Results 101 to 110 of about 260,299 (222)
Deceleration observed in the coronal mass ejection event of July 25, 1999
En el presente trabajo presentamos diagramas altura-tiempo de la eyección de masa coronal tipo halo observada en julio 25, 1999 con el Coronógrafo Espectroscópico y de Gran Ángulo (LASCO), a bordo del satélite Observatorio Heliosférico y Solar (SOHO ...
A. A. Dal Lago+8 more
doaj +1 more source
The Distribution of Linear Virgae Across the Saturnian Moons
Abstract Linear virgae are long (10–100s km), narrow (<5 km), and bright features, first found on the surface of Dione. On Dione, linear virgae run parallel to the equator and are found in the low‐to‐mid latitudes. Linear virgae are likely formed by a process that involves the emplacement of materials from an exogenic Chronocentric (Saturn centric), or
E. S. Martin+5 more
wiley +1 more source
LASCO/EIT Observations of Coronal Mass Ejections from Large-Scale Filament Channels [PDF]
Simon Plunket+6 more
openalex +1 more source
Abstract On 24 April 2023, an ICME reached Earth's orbit. The solar wind density dropped to 0.3 amu/cc while the IMF strength was about 25 nT. As a result, the solar wind flow transitions to a sub‐Alfvénic state with an Alfvén Mach number of 0.4. We carry out global magnetohydrodynamic simulations to investigate the responses of Earth's magnetosphere ...
Yuxi Chen+4 more
wiley +1 more source
Probing the magnetic topology of coronal mass ejections by means of Ulysses/HI-SCALE energetic particle observations [PDF]
O. Malandraki+2 more
openalex +2 more sources
Earth's Alfvén Wings Driven by the April 2023 Coronal Mass Ejection
We report a rare regime of Earth's magnetosphere interaction with sub‐Alfvénic solar wind in which the windsock‐like magnetosphere transforms into one with Alfvén wings.
Li‐Jen Chen+35 more
doaj +1 more source
Anisotropic Heating and Cooling within Interplanetary Coronal Mass Ejection Sheath Plasma
This study presents the first comprehensive investigation of the relationship between heating and cooling, temperature anisotropy, turbulence level, and collisional age within interplanetary coronal mass ejection (ICME) sheaths, which are highly ...
Zubair I. Shaikh+5 more
doaj +1 more source
Location of the activity responsible for the appearance of coronal mass ejections and the sites of their ejection from the solar surface [PDF]
N. S. Shilova
openalex +1 more source
Solar and Heliospheric ObservatoryObservations of a Helical Coronal Mass Ejection [PDF]
A. Ciaravella+10 more
openalex +1 more source