Similarity solutions for strong shock waves in magnetogasdynamics under a gravitational field
DOI10.1007/S11587-020-00529-1zbMath1514.35285OpenAlexW3038210400MaRDI QIDQ6044849
Rajan Arora, Deepika Singh, Astha Chauhan
Publication date: 22 May 2023
Published in: Ricerche di Matematica (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s11587-020-00529-1
shock wavessimilarity solutionsmagnetogasdynamicsRankine-Hugoniot conditionsLie group of transformationsself-gravitating ideal gas
Shocks and singularities for hyperbolic equations (35L67) PDEs in connection with fluid mechanics (35Q35) Magnetohydrodynamics and electrohydrodynamics (76W05) Initial value problems for first-order hyperbolic systems (35L45) Kinetic theory of gases in equilibrium statistical mechanics (82B40) Hyperbolic equations on manifolds (58J45)
Related Items (1)
Cites Work
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Self-similar solutions in a plasma with axial magnetic field (\(\theta\)-pinch)
- A study of stellar point explosion in a self-gravitating radiative magneto-hydrodynamic medium
- Self-similar solutions in the theory of flare-ups in novae. I
- Similarity methods for differential equations
- The propagation of converging and diverging shock waves under intense heat-exchange conditions
- A self-similar flow in generalized Roche model with increasing energy
- Similarity solutions for imploding shocks in a non-ideal magnetogasdynamics
- Similarity solutions of cylindrical shock waves in non-ideal magnetogasdynamics with thermal radiation
- Converging spherical and cylindrical shocks with zero temperature gradient in the rear flow field
- Similarity Solutions for Reactive Shock Hydrodynamics
- Equatorial propagation of axisymmetric magnetohydrodynamic shocks
- SIMILARITY SOLUTIONS FOR STRONG SHOCKS IN A NON-IDEAL GAS
- Cylindrical Shock Waves Produced by Instantaneous Energy Release
- Symmetries and differential equations
This page was built for publication: Similarity solutions for strong shock waves in magnetogasdynamics under a gravitational field