The quiet Sun is the region of the solar surface outside of sunspots, pores, and plages. In
continuum intensity it appears dominated by granular convection. However, in polarized …

In this article we review small-scale dynamo processes that are responsible for magnetic
field generation on scales comparable to and smaller than the energy carrying scales of …

Supergranulation is a fluid-dynamical phenomenon taking place in the solar photosphere,
primarily detected in the form of a vigorous cellular flow pattern with a typical horizontal …

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 …

With an emphasis on numerical modelling, Physics of the Sun: A First Course presents a
quantitative examination of the physical structure of the Sun and the conditions of its …

We study the photospheric footpoints of a set of 35 coronal jets in a coronal hole as
observed by Hinode/EIS. We use SDO/AIA data to coalign the spectroscopic EIS data with …

A number of observational and theoretical aspects of solar magnetoconvection are
considered in this review. We discuss recent developments in our understanding of the …

The Sun is replete with magnetic fields, with sunspots, pores and plage regions being their
most prominent representatives on the solar surface. But even far away from these active …

We present the first quiet Sun spectropolarimetric observations obtained with the Visible
SpectroPolarimeter at the 4 m Daniel K. Inouye Solar Telescope. We recorded observations …

The energy for the coronal heating must be provided from the convection zone. However,
the amount and the method by which this energy is transferred into the corona depend on …