Disclaimer: The following material is being kept online for archival purposes.
Although accurate at the time of publication, it is no longer being updated. The page may contain broken links or outdated information, and parts may not function in current web browsers.
- We want to get a clear view of the transport of energy from the solar
wind to the magnetosphere and the ionosphere
- Simulations and models will be run based on solar wind inputs and the
results will be compared with data from satellites and group-based
Above is background material for archival reference only.