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Drag Reduction of Superhydrophobic Surfaces

Super-hydrophobic surfaces were initially inspired by the unique water-repellent characteristics of the lotus leaf.

When contacting with water, super-hydrophobic surfaces trap a layer of air bubbles (or plastron) between the surface texture, forming the so-called Cassie-Baxter state.

micro images to show lotus leaf

This project focuses on reducing skin friction drag through the development of passive methods using bio-inspired micro/nano structural surfaces by employing advanced micro/nano fabrication techniques.

 

Fabrication of superhydrophobic surface with random structures

 

Our objective is to build on our understanding of wetting transition of hierarchical bio-inspired materials. We introduced superhydrophobic surfaces with large water contact angles and a small sliding angles were fabricated by spray coating of silica nano particles over sandpapers with different grit sizes. Optical setup is developed, and surface properties are studied by Scanning electron microscopy as well as a surface profiler.

 

The water contact angle and SEM images of the hierarchical SHS

 

 

Drag reduction and plastron status in turbulent flow

 

To visualize the plastron while the SHS was subjected to turbulent flows, Total Internal Reflection and Reflected Light Microscopy techniques were developed..

Silvery patches, that could be seen even with the naked eye, showed the surface was covered by an air layer.

Under turbulent flow, gas fraction was reduced due to the shear flow. In addition, the surface roughness greatly influenced the trend of plastron depletion in turbulent flows.

We found that the drag reducing property of superhydrophobic surfaces depends on the roughness height.

 

data chart

TIR and reflected light microscopy

TIR and reflected light microscopy

plastron data

 

 

Fabrication of superhydrophobic surface with regular structures

 

SHS were also fabricated by spraying nano particles over regular micro-scale textures fabricated by a MSLA 3D printer.

We showed that under the turbulent flow, SHS experienced a sudden transition from the Cassie-Baxter state to the Wenzel state, and no metastable state observed.