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 …

The Sun and space weather

N Gopalswamy - Atmosphere, 2022 - mdpi.com
The explosion of space weather research since the early 1990s has been partly fueled by
the unprecedented, uniform, and extended observations of solar disturbances from space …

Properties and geoeffectiveness of solar wind high‐speed streams and stream interaction regions during solar cycles 23 and 24

M Grandin, AT Aikio, A Kozlovsky - Journal of Geophysical …, 2019 - Wiley Online Library
We study the properties and geoeffectiveness of solar wind high‐speed streams (HSSs)
emanating from coronal holes and associated with stream interaction regions (SIRs). This …

Corotating interaction regions during solar cycle 24: A study on characteristics and geoeffectiveness

R Hajra, JV Sunny - Solar Physics, 2022 - Springer
Corotating interaction regions (CIRs) form in the interaction region between the solar-wind
high-speed streams and slow streams, leading to compressed plasma and magnetic fields …

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 …

[HTML][HTML] Predictability of variable solar–terrestrial coupling

IA Daglis, LC Chang, S Dasso… - Annales …, 2021 - angeo.copernicus.org
Abstract In October 2017, the Scientific Committee on Solar-Terrestrial Physics (SCOSTEP)
Bureau established a committee for the design of SCOSTEP's Next Scientific Programme …

The unusual widespread solar energetic particle event on 2013 August 19-Solar origin and particle longitudinal distribution

L Rodriguez-Garcia, R Gomez-Herrero… - Astronomy & …, 2021 - aanda.org
Context. Late on 2013 August 19, STEREO-A, STEREO-B, MESSENGER, Mars Odyssey,
and the L1 spacecraft, spanning a longitudinal range of 222° in the ecliptic plane, observed …

Association of the Main Phase of the Geomagnetic Storms in Solar Cycles 23 and 24 With Corresponding Solar Wind‐IMF Parameters

V Manu, N Balan, QH Zhang… - Journal of Geophysical …, 2022 - Wiley Online Library
The occurrence and intensity of the geomagnetic storms/activity in the weak solar cycle 24
(SC24) were studied mainly for low latitudes, with intensity being the maximum value of the …

The possible cause of most intense geomagnetic superstorm of the 21st century on 20 november 2003

A Raghav, Z Shaikh, P Vemareddy, A Bhaskar… - Solar Physics, 2023 - Springer
An extreme geomagnetic storm has the potential to affect various technologies and activities
in space and on the ground, eg, power grids, oil and gas industries, communications …