Luc Dame

In summary: Strong Solar Science Cases
for AFSIIC
• AFSIIC (before HiRISE and in complement –
hopefully – of ASPIICS PROBA-3) are adapted to
present challenging Solar Physics observations,
especially:
The dynamics of the small scale structure of active and quiet
magnetic fields and its relation to heating
Oscillations and energetics of the chromospheric small scale
structure, noticeably spicules (mass)
Coronal magnetic fields direct measurements (IR)
The magneto-hydrodynamics of sunspots and magnetoseismology
in general (e.g. with a Magneto-Optical Filter)