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 …
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
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 …
transients in the last decade that encompasses most of solar cycle 24. It is a part of the effort …
CME–CME interactions as sources of CME geoeffectiveness: The formation of the complex ejecta and intense geomagnetic storm in 2017 early September
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 …
where their geoeffectiveness is largely determined by their dynamic pressure and internal …
Origins of the ambient solar wind: implications for space weather
SR Cranmer, SE Gibson, P Riley - Space Science Reviews, 2017 - Springer
The Sun's outer atmosphere is heated to temperatures of millions of degrees, and solar
plasma flows out into interplanetary space at supersonic speeds. This paper reviews our …
plasma flows out into interplanetary space at supersonic speeds. This paper reviews our …
Transmission of foreshock waves through Earth's bow shock
The Earth's magnetosphere and its bow shock, which is formed by the interaction of the
supersonic solar wind with the terrestrial magnetic field, constitute a rich natural laboratory …
supersonic solar wind with the terrestrial magnetic field, constitute a rich natural laboratory …
In situ multi-spacecraft and remote imaging observations of the first CME detected by Solar Orbiter and BepiColombo
Context. On 2020 April 19 a coronal mass ejection (CME) was detected in situ by Solar
Orbiter at a heliocentric distance of about 0.8 AU. The CME was later observed in situ on …
Orbiter at a heliocentric distance of about 0.8 AU. The CME was later observed in situ on …
A Quarter Century of Wind Spacecraft Discoveries
LB Wilson III, AL Brosius, N Gopalswamy… - 2021 - Wiley Online Library
The Wind spacecraft, launched on November 1, 1994, is a critical element in NASA's
Heliophysics System Observatory (HSO)—a fleet of spacecraft created to understand the …
Heliophysics System Observatory (HSO)—a fleet of spacecraft created to understand the …
The response of Earth's electron radiation belts to geomagnetic storms: Statistics from the Van Allen Probes era including effects from different storm drivers
A statistical study was conducted of Earth's radiation belt electron response to geomagnetic
storms using NASA's Van Allen Probes mission. Data for electrons with energies ranging …
storms using NASA's Van Allen Probes mission. Data for electrons with energies ranging …
Geoeffectiveness of interplanetary Alfvén waves. I. Magnetopause magnetic reconnection and directly driven substorms
L Dai, Y Han, C Wang, S Yao, W Gonzalez… - The Astrophysical …, 2023 - iopscience.iop.org
In particular during the descending phase of the solar cycle, Alfvén waves in the high-speed
solar wind streams are a major form of interplanetary disturbances. The fluctuating …
solar wind streams are a major form of interplanetary disturbances. The fluctuating …
Observation-based modelling of magnetised coronal mass ejections with EUHFORIA
C Scolini, L Rodriguez, M Mierla, J Pomoell… - Astronomy & …, 2019 - aanda.org
Context. Coronal mass ejections (CMEs) are the primary source of strong space weather
disturbances at Earth. Their geo-effectiveness is largely determined by their dynamic …
disturbances at Earth. Their geo-effectiveness is largely determined by their dynamic …