Results 141 to 150 of about 881 (218)
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
30-min decayless kink oscillations in a very long bundle of solar coronal plasma loops. [PDF]
Zhong S +4 more
europepmc +1 more source
Using high-spatiotemporal-resolution multiwavelength observations from the New Vacuum Solar Telescope and the Solar Dynamics Observatory, we present a detailed analysis of a small-scale chromospheric jet driven by plasmoid-mediated magnetic reconnection.
Zehao Tang +5 more
doaj +1 more source
Fast plasmoid-mediated reconnection in a solar flare. [PDF]
Yan X +10 more
europepmc +1 more source
The chromosphere is an intermediate layer of the Sun's atmosphere where radiative equilibrium breaks down. The standard chromospheric diagnostics such as the Mg II h and k and Ca II H and K spectral lines are formed under nonlocal thermodynamic ...
da Silva Santos, João Manuel
core
Observation and modelling of solar jets. [PDF]
Shen Y.
europepmc +1 more source
Influence of ambipolar and Hall effects on vorticity in three-dimensional simulations of magneto-convection. [PDF]
Khomenko E +3 more
europepmc +1 more source
Five Solar Cycles of Solar Corona Investigations. [PDF]
Antonucci E.
europepmc +1 more source
Magnetohydrodynamic waves in structured atmospheres
The effect of structuring, in the form of magnetic or density inhomogeneities, on the magnetohydrodynamic (mhd) waves of an infinite plasma is investigated.
Edwin, Patricia Mary
core
The chromosphere is an intermediate layer of the Sun's atmosphere where radiative equilibrium breaks down. The standard chromospheric diagnostics such as the Mg II h and k and Ca II H and K spectral lines are formed under nonlocal thermodynamic ...
Heinzel, Petr, +3 more
core

