Results 191 to 200 of about 54,745 (274)

Cosmic ray and geomagnetic response to radio-loud coronal mass ejections (CMEs)

, 2013
213-218A catalog of type II bursts observed by the Radio and Plasma waves (WAVES) experiments onboard the wind space craft and the associated coronal mass ejections (CMEs) observed by the Solar and Heliospheric Observatory (SOHO) mission are used to ...
Sharma, N K
core  

Simulating Coronal Mass Ejections in the Heliosphere

, 2008
Coronal mass ejections (CMEs) and their attendant eruptive flares (EFs) are the most explosive events in the solar system. Magnetic reconnection, arguably the most universal of heliophysical processes, is widely accepted as playing crucial roles in these
Antiochos, Spiro K., DeVore, Richard C.
core  

MHD shocks in coronal mass ejections

, 1991
The primary objective of this research program is the study of the magnetohydrodynamic (MHD) shocks and nonlinear simple waves produced as a result of the interaction of ejected lower coronal plasma with the ambient corona.
Steinolfson, R. S.
core  

Associations between coronal mass ejections and interplanetary shocks

, 1983
Nearly continuous complementary coronal observations and interplanetary plasma measurements for the years 1979-1982 are compared. It is shown that almost all low latitude high speed coronal mass ejections (CME's) were associated with shocks at HELIOS 1 ...
Muhlhauser, K. H., Howard, R. A., Michels, D. J., Schwenn, R., Sheeley, N. R., Jr., Rosenbauer, H., Koomen, M. J.   +6 more
core  

The Sun as a driver of the inner heliosphere: Modern investigations of fundamental plasma processes. [PDF]

Nat Commun
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]

Sci Rep
Vasanth V.
europepmc   +1 more source

Magnetoacoustic wave propagation in the solar corona and filament dynamics. [PDF]

Sci Rep
Somaiyeh S, Stefaan P.
europepmc   +1 more source

Simulating high-speed solar wind streams from coronal holes using an L5-L1 configuration of lagrangian points. [PDF]

Sci Rep
Podladchikova T, Veronig AM, Temmer M, Hofmeister SJ.   +3 more
europepmc   +1 more source

Revealing Flare Energetics and Dynamics with SDO EVE Solar Extreme Ultraviolet Spectral Irradiance Observations. [PDF]

Sol Phys
Woods TN, Chamberlin PC, Jones A, Mason JP, Qian L, Warren HP, Woodraska D, Borelli R, Eparvier FG, Gonzalez G.   +9 more
europepmc   +1 more source

Global ozone loss following extreme solar proton storms based on the July 2012 coronal mass ejection. [PDF]

Sci Rep, 2023
Kalakoski N, Verronen PT, Szeląg ME, Jackman CH.   +3 more
europepmc   +1 more source