We present a novel global 3D coronal MHD model called COCONUT, polytropic in its first
stage and based on a time-implicit backward Euler scheme. Our model boosts run-time …

This paper is dedicated to the new implicit unstructured coronal code COCONUT, which
aims at providing fast and accurate inputs for space-weather forecasting as an alternative to …

We present the first statistical analysis of complexity changes affecting the magnetic
structure of interplanetary coronal mass ejections (ICMEs), with the aim of answering the …

Over the last decades, international attempts have been made to develop realistic space
weather prediction tools aiming to forecast the conditions on the Sun and in the …

In recent years, global coronal models have experienced an ongoing increase in popularity
as tools for forecasting solar weather. Within the domain of up to 21.5 R⊙ …

Coronal mass ejections (CMEs) cause severe space weather effects throughout our solar
system. As a fast CME propagates through interplanetary space, it accumulates solar wind …

Context. Coronal mass ejections (CMEs) are large-scale eruptions coming from the Sun and
transiting into interplanetary space. While it is widely known that they are major drivers of …

Context. Solar Orbiter, the new-generation mission dedicated to solar and heliospheric
exploration, was successfully launched on February 10, 2020, 04: 03 UTC from Cape …

Improvement of the model providing the boundary condition of the solar-wind speed near
the Sun is essential for gaining a better forecast of space weather. We optimized the …

Magnetohydrodynamic (MHD) simulations of the solar corona have become more popular
with the increased availability of computational power. Modern computational plasma codes …