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 …

Causality in heliophysics: magnetic fields as a bridge between the Sun's interior and the Earth's space environment

D Nandy, Y Baruah, P Bhowmik, S Dash… - Journal of Atmospheric …, 2023 - Elsevier
Our host star, the Sun, is a middle-aged main sequence G type star whose activity varies.
These variations are primarily governed by solar magnetic fields which are produced in the …

Propagation characteristics of coronal mass ejections (CMEs) in the corona and interplanetary space

F Shen, C Shen, M Xu, Y Liu, X Feng… - Reviews of Modern Plasma …, 2022 - Springer
Coronal mass ejections (CMEs) play an important role in space weather. The propagation
characteristics of CMEs in the Corona and interplanetary space determine whether, when …

Magnetoacoustic wave propagation in the solar corona and filament dynamics

S Somaiyeh, P Stefaan - Scientific Reports, 2024 - nature.com
The formation of a S-shaped filament was investigated to determine if and how
magnetoacoustic waves in the solar corona can trigger filament excitation. The study …

Characteristics and applications of interplanetary coronal mass ejection composition

HQ Song, S Yao - Science China Technological Sciences, 2020 - Springer
In situ measurements of interplanetary coronal mass ejection (ICME) composition, including
elemental abundances and charge states of heavy ions, open a new avenue to study …

Comparison of I-ICME and M-ICME Fittings and In Situ Observation Parameters for Solar Cycles 23 and 24 and Their Influence on Geoeffectiveness

Z Zhang, C Shen, Y Chi, D Mao, J Liu, M Xu, Z Zhong… - Solar Physics, 2023 - Springer
To understand the weaker geomagnetic activity in Solar Cycle 24, we present comparisons
of interplanetary coronal mass ejections (ICMEs) fittings and in situ observation parameters …

Origin of Extremely Intense Southward Component of Magnetic Field (B s ) in ICMEs

C Shen, Y Chi, M Xu, Y Wang - Frontiers in Physics, 2021 - frontiersin.org
The intensity of the southward component of the magnetic field (B s) carried by
Interplanetary Coronal Mass Ejections (ICMEs) is one of the most critical parameters in …

Relationships between interplanetary coronal mass ejection characteristics and geoeffectiveness in the declining phase of Solar Cycles 23 and 24

MB Lawrance, YJ Moon, A Shanmugaraju - Solar Physics, 2020 - Springer
In this paper, we have examined the relationships between the characteristics of
interplanetary coronal mass ejections (ICMEs) and geoeffectiveness in the declining phase …

Some Features of Interacting Solar Wind Disturbances

NS Shlyk, AV Belov, MA Abunina, SM Belov… - Geomagnetism and …, 2024 - Springer
The updated database of Forbush effects and interplanetary disturbances (https://tools.
izmiran. ru/feid) is used for an extensive analysis of various characteristics of events caused …

The Inhomogeneity of Composition Along the Magnetic Cloud Axis

H Song, Q Hu, X Cheng, J Zhang, L Li, A Zhao… - Frontiers in …, 2021 - frontiersin.org
Coronal mass ejections (CMEs) are one of the most energetic explosions in the solar
system. It is generally accepted that CMEs result from eruptions of magnetic flux ropes …