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The physical processes of CME/ICME evolution
As observed in Thomson-scattered white light, coronal mass ejections (CMEs) are manifest
as large-scale expulsions of plasma magnetically driven from the corona in the most …
as large-scale expulsions of plasma magnetically driven from the corona in the most …
Geoeffective properties of solar transients and stream interaction regions
EKJ Kilpua, A Balogh, R Von Steiger, YD Liu - Space Science Reviews, 2017 - Springer
Abstract Interplanetary Coronal Mass Ejections (ICMEs), their possible shocks and sheaths,
and co-rotating interaction regions (CIRs) are the primary large-scale heliospheric structures …
and co-rotating interaction regions (CIRs) are the primary large-scale heliospheric structures …
Near-Earth interplanetary coronal mass ejections during solar cycle 23 (1996–2009): Catalog and summary of properties
IG Richardson, HV Cane - Solar Physics, 2010 - Springer
In a previous study (Cane and Richardson, J. Geophys. Res. 108 (A4), SSH6-1, 2003), we
investigated the occurrence of interplanetary coronal mass ejections in the near-Earth solar …
investigated the occurrence of interplanetary coronal mass ejections in the near-Earth solar …
Observations of an extreme storm in interplanetary space caused by successive coronal mass ejections
Abstract Space weather refers to dynamic conditions on the Sun and in the space
environment of the Earth, which are often driven by solar eruptions and their subsequent …
environment of the Earth, which are often driven by solar eruptions and their subsequent …
Properties of interplanetary coronal mass ejections at one AU during 1995–2004
We present a comprehensive survey of 230 interplanetary CMEs (ICMEs) during 1995–2004
using Wind and ACE in situ observations near one AU, and examine the solar-cycle …
using Wind and ACE in situ observations near one AU, and examine the solar-cycle …
STEREO IMPACT investigation goals, measurements, and data products overview
Abstract The IMPACT (In situ Measurements of Particles And CME Transients) investigation
on the STEREO mission was designed and developed to provide multipoint solar wind and …
on the STEREO mission was designed and developed to provide multipoint solar wind and …
Self-consistent propagation of flux ropes in realistic coronal simulations
L Linan, F Regnault, B Perri, M Brchnelova… - Astronomy & …, 2023 - aanda.org
Context. The text has been edited to adhere to American English based on the spelling style
used in the text. In order to anticipate the geoeffectiveness of coronal mass ejections …
used in the text. In order to anticipate the geoeffectiveness of coronal mass ejections …
Discrepancies in the properties of a coronal mass ejection on scales of 0.03 au as revealed by simultaneous measurements at Solar Orbiter and wind: the 2021 …
Simultaneous in situ measurements of coronal mass ejections (CMEs), including both
plasma and magnetic field, by two spacecraft in radial alignment have been extremely rare …
plasma and magnetic field, by two spacecraft in radial alignment have been extremely rare …
Interplanetary coronal mass ejections from MESSENGER orbital observations at Mercury
We use observations from the MErcury Surface, Space ENvironment, GEochemistry, and
Ranging (MESSENGER) spacecraft, in orbit around Mercury, to investigate interplanetary …
Ranging (MESSENGER) spacecraft, in orbit around Mercury, to investigate interplanetary …
Bulk properties of the slow and fast solar wind and interplanetary coronal mass ejections measured by Ulysses: Three polar orbits of observations
We examined plasma and magnetic field observations from all three Ulysses polar orbits of
the Sun to study the properties of the slow and fast solar wind and interplanetary coronal …
the Sun to study the properties of the slow and fast solar wind and interplanetary coronal …