We present a review of the constrained interpolation profile (CIP) method that is known as a
general numerical solver for solid, liquid, gas, and plasmas. This method is a kind of semi …

We model the effects of repeated supernova (SN) explosions from starbursts in dwarf
galaxies on the interstellar medium of these galaxies, taking into account the gravitational …

This paper presents a simple and practical scheme for capturing moving interfaces or free
boundaries in multi‐fluid simulations. The scheme, which is called THINC (tangent of …

Flowing sediments such as debris and liquefied soils could exert a tremendous amount of
force as they impact objects along their paths. The total impact force generally varies with …

Abstract The Multi-slit Solar Explorer (MUSE) is a proposed mission composed of a multislit
extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and …

We present in this work a new reconstruction scheme, so-called MUSCL-THINC-BVD
scheme, to solve the five-equation model for interfacial two phase flows. This scheme …

An interface capturing method with a continuous function is proposed within the framework
of the volume-of-fluid (VOF) method. Being different from the traditional VOF methods that …

Feedback from massive stars is one of the least understood aspects of galaxy formation. We
perform a suite of vertically stratified local interstellar medium (ISM) models in which …

Two semi-Lagrangian schemes that guarantee exactly mass conservation are proposed.
Although they are in a nonconservative form, the interpolation functions are constructed …

We present the results of 2.5-dimensional MHD simulations of jet formation by magnetic
accretion disks in which both ejection and accretion of disk plasma are included self …