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 …

Space Weather: From solar origins to risks and hazards evolving in time

N Buzulukova, B Tsurutani - Frontiers in Astronomy and Space …, 2022 - frontiersin.org
Space Weather is the portion of space physics that has a direct effect on humankind. Space
Weather is an old branch of space physics that originates back to 1808 with the publication …

Decoding the pre-eruptive magnetic field configurations of coronal mass ejections

S Patsourakos, A Vourlidas, T Török, B Kliem… - Space Science …, 2020 - Springer
A clear understanding of the nature of the pre-eruptive magnetic field configurations of
Coronal Mass Ejections (CMEs) is required for understanding and eventually predicting …

Quantitative characterization of magnetic flux rope properties for two solar eruption events

W He, Q Hu, C Jiang, J Qiu… - The Astrophysical Journal, 2022 - iopscience.iop.org
In order to bridge the gap between heliospheric and solar observations of coronal mass
ejections (CMEs), one of the key steps is to improve the understanding of their …

The solar cycle dependence of in situ properties of two types of interplanetary CMEs during 1999–2020

X Shi, H Fu, Z Huang, C Ma, L Xia - The Astrophysical Journal, 2022 - iopscience.iop.org
Generally, in situ parameters of interplanetary coronal mass ejections (ICMEs) are analyzed
as a whole, or ICMEs are classified by speed or whether they are with and without magnetic …

Formation of magnetic flux rope during solar eruption. I. Evolution of toroidal flux and reconnection flux

C Jiang, J Chen, A Duan, X Bian, X Wang, J Li… - Frontiers in …, 2021 - frontiersin.org
Magnetic flux ropes (MFRs) constitute the core structure of coronal mass ejections (CMEs),
but hot debates remain on whether the MFR forms before or during solar eruptions …

The hyper-inflation stage in the coronal mass ejection formation: A missing link that connects flares, coronal mass ejections, and shocks in the low corona

LA Balmaceda, A Vourlidas, G Stenborg… - The Astrophysical …, 2022 - iopscience.iop.org
We analyze the formation and three-dimensional (3D) evolution of two coronal mass
ejections (CMEs) and their associated waves in the low corona via a detailed multi …

Acceleration and Expansion of a Coronal Mass Ejection in the High Corona: Role of Magnetic Reconnection

B Zhuang, N Lugaz, M Temmer, T Gou… - The Astrophysical …, 2022 - iopscience.iop.org
The important role played by magnetic reconnection in the early acceleration of coronal
mass ejections (CMEs) has been widely discussed. However, as CMEs may have …

Trajectory Determination for Coronal Ejecta Observed by WISPR/Parker Solar Probe

PC Liewer, J Qiu, P Penteado, JR Hall, A Vourlidas… - Solar Physics, 2020 - Springer
Abstract The Wide-field Imager for Solar Probe (WISPR) onboard the Parker Solar Probe
(PSP), observing in white light, has a fixed angular field of view, extending from 13.5∘ to …

Multi-point study of the energy release and impulsive CME dynamics in an eruptive C7 flare

J Saqri, AM Veronig, ECM Dickson… - Astronomy & …, 2023 - aanda.org
Context. The energy release in eruptive flares and the kinematics of the associated coronal
mass ejections (CMEs) are interlinked and require favorable observing positions as both on …