Skip to main content
Log in

Geomagnetic activity and wind velocity during the Maunder minimum

  • Original articles
  • Published:
Annales Geophysicae

Abstract

Following a given classification of geomagnetic activity, we obtained aa index values for the Maunder minimum (1645–1715). It is found that the recurrent and fluctuating activities were not appreciable and that the shock activity levels were very low. The aa index level was due almost entirely to the quiet days. Calculated average solar-wind velocities were 194.3 km s−1 from 1657 to 1700 and 218.7 km s−1 from 1700 onwards. Also, the coronal magnetic field magnitude and southward interplanetary magnetic field component Bz were lower. It is concluded that the nearly absent levels of geomagnetic activity during this period were due to lower coronal and Bz magnetic field magnitudes as well as to the continuous impinging on the Earth of a slow wind.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

Author information

Authors and Affiliations

Authors

About this article

Cite this article

Mendoza, B. Geomagnetic activity and wind velocity during the Maunder minimum. Annales Geophysicae 15, 397–402 (1997). https://doi.org/10.1007/s00585-997-0397-3

Download citation

  • Received:

  • Revised:

  • Accepted:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s00585-997-0397-3

Keywords

Navigation