Results 101 to 110 of about 4,375,884 (204)

A Simultaneous Forbush Decrease Associated with an Earthward Coronal Mass Ejection Observed by STEREO

open access: yes, 2012
The intensity–time profile of Forbush decrease (FD) events observed by neutron monitors (NMs) looks like that of a geomagnetic storm as defined by the Dst index. Oh, Yi, and Kim (J. Geophys. Res. 113, A01103, 2008) and Oh and Yi (J. Geophys. Res.
Suyeon Oh, Y. Yi
semanticscholar   +1 more source

The Major Solar Energetic Particle Event on 2024 May 20: Multispacecraft Observations of a Long-lasting Energetic Particle Reservoir

open access: yesThe Astrophysical Journal
The fleet of spacecraft distributed across the inner heliosphere during 2024 May–June provided a unique opportunity to analyze, over a broad range of heliolongitudes, the effects produced by the complex sunspot group associated with Active Region 13664 ...
D. Lario   +28 more
doaj   +1 more source

Study of Plasma Heating Processes in a Coronal Mass Ejection–driven Shock Sheath Region Observed with the Metis Coronagraph

open access: yesThe Astrophysical Journal
On 2021 September 28, a C1.6 class flare occurred in active region NOAA 12871, located approximately at 27°S and 51°W on the solar disk with respect to Earth’s point of view.
Federica Frassati   +27 more
doaj   +1 more source

3D Nonequilibrium Ionization and Spectroscopic Modeling of Coronal Mass Ejections. III. Charge State Evolution

open access: yesThe Astrophysical Journal
The ionization state of plasmas leaving the Sun freezes in low in the solar corona and carries information about the inner corona through the heliosphere.
E. M. Wraback   +3 more
doaj   +1 more source

Observations of a Solar Energetic Particle Event From Inside and Outside the Coma of Comet 67P. [PDF]

open access: yesJ Geophys Res Space Phys, 2022
Wellbrock A   +14 more
europepmc   +1 more source

Imaging and Radio Signatures of Shock–Plasmoid Interaction

open access: yesThe Astrophysical Journal Letters
Understanding how shocks interact with coronal structures is crucial for understanding the mechanisms of particle acceleration in the solar corona and inner heliosphere.
Pankaj Kumar   +3 more
doaj   +1 more source

Magnetosheath Jet Formation Influenced by Parameters in Solar Wind Structures. [PDF]

open access: yesJ Geophys Res Space Phys, 2023
Koller F   +5 more
europepmc   +1 more source

Identification of Coronal Mass Ejection–Driven Shocks Based on Numerical Simulation and Deep Learning

open access: yesThe Astrophysical Journal
Coronal mass ejections (CMEs) are eruptions originating from the solar corona, usually carrying a large amount of fast-flowing plasma into interplanetary space, accompanied by an enhanced magnetic field.
Jing’en Li   +4 more
doaj   +1 more source

Defining the Middle Corona. [PDF]

open access: yesSol Phys, 2023
West MJ   +41 more
europepmc   +1 more source

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