Magnetic Shear and Cross‐Field Currents: Roles in the Evolution of the Pre–Coronal Mass Ejection Corona [PDF]
Richard Wolfson, Bongani Dlamini
openalex +1 more source
Probing the magnetic topology of coronal mass ejections by means of Ulysses/HI-SCALE energetic particle observations [PDF]
O. Malandraki+2 more
openalex +2 more sources
The Role of Magnetic Skeleton in Solar Flare Filaments Activity
We report an M9.3 flare and filaments activities from NOAA Active Region 11261 that are strongly modulated by the 3D magnetic skeleton. Magnetic field extrapolation from the vector magnetic field suggests complex magnetic connectivity and the existence ...
Juan Guo+9 more
doaj +1 more source
Magnetic noise bursts near the interplanetary shock associated with the coronal mass ejection event on February 21, 1994: The Geotail observations [PDF]
Yongliang Zhang, H. Matsumoto
openalex +1 more source
The effect on the lunar exosphere of a coronal mass ejection passage
[1] Solar wind bombardment onto exposed surfaces in the solar system produces an energetic component to the exospheres about those bodies. The solar wind energy and composition are highly dependent on the origin of the plasma.
R. Killen, D. Hurley, W. Farrell
semanticscholar +1 more source
Observations of the low solar corona in the extreme ultraviolet and in soft X-rays evidence a close relationship of coronal dimmings and coronal mass ejections (CMEs). Dimmings are usually interpreted as places of plasma evacuation during a CME. We characterize a CME by the apparent angular extent of associated dimmings above the solar limb and define ...
Igor Veselovsky+3 more
openaire +1 more source
LASCO/EIT Observations of Coronal Mass Ejections from Large-Scale Filament Channels [PDF]
Simon Plunket+6 more
openalex +1 more source
A Deep Learning Method for Automatic Coronal Mass Ejection Feature Identification
Coronal mass ejections (CMEs), intense solar eruptive phenomena, are the primary drivers of extreme space weather storms on Earth. As space activities become increasingly frequent and infrastructure more reliant on space-based systems, the rapid and ...
P. Yang, H. S. Fu, J. B. Cao, F. Shen
doaj +1 more source
Properties of coronal mass ejections: SOHO LASCO observations from January 1996 to June 1998 [PDF]
O. C. St. Cyr+13 more
openalex +1 more source
Earth's Alfvén Wings Driven by the April 2023 Coronal Mass Ejection
We report a rare regime of Earth's magnetosphere interaction with sub‐Alfvénic solar wind in which the windsock‐like magnetosphere transforms into one with Alfvén wings.
Li‐Jen Chen+35 more
doaj +1 more source