Spatial variation of energy transport mechanisms within solar flare ribbons. [PDF]
Kerr GS +12 more
europepmc +1 more source
Transverse oscillations and an energy source in a strongly magnetized sunspot. [PDF]
Yuan D +14 more
europepmc +1 more source
Investigating the Correlation Between Inclination of Coronal Loops and Solar Flare Activity
The purpose of this research is to investigate changes in the coronal loop structures during the life cycle of a solar flare. Coronal loops are intricate and complicated magnetic features on the solar surface that are the source of large solar flares ...
Mann, John-Paul
core
Can Thermal Nonequilibrium Explain Coronal Loops?
Any successful model of coronal loops must explain a number of observed properties. For warm (approx. 1 MK) loops, these include: 1. excess density, 2. flat temperature profile, 3. super-hydrostatic scale height, 4. unstructured intensity profile, and 5.
Antiochos, Spiro K. +2 more
core
Quality Assessment of Solar EUV Remote Sensing Images Using Multi-Feature Fusion. [PDF]
Dai S +8 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
SuryaBench: Benchmark Dataset for Advancing Machine Learning in Heliophysics and Space Weather Prediction. [PDF]
Roy S +24 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
Numerical Modeling of Prominences and Coronal Rain with the MPI-AMRVAC Code. [PDF]
Liakh V, Jenkins J.
europepmc +1 more source
Spectroscopic Analysis and RHD Modeling of the First Ca II H and H ϵ Flare Spectra from DKIST/ViSP. [PDF]
Tamburri C +9 more
europepmc +1 more source

