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: 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 …

CME–CME interactions as sources of CME geoeffectiveness: The formation of the complex ejecta and intense geomagnetic storm in 2017 early September

C Scolini, E Chané, M Temmer… - The Astrophysical …, 2020 - iopscience.iop.org
Coronal mass ejections (CMEs) are the primary sources of intense disturbances at Earth,
where their geoeffectiveness is largely determined by their dynamic pressure and internal …

Rotation and interaction of the CMEs of September 8 and 10, 2014, tested with EUHFORIA

A Maharana, C Scolini, B Schmieder… - Astronomy & …, 2023 - aanda.org
Context. Solar coronal mass ejections (CMEs) can catch up and interact with preceding
CMEs and solar wind structures to undergo rotation and deflection during their propagation …

The GIC and geomagnetic response over Fennoscandia to the 7–8 September 2017 geomagnetic storm

AP Dimmock, L Rosenqvist, JO Hall, A Viljanen… - Space …, 2019 - Wiley Online Library
Abstract Between 7 and 8 September 2017, Earth experienced extreme space weather
events. We have combined measurements made by the IMAGE magnetometer array …

Merging of storm time midlatitude traveling ionospheric disturbances and equatorial plasma bubbles

E Aa, S Zou, A Ridley, S Zhang, AJ Coster… - Space …, 2019 - Wiley Online Library
Postsunset midlatitude traveling ionospheric disturbances (TIDs) and equatorial plasma
bubbles (EPBs) were simultaneously observed over American sector during the …

Eruption of a multi-flux-rope system in solar active region 12673 leading to the two largest flares in Solar Cycle 24

YJ Hou, J Zhang, T Li, SH Yang, XH Li - Astronomy & Astrophysics, 2018 - aanda.org
Context. Solar active region (AR) 12673 in 2017 September produced the two largest flares
in Solar Cycle 24: the X9. 3 flare on September 6 and the X8. 2 flare on September 10. Aims …

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 …

ICME evolution in the inner heliosphere: Invited review

JG Luhmann, N Gopalswamy, LK Jian, N Lugaz - Solar Physics, 2020 - Springer
ICMEs (interplanetary coronal mass ejections), the heliospheric counterparts of what is
observed with coronagraphs at the Sun as CMEs, have been the subject of intense interest …

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 …