Results 171 to 180 of about 65,282 (317)
The shape and dynamics of coronal mass ejections (CMEs) vary significantly based on the instrument and wavelength used. This has led to significant debate about the proper definitions of CME/shock fronts, pile-up/compression regions, and core ...
Stepanyuk Oleg, Kozarev Kamen
doaj +1 more source
Which Upstream Solar Wind Conditions Matter Most in Predicting Bz within Coronal Mass Ejections
Pete Riley +2 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
Anisotropic Heating and Cooling within Interplanetary Coronal Mass Ejection Sheath Plasma
This study presents the first comprehensive investigation of the relationship between heating and cooling, temperature anisotropy, turbulence level, and collisional age within interplanetary coronal mass ejection (ICME) sheaths, which are highly ...
Zubair I. Shaikh +5 more
doaj +1 more source
Interactions Between Coronal Mass Ejections
This work is supported by the NSF-REU Solar Physics program at SAO, grant number AGS-1850750.
openaire +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
Editorial: Magnetic Flux Ropes: From the Sun to the Earth and Beyond
Rui Liu +6 more
doaj +1 more source
LINKING REMOTE IMAGERY OF A CORONAL MASS EJECTION TO ITS IN SITU SIGNATURES AT 1 AU [PDF]
Christian Möstl +7 more
openalex +1 more source

