Results 81 to 90 of about 1,080,647 (142)
Topological structure of the magnetic solar corona [PDF]
The solar corona is a highly complex and active plasma environment, containing many exotic phenomena such as solar flares, coronal mass ejections, prominences, coronal loops, and bright points.
Maclean, Rhona Claire
core +2 more sources
Coronal oscillations offer insight into energy transport and driving in the solar atmosphere. Knowing its polarization state helps constrain a wave’s displacement and velocity amplitude, improving estimates of wave energy flux and deposition rate.
T. J. Duckenfield +3 more
doaj +1 more source
Coronal seismology and pulsations of microwave emission from solar flares [PDF]
Y. G. Kopylova +2 more
openaire +1 more source
A Large-Scale Dataset of Three-Dimensional Solar Magnetic Fields Extrapolated by Nonlinear Force-Free Method. [PDF]
Zhao Z +7 more
europepmc +1 more source
Unprecedented 19 Day Type IV Radio Burst as a Corotating Electron Reservoir
We report a hectometric (0.5–3 MHz) type IV continuum observed over nearly 19 days (2025 August 21–September 9) in three successive visibility windows as the source corotates with the Sun—first at Solar Orbiter, then 12 days later in the near-Earth ...
Vratislav Krupar +13 more
doaj +1 more source
Transverse oscillations and an energy source in a strongly magnetized sunspot. [PDF]
Yuan D +14 more
europepmc +1 more source
Context. Little attention has been paid to group velocities of three-dimensional (3D) magnetohydrodynamic (MHD) waves in solar coronal seismology. Aims.
Liu Jing +4 more
doaj +1 more source
Coronal seismology using transverse loop oscillations [PDF]
Coronal seismology exploits the properties of magnetohydrodynamics in the corona of the Sun to diagnose the local plasma. Therefore, seismology complements direct diagnostic techniques, which suffer from line-of-sight integration or may not give access ...
Verwichte, E. +9 more
core +1 more source
Electron transport in a radiation-dominated plasma
Context. Bremsstrahlung scattering of fast electrons on ions can be enhanced by the microwave radiation present in the solar corona. It can account for the electron diffusive transport along magnetic loops and high precipitation rates.
Duclous R. +5 more
doaj +1 more source
Large scale coherent magnetohydrodynamic oscillations in a sunspot. [PDF]
Stangalini M +13 more
europepmc +1 more source

