Comparison of the Eulerian and Lagrangian approaches to studying the peculiarities of the interstellar dust distribution in the heliosphere in the framework of the cold gas model
DOI10.1134/s0015462822601838zbMath1528.76085OpenAlexW4377042207MaRDI QIDQ6114745
V. V. Izmodenov, E. A. Godenko
Publication date: 12 July 2023
Published in: Fluid Dynamics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1134/s0015462822601838
Stochastic analysis applied to problems in fluid mechanics (76M35) Rarefied gas flows, Boltzmann equation in fluid mechanics (76P05) Dusty-gas two-phase flows (76T15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)
Cites Work
- Model representations of the interaction between the solar wind and the supersonic interstellar medium flow. Prediction and interpretation of experimental data
- Flows near stagnation points in non-orthogonally colliding disperse viscous flows
- Inertial phase separation in rotating self-gravitating media
- Full Lagrangian methods for calculating particle concentration fields in dilute gas-particle flows
- Lagrangian modelling of dust admixture in gas flows
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