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 …

Since its introduction to astro-and solar physics, the concept of helicity has proven to be
useful in providing critical insights into physics of various processes from astrophysical …

In this work, we present results of a time-dependent data-driven numerical simulation
developed to study the dynamics of coronal active region magnetic fields. The evolving …

The topology and dynamics of the three-dimensional magnetic field in the solar atmosphere
govern various solar eruptive phenomena and activities, such as flares, coronal mass …

The relative magnetic helicity is a quantity that is often used to describe the level of
entanglement of non-isolated magnetic fields, such as the magnetic field of solar active …

Context. The discovery of clear criteria that can deterministically describe the eruptive state
of a solar active region would lead to major improvements on space weather predictions …

Solar flares fall into two types, with eruptive ones associated with coronal mass ejection
(CME) and confined ones without CME. To explore whether there are preflare conditions in …

Context. Data-driven, time-dependent magnetofrictional modeling has proved to be an
efficient tool for studying the pre-eruptive build-up of energy for solar eruptions, and …

The nonlinear force-free field (NLFFF) model is often used to describe the solar coronal
magnetic field, however a series of earlier studies revealed difficulties in the numerical …

In this ISSI-supported series of studies on magnetic helicity in the Sun, we systematically
implement different magnetic helicity calculation methods on high-quality solar …