High order WENO and DG methods for time-dependent convection-dominated PDEs: A brief survey of several recent developments
CW Shu - Journal of Computational Physics, 2016 - Elsevier
For solving time-dependent convection-dominated partial differential equations (PDEs),
which arise frequently in computational physics, high order numerical methods, including …
which arise frequently in computational physics, high order numerical methods, including …
Shear-driven transition to isotropically turbulent solar wind outside the Alfvén critical zone
Shear-driven Transition to Isotropically Turbulent Solar Wind Outside the Alfvén Critical Zone -
IOPscience This site uses cookies. By continuing to use this site you agree to our use of …
IOPscience This site uses cookies. By continuing to use this site you agree to our use of …
Solar Orbiter observations of the Kelvin-Helmholtz waves in the solar wind
Context. The Kelvin-HeImholtz (KH) instability is a nonlinear shear-driven instability that
develops at the interface between shear flows in plasmas. KH waves have been inferred in …
develops at the interface between shear flows in plasmas. KH waves have been inferred in …
High-order targeted essentially non-oscillatory scheme for two-fluid plasma model
Y Hou, K Jin, Y Feng, X Zheng - Applied Mathematics and Mechanics, 2023 - Springer
The weakly ionized plasma flows in aerospace are commonly simulated by the single-fluid
model, which cannot describe certain nonequilibrium phenomena by finite collisions of …
model, which cannot describe certain nonequilibrium phenomena by finite collisions of …
High-order low-dissipation targeted ENO schemes for ideal magnetohydrodynamics
The recently proposed targeted ENO (TENO) schemes (Fu et al. J Comput Phys 305: 333–
359, 2016) are demonstrated to feature the controllable low numerical dissipation and sharp …
359, 2016) are demonstrated to feature the controllable low numerical dissipation and sharp …
[HTML][HTML] Compressibility effect on coherent structures, energy transfer, and scaling in magnetohydrodynamic turbulence
Compressible magnetohydrodynamic (MHD) turbulence, a model often used to study space
and astrophysical plasmas, differs from incompressible magnetohydrodynamic and …
and astrophysical plasmas, differs from incompressible magnetohydrodynamic and …
Energy cascade and its locality in compressible magnetohydrodynamic turbulence
We investigate energy transfer across scales in three-dimensional compressible
magnetohydrodynamic (MHD) turbulence, a model often used to study space and …
magnetohydrodynamic (MHD) turbulence, a model often used to study space and …
An efficient low-dissipation high-order TENO scheme for MHD flows
L Fu - Journal of Scientific Computing, 2022 - Springer
In this paper, an efficient low-dissipation high-order TENO scheme is proposed for ideal
MHD flows. For high computational efficiency, a troubled-cell indicator based on the ENO …
MHD flows. For high computational efficiency, a troubled-cell indicator based on the ENO …
A modified monotonicity-preserving high-order scheme with application to computation of multi-phase flows
CT Ha, JH Lee - Computers & Fluids, 2020 - Elsevier
The monotonicity preserving (MP) polynomial-based reconstruction scheme with Runge-
Kutta time stepping by Suresh and Huynh (1997) has been applied extensively in …
Kutta time stepping by Suresh and Huynh (1997) has been applied extensively in …
Magnetohydrodynamic Turbulence Simulations as a Testing Ground for PUNCH
Abstract The Polarimeter to UNify the Corona and Heliosphere (PUNCH) will image
macroscopic features of the inner heliosphere and also admit sufficiently high spatial …
macroscopic features of the inner heliosphere and also admit sufficiently high spatial …