There is considerable observational evidence of implosion of magnetic loop systems inside
solar coronal active regions following high-energy events like solar flares. In this work, we …

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

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 …

Coronal implosions—the convergence motion of plasmas and entrained magnetic field in
the corona due to a reduction in magnetic pressure—can help to locate and track sites of …

Eruptive flares are sudden releases of magnetic energy that involve many phenomena,
several of which can be explained by the standard 2D flare model and its realizations in 3D …

We present the observations of the contraction of the extreme-ultraviolet coronal loops
overlying the flaring region during the preheating as well as the early impulsive phase of a …

Context. Coronal and interplanetary shock waves produced by coronal mass ejections
(CMEs) are major drivers of space-weather phenomena, inducing major changes in the …

We study the relationship between implosive motions in a solar flare, and the energy
redistribution in the form of oscillatory structures and particle acceleration. The flare …

We study the MHD processes related to a flare/CME event in the lower solar corona using
numerical simulations. Our initial state is an isothermal gravitationally stratified corona with …

In this Letter, we study in detail the evolution of the post-flare loops on 2005 January 15 that
occurred between two consecutive solar eruption events, both of which generated a fast …