Time-dependent convection on self-adaptive grids

DOI10.1016/0010-4655(95)00189-MzbMath0923.76204OpenAlexW2052693561MaRDI QIDQ1378222

Günther Wuchterl

Publication date: 8 February 1998

Published in: Computer Physics Communications (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/0010-4655(95)00189-m

zbMATH Keywords

non-ideal mediaself-gravitating radiating spherical flowsturbulent convection in stars

Mathematics Subject Classification ID

Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Computational methods for problems pertaining to astronomy and astrophysics (85-08)

Cites Work

• Simple adaptive grids for 1-D initial value problems
• A New Method of Automatic Computation of Stellar Evolution.
• A Method for the Numerical Calculation of Hydrodynamic Shocks
• Unnamed Item
• Unnamed Item
• Unnamed Item
• Unnamed Item
• Unnamed Item

This page was built for publication: Time-dependent convection on self-adaptive grids