina, C. J. Farrugia, and S. Muhlbachler (eds), Proceedings of the 2nd International Workshop `Problems of Geospace 2’, St.Petersburg, June 29 —July 3, 1998, Verlag der Österreichischen Akademie der Wissenschaften, Wien, pp. 361–366.
Zosimovitch, I. D.: 1981, Geomagnetic Activity and Corpuscular Stability of the Sun, Nauka, Moscow.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2001 Springer Science+Business Media Dordrecht
About this paper
Cite this paper
Ponyavin, D.I. (2001). Geomagnetic Tracing of the Inner Heliosphere. In: Marsden, R.G. (eds) The 3-D Heliosphere at Solar Maximum. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-3230-7_36
Download citation
DOI: https://doi.org/10.1007/978-94-017-3230-7_36
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-5723-5
Online ISBN: 978-94-017-3230-7
eBook Packages: Springer Book Archive