Movie 1 (ようこう/宇宙研):
Soft X-ray images of solar corona observed with soft X-ray
telescope aboard Yohkoh (ISAS)
Movie 2 (飛騨天文台):
Moreton wave (MHD fast mode shock) observed with Flare Monitor
Telescope at Hida Observatory, Kyoto University
Movie 3 (SOHO/NASA):
White light images of outer solar corona observed
with SOHO/LASCO
Movie 4 (HST/NASA): Waves in Crab Nebula wind observed with HST
Movie 5 (横山央明):
2D MHD numerical simulations of magnetic reconnection occurring
between emerging flux and overlying coronal field
(Yokoyama and Shibata 1995, Nature 375, 42). The case of
oblique coronal magnetic field, as a model of X-ray jet.
These figures show the
density distribution, velocity vectors, and magnetic field lines.
Movie 6 (横山央明):
The same as in Movie 5 but for temperature
(Yokoyama and Shibata 1995, Nature 375, 42).
Movie 7 (工藤哲洋):
2D MHD simulations of magnetically driven jets ejected from
a thin accretion disk (Kudoh et al. 2000, in preparation).
Movie 8 (林満):
2D MHD simulations of protostellar flares
(Hayashi et al. 1996, ApJ 468, L37).
Movie 9 (林満):
The same as in Movie 8 but for 3D plot of magnetic field configuration
(Hayashi et al. 1996, ApJ 468, L37.
Movie 10 (田沼俊一):
2D MHD simulations of galactic flares (reconnection) triggered by
supernova shock
(Tanuma et al. 1999, PASJ 51, 161).