We analysed a GOES C6. 2 class solar flare that occurred on 27 October 2003 at the
heliographic position S20E29. Utilising a database developed from a simplified 3D magnetic …

Magnetic reconnection is a fundamental process in astrophysical and space plasmas which
is responsible for particle acceleration, in particular, in solar flares. Separator reconnection …

Abstract Three-dimensional (3D) magnetic reconnection is taking place commonly in
astrophysical and space plasmas, especially in solar flares which are rich sources of highly …

Magnetic reconnection is understood to be a potential mechanism for particle acceleration in
astrophysical and space plasmas, especially in solar flares. Torsional fan reconnection is …

Magnetic reconnection is a common phenomenon taking place in astrophysical and space
plasmas, especially in solar flares which are rich sources of highly energetic particles …

Magnetic reconnection is a potential mechanism for charged particle acceleration in
astrophysical and space plasmas, especially in solar flares, which are rich sources of highly …

We investigate charged particle dynamics and acceleration in the current sheet located in
the reconnection outflow region. We consider parameter ranges corresponding to current …

Magnetic reconnection is known as an essential process to convert stored energy of
magnetic field into the kinetic, thermal energy of plasma and the acceleration of charged …

Abstract “Flux-tube disconnection” is a type of steady-state three-dimensional magnetic
reconnection with O-point at the origin of the resistive diffusion region. Magnetic …

In a three-dimensional non-null magnetic reconnection, the process of magnetic
reconnection takes place in the absence of a null point where the magnetic field vanishes …