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ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 09/2019, Volume 882, Issue 2, p. 125
Interchange reconnection is thought to play an important role in driving the dynamics of the slow solar wind. To understand the details of this process, it is... 
SOLAR-WIND | RECONNECTION | CURRENT SHEET | HYPERBOLIC FLUX TUBES | ASTRONOMY & ASTROPHYSICS | SLOW
Journal Article
Physical Review Letters, ISSN 0031-9007, 10/2014, Volume 113, Issue 15, p. 155005
Using fully kinetic simulations, we demonstrate that magnetic reconnection in relativistic plasmas is highly efficient at accelerating particles through a... 
PHYSICS, MULTIDISCIPLINARY | HYPERBOLIC FLUX TUBES | GENERATION | SIMULATIONS | MODEL | SHEET | GAMMA-RAY BURSTS | ELECTRON ACCELERATION | PAIR PLASMAS | NONTHERMAL PARTICLES | Rest | Simulation | Mathematical analysis | Energy density | Mathematical models | Formations | Spectra | Energetic particles
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2012, Volume 541, p. A78
Context. The study of the magnetic topology of magnetic fields aims at determining the key sites for the development of magnetic reconnection. Quasi-separatrix... 
Magnetohydrodynamics (MHD) | Magnetic reconnection | Sun: magnetic topology | Magnetic fields | TOPOLOGY | QUASI-SEPARATRIX LAYERS | SOLAR-FLARES | magnetic fields | magnetic reconnection | HYPERBOLIC FLUX TUBES | CORONAL LOOPS | MODEL | ASTRONOMY & ASTROPHYSICS | EQUILIBRIUM | FILAMENT | magnetohydrodynamics (MHD) | CONFIGURATIONS
Journal Article
Astrophysical Journal, ISSN 0004-637X, 10/2017, Volume 848, Issue 2, p. 117
The squashing factor (or squashing degree) of a vector field is a quantitative measure of the deformation of the field line mapping between two surfaces. In... 
Magnetic Reconnection | Sun: corona | Sun: magnetic fields | FIELDS | QUASI-SEPARATRIX LAYERS | SOLAR-FLARES | HYPERBOLIC FLUX TUBES | ASTRONOMY & ASTROPHYSICS | RECONNECTION | NULL POINTS | MAGNETIC FIELDS | MAGNETIC FLUX | APPROXIMATIONS | MAGNETIC RECONNECTION | TRAJECTORIES | COMPARATIVE EVALUATIONS | DEFORMATION | SUN | VECTOR FIELDS | ACCURACY | LAYERS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | SURFACES
Journal Article
Physical Review Letters, ISSN 0031-9007, 09/2009, Volume 103, Issue 10, p. 105002
The concept of quasiseparatrix layers (QSLs) has emerged as a powerful tool to study the connectivity of magnetic field lines undergoing magnetic reconnection... 
QUASI-SEPARATRIX LAYERS | PLASMA | PHYSICS, MULTIDISCIPLINARY | HYPERBOLIC FLUX TUBES | CORONAL MASS EJECTION | MAGNETIC RECONNECTION | MODEL
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 0004-6361, 01/2020, Volume 633, p. A92
The squashing factor of a magnetic field, Q, is commonly used as an indicator of magnetic reconnection, but few studies seek to evaluate how reliable it is in... 
3-DIMENSIONAL MAGNETIC RECONNECTION | QUASI-SEPARATRIX LAYERS | Sun: corona | MAGNETOSTATIC ATMOSPHERES | FLARES | magnetic reconnection | HYPERBOLIC FLUX TUBES | MAGNETOHYDRODYNAMIC MODEL | SOLAR CORONA | EVOLUTION | CONNECTIVITY | Sun: magnetic fields | ASTRONOMY & ASTROPHYSICS | 3D RECONNECTION | magnetohydrodynamics (MHD)
Journal Article
Journal of Geophysical Research: Space Physics, ISSN 0148-0227, 02/2010, Volume 115, Issue A2, p. n/a
Journal Article