Strong solar flares and coronal mass ejections, here defined not only as the bursts of
electromagnetic radiation but as the entire process in which magnetic energy is released …

Magnetic fields suspend the relatively cool material of solar prominences in an otherwise hot
corona. A comprehensive understanding of solar prominences ultimately requires complex …

Context. Computational astrophysics nowadays routinely combines grid-adaptive
capabilities with modern shock-capturing, high resolution spatio-temporal integration …

Prominences and filaments are manifestations of magnetized, levitated plasma within the
solar coronal atmosphere. Their structure is assumed to be driven by the ambient magnetic …

The complex interaction of the magnetic field with matter is the key to some of the most
puzzling observed phenomena at multiple scales across the Universe, from tokamak plasma …

Hinode is Japan's third solar mission following Hinotori (1981–1982) and Yohkoh (1991–
2001): it was launched on 2006 September 22 and is in operation currently. Hinode carries …

Adopting the MPI-AMRVAC code, we present a 2.5-dimensional magnetohydrodynamic
simulation, which includes thermal conduction and radiative cooling, to investigate the …

Solar filaments are an intriguing phenomenon, like cool clouds suspended in the hot corona.
Similar structures exist in the intergalactic medium as well. Despite being a long-studied …

Context. The tearing instability plays a major role in the disruption of current sheets, whereas
thermal modes can be responsible for condensation phenomena (forming prominences and …

Context. Thermal instability plays a major role in condensation phenomena in the solar
corona (eg, for coronal rain and prominence formation). In flare-relevant current sheets …