Thermal convection
Whether cooling a power
station, insulating a confined plasma, or simply cooling
our laptop, heat transfer is one of the most important and exciting research
areas in Engineering. However, several problems are still poorly
understood.
We enjoy tackling old and
not-so-old heat transfer problems and solve them in a creative way.
The thin cylinder in cross-flow
Heat transfer between a cylinder
with large length to diameter ratio and a fluid stream in cross-flow occurs
in many applications, such as hot-wire anemometers, submarine pipelines,
electrical and telecommunication cables.
We have found that in the
limit of small Péclet numbers the wire can be
treated as a mathematical singularity in the plane normal to its axis:
With these
approximations, the dimensionless energy equation is:
(1)
Solving the energy
equation with the theory of analytical functions, we have been able to
obtain a solution in closed form, with
no empirical coefficients:
(2)
where K0(x) is a modified Bessel function of second kind.
Our solution is in very
good agreement with other approximate solutions existing in the literature:
V. Bertola,
E. Cafaro, Analytical function theory approach to
the heat transfer problem of a cylinder in cross-flow at small Péclet numbers, International Journal of Heat and Mass Transfer, Vol 49(17-18), pp. 2859-2863, 2006.
Rayleigh-Bénard convection of a viscoelastic
fluid in porous media
We have studied the
Horton-Rogers-Lapwood problem of Rayleigh-Bénard convection in a porous medium for a viscoelastic fluid with a single relaxation time.
If is the retardation
time due to the action of the porous matrix, and is the relaxation
time due to viscoelasticity, the conservation
equations for mass, momentum and energy are:
with the boundary conditions and .
Similar to the Salzmann-Lorenz
analysis of atmospheric convection, the conservation equations can be
transformed into a reduced-order dynamical system by a Galerkin
projection in the space of eigenfunctions of the temperature
fluctuations and the stream function (D1 and D2 are
the dimensionless characteristic times, and r is the Rayleigh
number)
Depending on the
characteristic times, the critical Rayleigh
number for the onset of convection can be significantly lower than for a
Newtonian fluid:
The trajectory of the
system in the phase space may converge to an equilibrium point
(steady-state convection):
or to a stable orbit
(oscillatory convection):
V. Bertola,
E. Cafaro, Thermal instability of viscoelastic fluids in horizontal porous layers as
initial value problem, International Journal of Heat and Mass Transfer, Vol 49(21-22), pp 4003-4012, 2006.