Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]
Veronig AM +12 more
europepmc +2 more sources
The environment of the sun during the explosion of Coronal Mass Ejections (CMEs) on 2nd May 2016
Coronal Mass Ejections (CMEs) have been studied has become the most important phenomena of solar activity because it is the most energetic phenomena on the Sun. Concerning the importance of the impact of solar radio burst, we study the selected event of CMEs to observe the environment of the atmosphere of the Sun.
Hamidi, Z.S. +3 more
openaire +1 more source
How Magnetic Erosion Affects the Drag-Based Kinematics of Fast Coronal Mass Ejections. [PDF]
Stamkos S +3 more
europepmc +1 more source
Magnetosheath Jet Formation Influenced by Parameters in Solar Wind Structures. [PDF]
Koller F +5 more
europepmc +1 more source
Observations of successive CMEs and their successive Type II solar radio bursts in the corona. [PDF]
Vasanth V.
europepmc +1 more source
Magnetoacoustic wave propagation in the solar corona and filament dynamics. [PDF]
Somaiyeh S, Stefaan P.
europepmc +1 more source
Integration of solar flare and coronal mass ejection event data. [PDF]
Ji A, Georgoulis MK, Aydin B.
europepmc +1 more source
Evaluating Solar Wind Forecast Using Magnetic Maps That Include Helioseismic Far-Side Information. [PDF]
Heinemann SG +7 more
europepmc +1 more source
Multiwavelength Multipoint Observations of the October 28, 2021 Type III Radio Burst. [PDF]
Martinez Oliveros JC +8 more
europepmc +1 more source
Observations of a Solar Energetic Particle Event From Inside and Outside the Coma of Comet 67P. [PDF]
Wellbrock A +14 more
europepmc +1 more source

