CFD-MHD(自2012年2月更名為計算天文物理,或簡稱CompAS)起源自中央研究院天文及天文物理研究所、中央研究院數學所以及台灣大學數學系共同合作的主題計畫,主要目標是要針對天文物理學問題而發展的高效能計算流體力學及磁流體力學程式碼。
我們已經根據精確/近似的黎曼解為基礎,成功發展了一套二/三維度的 Godunov 程式碼,主要功能包括自有重力、邊界的特徵分解以及邊界無反射現象。現已應用在兩項主要問題:螺旋星系內氣體盤的結構和演化,原恒星盤內的行星遷移效應。
Formation and Evolution of Protoplanetary and Circumplanetary Disks with Antares Three-Dimensional Global Hydrodynamic Simulations
Cotribution analysis of molecular line of a disk
Formation of Isothermal Circumplanetary Disks with Three-Dimensional Global Simulations for Sub-Neptune-Mass Protoplanets
A Self-consistent Model for Super/sub-luminal Motions and Particle Acceleration in the M87 Jet
HYDRODYNAMICAL SIMULATIONS OF THE BARRED SPIRAL GALAXY NGC 1097
Micro-ejections in star-disk resistive magnetohydrodynamic simulations
On the Orbital Evolution of a Jovian Planet Embedded in a Self-Gravitating Disk
Self-gravitational force calculation of infinitely thin gaseous disks
The Effect of Bars and Transient Spirals on the Vertical Heating in Disk Galaxies
Hydrodynamical Simulations of the Barred Spiral Galaxy NGC 6782
Probing Substellar Companions of Asymptotic Giant Branch Stars through Spirals and Arcs
Gravitationally Induced Density Wake of a Circularly Orbiting Object As an Interpretative Framework of Ubiquitous Spirals and Arcs
Impact of Type Ia Supernova Ejecta on a Helium Star Binary Companion
Collimated fast winds in Preplanetary Nebulae
Magnetospheric Accretion and Ejection of Matter in Resistive MHD Simulations
Simulations of winds