There is no direct means to measure the amount of magnetic flux dragged out from the corona by the solar wind to form the “open” solar flux (OSF) component which…Read More >
- SPATE PhD studentships available!
- A diagnosis of the plasma waves responsible for the explosive energy release of substorm onset
- Nudging solar wind forecasts back towards reality
- Modelling asymmetric current sheets in Earth’s magnetosphere
- Forecast uncertainty in the near-Earth solar wind conditions