Numerical Methods for MHD - Part 4: Advanced Topics
Series Navigation Part 1: Introduction and Basic Equations Part 2: Numerical Methods and Solution Techniques Part 3: Riemann Solvers Part 4: Advanced Topics Table of Contents Advance...
Numerical Methods for MHD - Part 3: Riemann Solvers
Series Navigation Part 1: Introduction and Basic Equations Part 2: Numerical Methods and Solution Techniques Part 3: Riemann Solvers Part 4: Advanced Topics Table of Contents Riemann...
Numerical Methods for MHD - Part 2: Numerical Methods and Solution Techniques
Series Navigation Part 1: Introduction and Basic Equations Part 2: Numerical Methods and Solution Techniques Part 3: Riemann Solvers Part 4: Advanced Topics Table of Contents Numeric...
Ideal MHD Equations, Conserved Variables, and Fluxes
Series navigation Ideal MHD Equations Finite Difference versus Finite Volume Riemann Problems and Approximate Solvers WENO-JS Reconstruction Ideal MHD Equations, Conserved Variables, and...
Scale Height
스케일 높이란 무엇인가? 스케일 높이 (Scale Height, \(H\))는 대기에서 고도에 따라 압력과 밀도가 어떻게 감소하는지를 설명하는 중요한 물리적 개념입니다. 구체적으로, 스케일 높이는 대기의 압력이나 밀도가 고도 \(H\) 만큼 증가할 때마다 약 \(\frac{1}{e}\) 만큼 감소하는 높이를 의미합니다. 이 개념은 행성의 대기뿐만 아...
Parker Instability
Parker Instability Introduction The Parker instability (proposed by E.N. Parker in 1966) is a classic example of magnetic buoyancy instability in astrophysical plasmas. It arises in a gravitati...