Abstract The Solar Optical Telescope (SOT) aboard the Hinode satellite (formerly called
Solar-B) consists of the Optical Telescope Assembly (OTA) and the Focal Plane Package …

The question of what heats the solar corona remains one of the most important problems in
astrophysics. Finding a definitive solution involves a number of challenging steps, beginning …

Recent observations have revealed that magnetohydrodynamic (MHD) waves and
oscillations are ubiquitous in the solar atmosphere, with a wide range of periods. We give a …

Wave and oscillatory activity of the solar corona is confidently observed with modern
imaging and spectral instruments in the visible light, EUV, X-ray and radio bands, and …

We develop a theoretical model that explains the formation of hot coronae around strongly
magnetized neutron stars—magnetars. The starquakes of a magnetar shear its external …

The heating of the solar chromosphere and corona to the observed high temperatures, imply
the presence of ongoing heating that balances the strong radiative and thermal conduction …

Outwardly propagating intensity disturbances are a common feature in large, quiescent
coronal loop structures. In this paper, an overview is given of the observed properties and …

This publication provides an overview of magnetic fields in the solar atmosphere with the
focus lying on the corona. The solar magnetic field couples the solar interior with the visible …

ABSTRACT Advanced three-dimensional (3D) radiative MHD simulations now reproduce
many properties of the outer solar atmosphere. When including a domain from the …

Peace from coloniality has been a device of power within the invention of Latin America
which has engaged in different ways of circulation and domination. For example, we see the …