Density-driven environmental flows

 

Personnel

James Rottman (Adjunct professor, UCSD)

Ryan Lowe (former undergraduate at UCSD, now graduate student at Stanford)

Eckart Meiburg (UCSB)

Jake Hacker (Arup)

Stuart Dalziel (DAMTP)

Jonathan Shin (former PhD student, DAMTP)

 

 

1 Gravity currents

 

Gravity currents occur when there are horizontal variations in density in a fluid under the action of a gravitational field. A simple example that can readily be experienced is the gravity current that flows into a warm house through a doorway when it is opened on a cold windless day. The larger density of the cold air produces a higher pressure on the outside of the doorway which drives the cold air in at the bottom. If the temperature difference is large enough you will experience a cool draft around your legs if you stand in the doorway.

 

Gravity currents occur in gases when there are temperature differences, as in the doorway flow just described. An important atmospheric example is the sea breeze, which is the flow of cool moist air from the sea to the land. On a warm day the sun heats the land more than the sea and, consequently, the air at low altitudes over the land is warmer than that over the sea. The resulting density difference drives the sea breeze. The sea breeze is a significant feature of coastal meteorology in many parts of the world. For example, the wind measured at Scripps Institution of Oceanography pier in La Jolla, California shows a strong daily signal with a maximum wind directed almost exactly normal to the coast at 1400 local time during the summer. This flow ventilates the coastal strip in southern California with cool air, reducing the peak summer temperatures.

 

Another important class of gravity currents is the flow of dense gases caused by the accidental release of a liquefied gas. There are many examples of liquefied storage of gas. Chlorine, commonly used for sterilizing swimming pools, is an example of a toxic gas that is stored in a pressurised container. These containers are found in residential areas, and chlorine is transported by road and rail. Flammable gases such as natural gas and propane are also stored in this way, often in large quantities. If a leak occurs or the container fails catastrophically, the released liquid vaporizes and produces cold gas, which is denser than air because of its low temperature. Even for low molecular weight gases such as methane the effects of temperature dominate and the cold gas will, under most circumstances, produce a gravity current. Because of the potential dangers of a toxic or flammable gas spreading over the ground in populated regions, there has been considerable research into the consequences of such accidental spills over the past 20 years and much of our understanding of gravity currents comes from field, laboratory and theoretical studies focused on this problem. A nice recent summary of the subject is John Simpson’s book “Gravity currents in the laboratory and the environment” published in 1997 by Cambridge University Press.

 

We focus on the dynamics of gravity currents and have been particularly concerned with currents produced by lock exchange, where two fluids of different densities are initially separated by a vertical barrier. The gravity currents that result when the barrier is removed have been studied in a number of experiments. A summary of present theory, essentially due to Benjamin (1968), can be found in [141] and we note that there are some difficulties with his theory. Our research has examined the assumptions behind Benjamin’s theory. In [147] we examine the flow in an intrusion along an interface, which is an approximation of a current along a stress-free boundary. We find that, in contrast to the accepted view, there is little relative flow and that Benjamin’s assumption that the internal flow is small is valid. In [153] we present experimental observations of lock exchange currents that appear to be energy conserving in that they occupy half the channel depth and have flow speeds close to that predicted by Benjamin. We also study currents in deep ambient fluids and show that, in contrast to Benjamin’s theory, they too can be described by a new energy-conserving theory. We show that both von Karman’s (1940) and Benjamin’s (1968) result that the front Froude number is √2 when the ambient is infinitely deep is wrong and that the correct value is 1.

 

Recently, this work has been extended to non-Boussinesq currents. When the density difference becomes large, there is an asymmetry between the flow of the light and heavy current – see [141]. The theory is singular in the limit of vanishing density ratio, and we have recently carried out experiments which show that it is necessary for an additional hydraulic jump to form. A theory, which includes the jump (but see below) is under development. Some details of this and the Boussinesq case can be found in the lecture I gave at the European Geophysical Society in April 2002 (see EGS_2002.pdf).

 

The effects of rotation on lock exchange currents are discussed in [148]. This paper extends Benjamin’s full-depth lock exchange theory to include the effects of rotation. energy-conserving gravity currents in rotating channels.  The theory is an extension of Benjamin’s for nonrotating gravity currents, and in a similar way makes use of the steady-state and prefect-fluid (incompressible, inviscid, and immiscible) approximations, and supposes the existence of a hydrostatic control point in the current some distance away from the nose. The model allows for fully nonhydrostatic and ageostrophic motion in a control volume V ahead of the control point, with the solution being determined by the requirements that energy and momentum are conserved. The governing parameter is the ratio of the channel width to the internal Rossby radius of deformation. Analytic solutions are determined for the particular case of zero front-relative flow within the gravity current. 

 

2 Two-layer bores

 

A closely related flow to the gravity current is the two-layer bore. Consider a dense gravity current travelling along the lower boundary into a lighter ambient fluid. Now suppose that the ambient fluid ahead of the current also has a lower layer of fluid with the same density as the current. In this case the propagating disturbance is a bore and its speed depends on the depth of the current and the depth of the layer ahead.

 

The classical case when the dense fluid is water and the less dense fluid is air is observed in many rivers, such as the River Severn as shown. The flow in this one-layer bore (or hydraulic jump if the bore is stationary) is determined by the conservation of volume and momentum fluxes – the analysis can be found in standard fluid dynamics text books. It is also known that there is dissipation as the fluid passes through the jump.

 

For the two-layer case conservation of volume and momentum fluxes are not sufficient to determine the flow. It is necessary to state where the dissipation occurs and this is not known a priori. There have been a number of attempts to resolve this issue, and we discuss them in [141]. In the Boussinesq case of small density differences, we have extended the energy-conserving gravity current theory and obtain a good agreement with experiments on bores produced by gravity currents. A paper on this work is in preparation. However, the extension of this theory to the non-Boussinesq case is unclear.

 

We are about to start (July 2002) a project funded by NSF in collaboration with UCSB (PI’s PFL, JWR, Eckart Meiburg) to examine this problem. Experiments and theory will be done at UCSD and compared with DNS calculations done at UCSB.