Jacobian-free Newton–Krylov (JFNK) methods are synergistic combinations of Newton-type
methods for superlinearly convergent solution of nonlinear equations and Krylov subspace …

Magnetic reconnection is a topological rearrangement of magnetic field that converts
magnetic energy to plasma energy. Astrophysical flares, from the Earth's magnetosphere to …

While it is certain that the fast solar wind originates from coronal holes, where and how the
slow solar wind (SSW) is formed remains an outstanding question in solar physics even in …

The ever increasing processing capabilities of the supercomputers available to
computational scientists today, combined with the need for higher and higher resolution …

Abstract The four Magnetospheric Multiscale (MMS) spacecraft recorded the first direct
evidence of reconnection exhausts associated with Kelvin‐Helmholtz (KH) waves at the …

Alongside magnetic reconnection, turbulence is another fundamental nonlinear plasma
phenomenon that plays a key role in energy transport and conversion in space and …

Three-dimensional kinetic simulations of magnetic reconnection for parameter regimes
relevant to the magnetopause current layer feature the development of turbulence, driven by …

Magnetic reconnection is believed to be the main driver to transport solar wind into the
Earth's magnetosphere when the magnetopause features a large magnetic shear. However …

Inertial fusion energy (IFE) has been considered a promising, nearly inexhaustible source of
sustainable carbon-free power for the world's energy future. It has long been recognized that …

Implicit time differencing of the resistive magnetohydrodynamic (MHD) equations can step
over the limiting time scales—such as Alfvén time scales—to resolve the dynamic time …