Simulate how solar wind dynamic pressure affects: magnetosphere-ionosphere coupling currents,
Lundstedt (IRF-Lund)
STRUCTURE
A Survey of the Solar System Class web site: mboett/PSC100D/winter09/PSC100D_winter09.html Please take your assigned transmitter.
The Sun
Evolution of understanding of solar wind-gaseous obstacle interaction O. Vaisberg Space Research Institute (IKI), Moscow, Russia
Dave Brain UC Berkeley Space Sciences Lab (Hi folks! Sorry I couldn’t make it!)
