A Unified Picture of Swirl-driven Solar Coronal Heating: Magnetic Energy Supply and Dissipation
The coronal heating problem is one of the most critical challenges in solar physics. Recent observations have revealed that small-scale swirls are ubiquitous in the photosphere and chromosphere, suggesting that they may play a significant role in ...
Hidetaka Kuniyoshi +2 more
doaj +1 more source
The role and contribution of magnetic fields, characterized via their magnetic flux, to the statistical structuring of the solar atmosphere. [PDF]
Li KJ, Xu JC, Feng W.
europepmc +1 more source
Solar Doppler Velocity Results from the SDO EVE Level 4 Lines Data Product. [PDF]
Woods TN +6 more
europepmc +1 more source
Historical records in solar physics. [PDF]
Chatzistergos T.
europepmc +1 more source
Potential Solar Precursors to Magnetic Switchbacks. [PDF]
Tripathi D +11 more
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
Can Small-scale Eruptions in the Quiet Sun Propagate into the Higher Solar Corona?
Abstarct Recent research has revealed that small-scale coronal mass ejections (CMEs) in the quiet Sun exhibit similarities in their formation mechanisms and eruption characteristics when compared to large-scale solar eruptions. The occurence of small-scale CMEs increases exponentially as their size decreases.
openaire +1 more source
Investigating the Relationship Between Physical Properties and Spatial Irregularities at Coronal Hole Boundaries. [PDF]
Ngampoopun N +7 more
europepmc +1 more source
Study on the relation of the solar coronal rotation with magnetic field structures. [PDF]
Xiang NB +4 more
europepmc +1 more source

