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Updated: Jan 9, 2026

Uncoupling Coriolis Force and Rotating Buoyancy Effects on Full-Field Heat Transfer Properties of a Rotating Channel
Published on: October 5, 2018
A versatile high-performance rotating facility for geophysical and astrophysical flows
Yun-Bing Hu1,2, Xiao-Shen Liu1, Lin Sun1
1Centre for Complex Flows and Soft Matter Research and Department of Mechanics and Aerospace Engineering, Southern University of Science and Technology, Shenzhen 518055, China.
We developed a versatile rotating facility for geophysical and astrophysical flow research. Its modular design and high precision enable advanced laboratory simulations of complex phenomena.
Area of Science:
- Geophysics
- Astrophysics
- Fluid Dynamics
- Laboratory Simulation
Background:
- Geophysical and astrophysical phenomena often involve complex rotating fluid dynamics.
- Laboratory experiments require high-precision facilities to accurately simulate these phenomena.
Purpose of the Study:
- To design, implement, and validate a high-precision rotating facility for laboratory investigations.
- To create a versatile and extensible platform for studying rotating flows.
Main Methods:
- A modular rotating system with a stationary base, dual-bearing stabilized assembly, and servo-driven transmission.
- Achieved leveling accuracy better than 10-4 rad and vibration isolation.
- Tested rotation speeds from 0.1-80 rpm with 0.01 rpm precision.
Main Results:
- Demonstrated exceptional axis stability using a dual-bearing configuration.
- Validated the facility's versatility with particle image velocimetry in Rayleigh-Bénard convection and zonal jet formation experiments.
- Confirmed a static load capacity of 2 tons.
Conclusions:
- The developed rotating facility provides a robust platform for laboratory analogs of geophysical and astrophysical flows.
- Its modular and extensible design supports diverse experimental setups and future upgrades.
- Enables precise simulation of phenomena like convection and jet formation.
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