as initial condition for the simulation of the blowing
step. For that, the finite element commercial package
ABAQUS
®
was used. Thanks to a thermodynamic
model, the air pressure inside the preform is
automatically calculated during simulation. Following
sections focus on presenting each model.
PREFORM HEATING MODELING
In the SBM process, heating devices are often
composed by a set of halogen lamps associated to
aluminum reflectors. The preform translates through
the oven, and is animated by a rotational movement to
provide a uniform temperature along its
circumference. Radiation emitted by the IR lamps is
partially absorbed through the preform thickness,
before being diffused in each space direction.
Additionally, the preform tends to be cooled by air
venting. In other words, preform reheating results from
a combination between conductive, convective, and
radiative heat transfers.
Heat Balance Equation
The evolution versus time of the preform
temperature is governed by the following heat balance
equation:
( )
rp
qTk
dT
c ⋅∇−∇⋅∇=
ρ
(1)
Where T = temperature, t = time, ρ = density, c
p
=
specific heat, k = thermal conductivity, q
r
= radiative
heat flux density. In order to solve this equation in 3D,
a finite volume discretization is adopted. For that, the
preform is meshed into hexahedral elements called
control volumes. Equation (1) is integrated over each
control volume and over the time, to obtain the
following integro-differential formulation:
( )
( )
dtdnq
dtdnTkdtd
t
T
c
t
r
tt
p
Γ
−Γ∇=Ω
∂
∂
∫∫
∫∫∫∫
∆ Γ
∆ Γ∆ Ω
.
.
ρ
(2)
where Ω = control volume, Γ = surface of a control
volume. Unknown temperatures are computed at the
cell centre of each element. While the internal side of
the preform is supposed to be adiabatic, the following
boundary condition is applied to the external one:
( )
44
∞∞
−+−=
∂
∂
− TTTTh
n
T
k
PPETPc
P
σε
(3)
Where h
c
= natural heat transfer coefficient, ε
PET
=
PET mean emissivity, σ = Stefan-Boltzman constant,
T
p
= preform surface temperature at external side, T
∞
=
ambient temperature. The method used for estimating
PET mean emissivity is fully detailed in [2]. This
boundary condition takes into account two types of
thermal exchanges. The first one is due to the cooling
by natural convection, the second one to the own
emission of the preform. These exchanges are
particularly important during the cooling stage.
Radiative Transfer Modeling
Over the spectral band corresponding to the IR
lamps emission (0.38-10µm), PET behaves like a
semi-transparent body. This involves that the radiative
heat flux is absorbed inside the wall thickness of the
preform, and can not be simply applied as a boundary
condition. The radiation absorption must be taken into
account through the divergence of the radiative heat
flux, previously presented in the heat balance equation.
This term represents the amount of radiative energy
absorbed per volume unit; it is also more commonly
called radiative source term. The computation of this
source term can not be carried out without a precise
understanding of radiative transfer properties,
including its spectral and directional dependencies.
Researchers proposed different numerical methods in
order to compute the radiative source term, like
raytracing [5] or zonal method [6]. The method used in
this work is divided into two steps:
First of all, radiative heat fluxes reaching the
preform surface are computed. For that, IR lamps are
meshed into surface elements of which the
contribution is taken into account via view factors
computation. Moreover, IR lamps are assumed to
behave like isothermal grey-bodies. Their emission is
then defined by the Planck’s law [13]. Finally, incident
fluxes are calculated with the following equation:
tit
i
iip
TLSFq
λλλλ
περ
−= 1
0
(4)
Where ρ
λ
= PET reflexion coefficient, F
ip
= view
factor between the lamp element i and the preform, S
i
= surface area of the lamp element, ε
tλ
= tungsten
emissivity, L
λ
= Planck’s intensity of the lamp i at the
filament temperature T
ti
.
In a second time, the radiation absorption is
computed according to the Beer-Lambert law (under
the assumption of the non-scattering cold medium
[13]):
xqxq
λλλ
exp
0
(5)