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- W2034876006 abstract "Abstract The recent solar minimum (2008-2009) was extreme in several aspects: the sunspot number, R z , interplanetary magnetic field (IMF) magnitude B o and solar wind speed V sw were the lowest during the space era. Furthermore, the variance of the IMF southward B z component was low. As a consequence of these exceedingly low solar wind parameters, there was a minimum in the energy transfer from solar wind to the magnetosphere, and the geomagnetic activity ap index reached extremely low levels. The minimum in geomagnetic activity was delayed in relation to sunspot cycle minimum. We compare the solar wind and geomagnetic activity observed in this recent minimum with previous solar cycle values during the space era (1964-2010). Moreover, the geomagnetic activity conditions during the current minimum are compared with long term variability during the period of available geomagnetic observations. The extremely low geomagnetic activity observed in this solar minimum was previously recorded only at the end of XIX century and at the beginning of the XX century, and this might be related to the Gleissberg (80-100 years) solar cycle." @default.
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- W2034876006 date "2011-10-01" @default.
- W2034876006 modified "2023-10-01" @default.
- W2034876006 title "Extremely low geomagnetic activity during the recent deep solar cycle minimum" @default.
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- W2034876006 doi "https://doi.org/10.1017/s174392131200484x" @default.
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