We analyze high-cadence vector magnetograms (135 s) and flare-ribbon observations of 37
flares from the Solar Dynamics Observatory to understand the spatial and temporal …

In contemporary astronomy and astrophysics (A&A), the integration of high-performance
computing (HPC), big data analytics, and artificial intelligence/machine learning (AI/ML) has …

Kink oscillations of a curved coronal slab with finite plasma-β, simulating a loop arcade, are
examined. Perpendicular propagation, ie propagation along the arcade axis (ky> 0) is taken …

Coronal mass ejections and high speed solar streams serve as perturbations to the
background solar wind that have major implications in space weather dynamics. Therefore …

In the implosion conjecture, coronal loops contract as the result of magnetic energy release
in solar eruptions and flares. However, after almost two decades, observations of this …

The phenomenon of peripheral coronal loop contraction during solar flares and eruptions,
recently discovered in observations, has gradually drawn the attention of solar physicists …

Resonant absorption is considered to be a crucial mechanism for the damping of the coronal
loop oscillations and plasma heating. We study resonant absorption of the coronal loop kink …

Recently, quasi-periodic propagating disturbances have been detected frequently in
different structures of the solar corona. These propagating disturbances are interpreted as …

Oscillations in various structures of the solar atmosphere, such as transverse (kink)
oscillations of coronal loops, can be used in seismology. Transvers kink oscillations of …