¥Since these phenomena are almost
certainly magnetically
driven, they must incorporate magnetic field observations (line-of-sight and vector magnetogram data)
¥Governing evolutionary equations
believed to be (pretty)
well described by 3-d magnetohydrodynamics (MHD)
¥How does one incorporate the
observations (the A-word) into an MHD model? Solving this problem is absolutely critical if we ever want
to have a predictive
(forecasting) model of space weather.