Results 121 to 130 of about 16,204 (260)

Transport in the interplanetary medium of coronal mass ejections [PDF]

open access: yesGeofísica Internacional, 2008
Coronal mass ejections (CMEs) are large scale structures of plasma and magnetic field expelled from the Sun to the interplanetary medium and generally observed in white light coronagraphs.
A. Ventura, A. Lara, A. Borgazzi
doaj  

PECULIARITIES OF THE MICROWAVE EMISSION BEHAVIOR IN SOLAR ACTIVE REGIONS BEFORE CORONAL MASS EJECTIONS

open access: gold, 2020
I. A. Bakunina   +7 more
openalex   +1 more source

Automatic Detection of Interplanetary Coronal Mass Ejections in Solar Wind In Situ Data [PDF]

open access: diamond, 2022
Hannah T. Rüdisser   +6 more
openalex   +1 more source

Behavior of Flare-associated Suprathermal Ions at Coronal Mass Ejections observed with Solar Orbiter at 0.5 AU

open access: gold, 2023
Nils Janitzek   +16 more
openalex   +1 more source

Discrepancies in the Properties of a Coronal Mass Ejection on Scales of 0.03 au as Revealed by Simultaneous Measurements at Solar Orbiter and Wind: The 2021 November 3–5 Event

open access: yesThe Astrophysical Journal
Simultaneous in situ measurements of coronal mass ejections (CMEs), including both plasma and magnetic field, by two spacecraft in radial alignment have been extremely rare.
F. Regnault   +6 more
doaj   +1 more source

3D Non-equilibrium Ionization and Spectroscopic Modeling of Coronal Mass Ejections. II. CME Energy Budget

open access: yesThe Astrophysical Journal
Coronal mass ejections (CMEs) release between ≈10 ^30 and 10 ^33 erg of energy into the corona; however, their detailed energy budget is difficult to constrain.
E. M. Wraback   +3 more
doaj   +1 more source

Understanding the Effects of Spacecraft Trajectories through Solar Coronal Mass Ejection Flux Ropes Using 3DCOREweb [PDF]

open access: gold
Hannah T. Rüdisser   +6 more
openalex   +2 more sources

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