Results 101 to 110 of about 4,375,884 (204)
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 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
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
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]
Wellbrock A +14 more
europepmc +1 more source
Imaging and Radio Signatures of Shock–Plasmoid Interaction
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]
Koller F +5 more
europepmc +1 more source
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
How Magnetic Erosion Affects the Drag-Based Kinematics of Fast Coronal Mass Ejections. [PDF]
Stamkos S +3 more
europepmc +1 more source

