Storm will help us understand the nature of the dayside magnetopause better.
- XRI observes rate/location of magnetopause and cusp erosion.
- FUV observes rate/location of auroral oval expansions and brightening.
- MAG and IES provide solar wind input, identify triggers significance from amplitudes of magnetopause, oval, and cusp motion
Picking out RMPdistance to Magnetopause
thestormmission.com 