Results 111 to 120 of about 3,305 (196)
Although multiscale filament eruptions serve as significant triggers for various energetic release processes in the solar atmosphere, the underlying mechanisms remain elusive.
Liping Yang +13 more
doaj +1 more source
Ultra-high-resolution observations of persistent null-point reconnection in the solar corona. [PDF]
Cheng X +23 more
europepmc +1 more source
The southward component of the interplanetary magnetic field, often originating from solar coronal mass ejections (CMEs), plays a crucial role in driving geomagnetic storms. Accurate prediction of the flux rope orientation of CMEs as they arrive at Earth
Ying Wang +6 more
doaj +1 more source
The Kinematical Behavior of Solar Eruptive Filaments Affected by the Poloidal Magnetic Field
Kinematics of solar eruptive filaments is one of the important diagnostic parameters for predicting whether solar eruptions would induce geomagnetic storms.
Ye Qiu +5 more
doaj +1 more source
Diverse glasses revealed from Chang'E-5 lunar regolith. [PDF]
Zhao R +15 more
europepmc +1 more source
Large-scale Coronal Dimming Foreshadowing a Solar Eruption on 2011 October 1
Understanding large-scale solar eruptions requires detailed investigation of the entire system’s evolution, including the magnetic environment enveloping the source region and searches for precursor activity prior to event onset.
Chunming Zhu +6 more
doaj +1 more source
Data-driven modeling of solar coronal magnetic field evolution and eruptions. [PDF]
Jiang C, Feng X, Guo Y, Hu Q.
europepmc +1 more source
Minifilaments are widespread small-scale structures in the solar atmosphere. To better understand their formation and eruption mechanisms, we investigate the entire life of a sigmoidal minifilament located below a large quiescent filament observed by Big
Weilin Teng +8 more
doaj +1 more source
The SWAP Filter: A Simple Azimuthally Varying Radial Filter for Wide-Field EUV Solar Images. [PDF]
Seaton DB +7 more
europepmc +1 more source

