[HTML][HTML] Review of solar energetic particle prediction models

K Whitman, R Egeland, IG Richardson, C Allison… - Advances in Space …, 2023 - Elsevier
Abstract Solar Energetic Particle (SEP) events are interesting from a scientific perspective as
they are the product of a broad set of physical processes from the corona out through the …

Earth-affecting solar transients: a review of progresses in solar cycle 24

J Zhang, M Temmer, N Gopalswamy… - Progress in Earth and …, 2021 - Springer
This review article summarizes the advancement in the studies of Earth-affecting solar
transients in the last decade that encompasses most of solar cycle 24. It is a part of the effort …

Understanding the origins of problem geomagnetic storms associated with “stealth” coronal mass ejections

NV Nitta, T Mulligan, EKJ Kilpua, BJ Lynch… - Space Science …, 2021 - Springer
Geomagnetic storms are an important aspect of space weather and can result in significant
impacts on space-and ground-based assets. The majority of strong storms are associated …

The origin, early evolution and predictability of solar eruptions

LM Green, T Török, B Vršnak, W Manchester… - Space Science …, 2018 - Springer
Coronal mass ejections (CMEs) were discovered in the early 1970s when space-borne
coronagraphs revealed that eruptions of plasma are ejected from the Sun. Today, it is known …

The physical processes of CME/ICME evolution

W Manchester, EKJ Kilpua, YD Liu, N Lugaz… - Space Science …, 2017 - Springer
As observed in Thomson-scattered white light, coronal mass ejections (CMEs) are manifest
as large-scale expulsions of plasma magnetically driven from the corona in the most …

Suppression of coronal mass ejections in active stars by an overlying large-scale magnetic field: a numerical study

JD Alvarado-Gómez, JJ Drake, O Cohen… - The Astrophysical …, 2018 - iopscience.iop.org
We present results from a set of numerical simulations aimed at exploring the mechanism of
coronal mass ejection (CME) suppression in active stars by an overlying large-scale …

What sustained multi-disciplinary research can achieve: The space weather modeling framework

TI Gombosi, Y Chen, A Glocer, Z Huang… - Journal of Space …, 2021 - swsc-journal.org
Magnetohydrodynamics (MHD)-based global space weather models have mostly been
developed and maintained at academic institutions. While the “free spirit” approach of …

Data-driven modeling of solar coronal magnetic field evolution and eruptions

C Jiang, X Feng, Y Guo, Q Hu - The Innovation, 2022 - cell.com
Magnetic fields play a fundamental role in the structure and dynamics of the solar corona. As
they are driven by their footpoint motions on the solar surface, which transport energy from …

Observation-based modelling of magnetised coronal mass ejections with EUHFORIA

C Scolini, L Rodriguez, M Mierla, J Pomoell… - Astronomy & …, 2019 - aanda.org
Context. Coronal mass ejections (CMEs) are the primary source of strong space weather
disturbances at Earth. Their geo-effectiveness is largely determined by their dynamic …

Planet-induced radio emission from the coronae of M dwarfs: the case of Prox Cen and AU Mic

RD Kavanagh, AA Vidotto, B Klein… - Monthly Notices of …, 2021 - academic.oup.com
There have recently been detections of radio emission from low-mass stars, some of which
are indicative of star–planet interactions. Motivated by these exciting new results, in this …