Pages that link to "Item:Q3614105"
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The following pages link to Supersonic solar wind ion flows downstream of the termination shock explained by a two-fluid shock model (Q3614105):
Displaying 7 items.
- Gasdynamic models of physical phenomena occurring in the space. An overview (Q408737) (← links)
- Model representations of the interaction between the solar wind and the supersonic interstellar medium flow. Prediction and interpretation of experimental data (Q605768) (← links)
- Turbulent drag reduction by spanwise oscillations of a channel wall with porous layer (Q667363) (← links)
- Enhanced drag-reduction over superhydrophobic surfaces with sinusoidal textures: a DNS study (Q667451) (← links)
- Phasespace transport of a quasi-neutral multi-fluid plasma over the solar wind MHD termination shock (Q2443576) (← links)
- The confrontation between general relativity and experiment (Q5919790) (← links)
- Influence of streamwise and spanwise wall magnet arrays on near-wall MHD turbulence (Q6555051) (← links)
