Coronal mass ejections and their sheath regions in interplanetary space

E Kilpua, HEJ Koskinen, TI Pulkkinen - Living Reviews in Solar Physics, 2017 - Springer
Interplanetary coronal mass ejections (ICMEs) are large-scale heliospheric transients that
originate from the Sun. When an ICME is sufficiently faster than the preceding solar wind, a …

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 …

[HTML][HTML] The solar orbiter mission-science overview

D Müller, OCS Cyr, I Zouganelis, HR Gilbert… - Astronomy & …, 2020 - aanda.org
Aims. Solar Orbiter, the first mission of ESA's Cosmic Vision 2015–2025 programme and a
mission of international collaboration between ESA and NASA, will explore the Sun and …

A 21st century view of the March 1989 magnetic storm

DH Boteler - Space Weather, 2019 - Wiley Online Library
On 13 March 1989, the largest magnetic storm of the last century caused widespread effects
on power systems including a blackout of the Hydro‐Québec system. Since then this event …

Density of neutral hydrogen in the sun's interstellar neighborhood

P Swaczyna, DJ McComas, EJ Zirnstein… - The Astrophysical …, 2020 - iopscience.iop.org
Interstellar neutral atoms, unlike charged particles, freely penetrate the heliosphere,
allowing us to sample the physical state of the interstellar matter directly. Most interstellar …

[HTML][HTML] Quantifying errors in 3D CME parameters derived from synthetic data using white-light reconstruction techniques

C Verbeke, ML Mays, C Kay, P Riley, E Palmerio… - Advances in Space …, 2023 - Elsevier
Current efforts in space weather forecasting of CMEs have been focused on predicting their
arrival time and magnetic structure. To make these predictions, methods have been …

Space weather: The solar perspective: An update to Schwenn (2006)

M Temmer - Living Reviews in Solar Physics, 2021 - Springer
The Sun, as an active star, is the driver of energetic phenomena that structure interplanetary
space and affect planetary atmospheres. The effects of Space Weather on Earth and the …

Geoeffective properties of solar transients and stream interaction regions

EKJ Kilpua, A Balogh, R Von Steiger, YD Liu - Space Science Reviews, 2017 - Springer
Abstract Interplanetary Coronal Mass Ejections (ICMEs), their possible shocks and sheaths,
and co-rotating interaction regions (CIRs) are the primary large-scale heliospheric structures …

Implementation and validation of the FRi3D flux rope model in EUHFORIA

A Maharana, A Isavnin, C Scolini, N Wijsen… - Advances in Space …, 2022 - Elsevier
Abstract The “Flux Rope in 3D”(FRi3D, Isavnin, 2016), a coronal mass ejection (CME) model
with global three-dimensional (3D) geometry, has been implemented in the space weather …

Sun-to-Earth MHD simulation of the 2000 July 14 “Bastille Day” eruption

T Török, C Downs, JA Linker, R Lionello… - The Astrophysical …, 2018 - iopscience.iop.org
Solar eruptions are the main driver of space-weather disturbances at Earth. Extreme events
are of particular interest, not only because of the scientific challenges they pose, but also …