MANCHA 3D numerical experiments and observations:
(It is recommended download the movies instead of reproduce them in the web browser)
- Large-Amplitude longitudinal oscillations in a solar prominence. See the similarity with the oscillations in the aircraft-carrier prominence.
- Filament formation and eruption by flux cancellation.
- Reconstruction of filament magnetic field using large-amplitude seismology.
- Magnetic Rayleigh-Taylor instability in prominences: 0.3 Gauss, 4 Gauss, and 10 Gauss.
- Prominence formation: Hα end view, side view, SDO/AIA 171Å end view, side view, SDO/AIA 211Å end view, side view.
- Oscillations of multi-strand solar corona: Movie