The current understanding of astrophysical magnetic fields is reviewed, focusing on their
generation and maintenance by turbulence. In the astrophysical context this generation is …

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 flux emergence from the solar convection zone into the overlying atmosphere is
the driver of a diverse range of phenomena associated with solar activity. In this article, we …

We present the first quantitative comparison between the total magnetic reconnection flux in
the low corona in the wake of coronal mass ejections (CMEs) and the magnetic flux in …

Context. Magnetic clouds are transient magnetic structures expulsed from the Sun that travel
toward the external heliosphere carrying a significant amount of magnetic flux and helicity …

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 …

Several recent studies have developed the measurement of magnetic helicity flux from the
time evolution of photospheric magnetograms. The total flux is computed by summing the …

The magnetic energy and relative magnetic helicity in two emerging solar active regions, AR
11072 and AR 11158, are studied. They are computed by integrating over time the energy …

We identified 17 magnetic clouds (MCs) with durations longer than 30 h, surveying the solar
wind data obtained by the WIND and ACE spacecraft during 10 years from 1995 through …

Aims. We investigate the formation of flux ropes in a flux emergence region and their rise
into the outer atmosphere of the Sun. Methods. We perform 3D numerical experiments by …