Results 101 to 110 of about 11,117 (189)
Dynamics of An Erupting Filament and a Coronal Loop during Their Interaction
Although interactions between filaments and other atmospheric structures are frequently observed, detailed studies on how these interactions affect the dynamics of the involved structures remain scarce.
Yue Fang +3 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
The SWAP Filter: A Simple Azimuthally Varying Radial Filter for Wide-Field EUV Solar Images. [PDF]
Seaton DB +7 more
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
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
Observation and modelling of solar jets. [PDF]
Shen Y.
europepmc +1 more source

