Results 111 to 120 of about 22,597 (264)
Prompt Response of the Dayside Magnetosphere to Discrete Structures Within the Sheath Region of a Coronal Mass Ejection. [PDF]
Blum LW +6 more
europepmc +1 more source
MMS Observations of a Compressed, Strongly Driven Magnetopause During the 2024 Mother's Day Storm
Abstract From 10 to 12 May 2024, a series of coronal mass ejections led to one of the strongest geomagnetic storms of the century, referred to as the Mother's Day or Gannon Storm. MMS's position on the dayside magnetosphere on 11 May provided observations of a strongly driven and compressed ∼7RE $\left(\sim 7\ {R}_{E}\right)$ reconnecting magnetopause.
Jason M. H. Beedle +19 more
wiley +1 more source
Eruption of a plasma blob, associated M-class flare, and large-scale EUV wave observed by SDO
We present a multiwavelength study of the formation and ejection of a plasma blob and associated EUV waves in AR NOAA 11176, observed by SDO/AIA and STEREO on 25 March 2011. SDO/AIA images clearly show the formation and ejection of a plasma blob from the
Kumar, Pankaj, Manoharan, P. K.
core +1 more source
Understanding Interplanetary Coronal Mass Ejection Signatures
While interplanetary coronal mass ejections (ICMEs) are understood to be the heliospheric counterparts of CMEs, with signatures undeniably linked to the CME process, the variability of these signatures and questions about mapping to observed CME features raise issues that remain on the cutting edge of ICME research.
Wimmer-Schweingruber, R.F. +15 more
openaire +3 more sources
Solar Energetic Particle Events During May 2024 Geomagnetic Superstorm
Abstract Three solar energetic particle (SEP) events originating from solar active region 13664 occurred on 10–16 May 2024, coinciding with a geomagnetic superstorm. Using data from the Geostationary Operational Environmental Satellites and Meteorological Operational satellite‐C, we investigate the energetic proton fluxes and east‐west flux ratios in ...
Zhenghao She +7 more
wiley +1 more source
A Workflow-Oriented Approach To Propagation Models In Heliophysics
The Sun is responsible for the eruption of billions of tons of plasma andthe generation of near light-speed particles that propagate throughout the solarsystem and beyond.
Gabriele Pierantoni +4 more
doaj +1 more source
Deflection and Rotation of CMEs from Active Region 11158
Between the 13 and 16 of February 2011 a series of coronal mass ejections (CMEs) erupted from multiple polarity inversion lines within active region 11158.
A. Isavnin +40 more
core +1 more source
Magnetic field and dynamic pressure ULF fluctuations in coronal-mass-ejection-driven sheath regions [PDF]
Emilia Kilpua +4 more
openalex +1 more source
A probabilistic approach to the drag-based model
The forecast of the time of arrival (ToA) of a coronal mass ejection (CME) to Earth is of critical importance for our high-technology society and for any future manned exploration of the Solar System. As critical as the forecast accuracy is the knowledge
Napoletano Gianluca +5 more
doaj +1 more source

