Models the Sun's convective surface and coronal mass ejections: turbulent plasma churns via layered simplex-noise (fbm) on the photosphere shader, while magnetic reconnection events periodically snap open coronal loop arcs that fling ionized particles outward. Each flare arc is a cubic Bezier curve sampled by up to 480 additive-blended point particles (8 arcs x 60 particles), staggered along the curve to fake a traveling plasma front.