Results 151 to 160 of about 65,282 (317)
, 2015 The process by which the Sun affects the terrestrial environment on short timescales is predominately driven by the amount of magnetic reconnection between the solar wind and Earth's magnetosphere. Reconnection occurs most efficiently when the solar wind
Evans, R. +8 more
core +1 more source
Understanding Interplanetary Coronal Mass Ejection Signatures
, 2006 While interplanetary coronal mass ejections (ICMEs) are understood to be the heliospheric counterparts of CMEs, with signatures undeniably linked to the CME process, the variability of these signatures and questions about mapping to observed CME features raise issues that remain on the cutting edge of ICME research.
Wimmer-Schweingruber, R.F. +15 more
openaire +3 more sources
Segmentation and Tracking of Eruptive Solar Phenomena With Convolutional Neural Networks
Journal of Geophysical Research: Machine Learning and Computation, Volume 3, Issue 1, February 2026.Abstract Solar eruptive events are complex phenomena, which most often include coronal mass ejections (CME), CME‐driven compressive and shock waves, flares, and filament eruptions. CMEs are large eruptions of magnetized plasma from the Sun's outer atmosphere or corona, that propagate outward into the interplanetary space.
Oleg Stepanyuk, Kamen Kozarev
wiley +1 more source
Solar Sources of Interplanetary Magnetic Clouds Leading to Helicity Prediction
, 2018 This study identifies the solar origins of magnetic clouds that are observed at 1 AU and predicts the helical handedness of these clouds from the solar surface magnetic fields.
Riley, Pete, Tran, T., Ulrich, Roger K.
core +2 more sources
SCALING RELATIONS IN CORONAL MASS EJECTIONS AND ENERGETIC PROTON EVENTS ASSOCIATED WITH SOLAR SUPERFLARES [PDF]
, 2016 Takuya Takahashi +2 more
openalex +1 more source
MAVEN EUVM Data Products for Space Weather at Mars
Space Weather, Volume 24, Issue 2, February 2026.Abstract Space weather monitoring is critical to protect not only our technological assets in space, but also mitigate disruptions to life and society that depends on these vulnerable assets. Significant attention and resources have been dedicated to space weather monitoring at Earth, but little attention to date has been paid to planetary space ...
P. C. Chamberlin +9 more
wiley +1 more source
A Workflow-Oriented Approach To Propagation Models In Heliophysics
Computer Science, 2014 The Sun is responsible for the eruption of billions of tons of plasma andthe generation of near light-speed particles that propagate throughout the solarsystem and beyond.
Gabriele Pierantoni +4 more
doaj +1 more source
Modeling of transient disturbances in coronal-streamer configurations [PDF]
, 1983 Numerical simulations of the formation and propagation of mass ejection, loop transients in coronal streamers are discussed. The simulations are accomplished with numerical solutions of the single fluid, ideal MHD equations of motion in the meridional ...
Steinolfson, R. S.
core +1 more source
Using the Coronal Evolution to Successfully Forward Model CMEs' In Situ Magnetic Profiles
, 2017 Predicting the effects of a coronal mass ejection (CME) impact requires knowing if impact will occur, which part of the CME impacts, and its magnetic properties. We explore the relation between CME deflections and rotations, which change the position and
Gopalswamy, N., Kay, C.
core +1 more source