A solar storm observed from the Sun to Venus using the STEREO, Venus Express, and MESSENGER spacecraft [PDF]
, 2009 The suite of SECCHI optical imaging instruments on the STEREO-A spacecraft is used to track a solar storm, consisting of several coronal mass ejections (CMEs) and other coronal loops, as it propagates from the Sun into the heliosphere during May 2007 ...
Anderson, B. +25 more
core +6 more sources
Geomagnetic storms driven by ICME- and CIR-dominated solar wind. [PDF]
, 2006 The interaction of the solar wind and the Earth's magnetosphere is complex and the phenomenology of the interaction is very different for solar wind dominated by interplanetary coronal mass ejections (ICMEs) compared to solar wind dominated by corotating
Liemohn, M. W. +8 more
core +5 more sources
First imaging of corotating interaction regions using the STEREO spacecraft [PDF]
, 2008 Plasma parcels are observed propagating from the Sun out to the large coronal heights monitored by the Heliospheric Imagers (HI) instruments onboard the NASA STEREO spacecraft during September 2007. The source region of these out-flowing parcels is found
Eyles, C. J. +11 more
core +6 more sources
Multiple regions of shock-accelerated particles during a solar coronal mass ejection [PDF]
Nature Astronomy, 2019 The Sun is an active star that can launch large eruptions of magnetized plasma into the heliosphere, known as coronal mass ejections (CMEs). These can drive shocks that accelerate particles to high energies, often resulting in radio emission at low ...
D. Morosan +10 more
semanticscholar +1 more source
The Efficiency of Electron Acceleration by ICME-driven Shocks
The Astrophysical Journal, 2023 We present a study of the efficiency of the acceleration of suprathermal electrons at collisionless shock waves driven by interplanetary coronal mass ejections (ICMEs), with the data analysis from both the spacecraft observations and test-particle ...
G. Qin, F.-J. Kong, S.-S. Wu
doaj +1 more source
Modeling Solar Energetic Neutral Atoms from Solar Flares and CME-driven Shocks
The Astrophysical Journal, 2023 We examine the production of energetic neutral atoms (ENAs) in solar flares and coronal mass ejection (CME)-driven shocks and their subsequent propagation to 1 au. Time profiles and fluence spectra of solar ENAs at 1 au are computed for two scenarios: (1)
Gang Li +7 more
doaj +1 more source
Particle acceleration and coronal mass ejection driven shocks: Shocks of arbitrary strength
Journal of Geophysical Research: Space Physics, 2003 Gary P. Zank, Gang Li, W K M Rice
exaly +2 more sources
Radio Observations of Coronal Mass Ejection Initiation and Development in the Low Solar Corona
Frontiers in Astronomy and Space Sciences, 2020 Coronal mass ejections (CMEs) are large eruptions of plasma and magnetic field from the low solar corona into the heliosphere. These eruptions are often associated with energetic electrons that produce various kinds of radio emission.
E. Carley, N. Vilmer, A. Vourlidas
semanticscholar +1 more source
Statistical Analysis of Magnetic Field Fluctuations in Coronal Mass Ejection-Driven Sheath Regions
Frontiers in Astronomy and Space Sciences, 2021 We report a statistical analysis of magnetic field fluctuations in 79 coronal mass ejection- (CME-) driven sheath regions that were observed in the near-Earth solar wind.
E. Kilpua +7 more
semanticscholar +1 more source
Simultaneous interplanetary scintillation and Heliospheric Imager observations of a coronal mass ejection [PDF]
, 2008 We describe simultaneous Interplanetary Scintillation (IPS) and STEREO Heliospheric Imager (HI) observations of a coronal mass ejection (CME) on 16 May 2007. Strong CME signatures were present throughout the IPS observation.
Davies, Jackie +5 more
core +6 more sources