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
core +5 more sources
Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]
Veronig AM +12 more
europepmc +2 more sources
How Magnetic Erosion Affects the Drag-Based Kinematics of Fast Coronal Mass Ejections. [PDF]
Stamkos S +3 more
europepmc +1 more source
The Sun as a driver of the inner heliosphere: Modern investigations of fundamental plasma processes. [PDF]
Ervin T, Nakhleh AJ, Bharati Das S.
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
Revealing Flare Energetics and Dynamics with SDO EVE Solar Extreme Ultraviolet Spectral Irradiance Observations. [PDF]
Woods TN +9 more
europepmc +1 more source
Magnetosheath Jet Formation Influenced by Parameters in Solar Wind Structures. [PDF]
Koller F +5 more
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

