# Flow field evolution and entrainment in a free surface plunging jet

## TL;DR

This study examines the flow evolution and ambient fluid entrainment in a free surface plunging jet across various Reynolds numbers, revealing unique flow decay characteristics and higher entrainment compared to free jets, with implications for turbulence and mixing.

## Contribution

It provides the first measurements of near-field ambient fluid entrainment in plunging jets and compares flow features across Reynolds numbers, highlighting differences from free jets.

## Key findings

- Plunging jets have shorter potential core lengths.
- Higher ambient fluid entrainment at low Reynolds numbers.
- Primary vortices influence jet decay and entrainment efficiency.

## Abstract

We investigate ambient fluid entrainment and near-field flow characteristics of a free surface plunging jet for five Reynolds numbers ranging from 3000 to 10000 using time-resolved stereo particle image velocimetry (SPIV). We present time-averaged velocities, RMS velocity fluctuations, mean entrainment and unsteady flow features and compare them with previous studies on free jets. We find that plunging jets have a smaller potential core length, and earlier decay of the mean centerline velocity. The peak RMS velocity fluctuations occur at a location significantly upstream compared to the free jets reported in the literature. Near-field ambient fluid entrainment of plunging jets is measured for the first time and is found to be considerably higher than free jets in the low Reynolds number range. For the plunging jet case at Re = 3000, faster jet decay, higher levels of turbulent intensity in the near-field, and augmented mass entrainment result from strong primary vortices that give the turbulent/non-turbulent interface (TNTI) its convoluted shape which facilitates both bulk entrapment of ambient fluid and small scale nibbling because of larger surface area. These primary vortices occur right below the free surface and disintegrate into secondary structures at axial locations that are upstream compared to those of free jets. At higher Reynolds numbers, primary vortices are smaller in size, weak in swirling strength, and disintegrate prematurely, resulting in suppressed mixing and reduced entrainment efficiency.

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Source: https://tomesphere.com/paper/1903.01906