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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 15, issue 4
Ann. Geophys., 15, 397–402, 1997
https://doi.org/10.1007/s00585-997-0397-3
© European Geosciences Union 1997
Ann. Geophys., 15, 397–402, 1997
https://doi.org/10.1007/s00585-997-0397-3
© European Geosciences Union 1997

  30 Apr 1997

30 Apr 1997

Geomagnetic activity and wind velocity during the Maunder minimum

B. Mendoza B. Mendoza
  • Instituto de Geofísica UNAM, Circuito Exterior Ciudad Universitaria, 04510 México DF, México

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.

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