FENSAP-ICE: Analytical Model for Spatial and Temporal
Evolution of In-Flight Icing Roughness
Giulio Croce
*
and Erika De Candido
†
Università di Udine, 33100 Udine, Italy
Wagdi G. Habashi
‡
and Jeffrey Munzar
§
McGill University, Montreal, Quebec H3A 2S6, Canada
and
Martin S. Aubé,
¶
Guido S. Baruzzi,
**
and Cristhian Aliaga
††
Newmerical Technologies International, Montreal, Quebec H3A 2M7, Canada
DOI: 10.2514/1.47143
Ice roughness, which has a major influence on in-flight icing heat transfer and, hence, ice shapes, is generally input
from empirical correlations to numerical simulations. It is given as uniform in space, while sometimes being varied in
time. In this paper, a predictive model for roughness evolution in both space and time during in-flight icing is
presented. The distribution is determined mathematically via a Lagrangian model that accounts for the stochastic
process of bead nucleation, growth, and coalescence into moving droplets and/or rivulets and/or water film. This
general model matches well the spatial and temporal roughness distributions observed in icing tunnel experiments
and is embedded in FENSAP-ICE, extending its applicability outside the range of airfoil types for which correlations
exist. Thus, an additional important step has been taken toward removing another empirical aspect of in-flight icing
simulation.
Nomenclature
g = gravity
h = height
L = latent heat
m = mass flow
p = pressure
Q
h
= convective heat flux
T = temperature
u, v = velocity
= collection efficiency
= viscosity
= density of water
= shear stress
I. Introduction
I
N-FLIGHT icing continues to represent major risks for aircraft
safety. When an airplane crosses clouds of supercooled droplets
during takeoff, holding, or landing, the impinging droplets may
freeze on the exposed surfaces and build up ice around wings,
nacelles, tail, empennage, antennas, and several other lifting and
nonlifting areas. The accreted ice may alter the aerodynamic
performance of the aircraft, interfere with the movement of control
surfaces and their effectiveness, block engine inlets, or be shed and
damage engines, propellers, or structural components.
Computational fluid dynamics (CFD) modeling has emerged as a
powerful tool for the prediction of ice shapes and for the simulation
and optimization of ice protection systems. However, the simulation
of in-flight icing is a very complex multiphysics problem, and several
aspects are still far from being well represented. The present paper
borrows ideas in a multidisciplinary way from various fields to
elucidate one of these issues, namely, the analytical versus empirical
evaluation of ice-induced surface roughness, which has an important
effect on conjugate heat transfer and, ultimately, on accreted ice
shapes. FENSAP-ICE, a 3-D in-flight icing system, serves as the
ideal vehicle for the new models developed.
Experimental evidence shows that an iced surface is not smooth,
but covered by a collection of nearly hemispherical beads with radii
of the order of millimeters [1]. Furthermore, because roughness is
induced by the ice accretion itself, it is far from being constant in
either space or time. In particular, roughness appears at the beginning
of ice formation and grows with time until a final distribution is
attained asymptotically [2]. Roughness height is also not constant in
space but is usually very small around the leading edge and becomes
larger further downstream [1,3].
The roughness shape and distribution ought to be intuitively
related to the size and evolution of the beads and rivulets formed on
the surface by impinging droplets and their interaction with the
already accreted layer. Surface roughness affects shear stress and
heat transfer [4], which in turn determine the shape and size of the
accreted ice layer. Thus, there is a time-varying two-way coupling
between roughness buildup and ice accretion. Finally, the liquid
water layer on the ice surface affects the effective area exposed to
evaporation and, consequently, the evaporative heat flux. The
importance of the effective surface fraction exposed to evaporation in
heat transfer processes has been clearly demonstrated in different
application fields [5,6] and should not be neglected in the simulation
of anti- and de-icing systems.
The understanding and handling of ice-induced roughness is of
crucial importance to obtain accurate and reliable CFD-based ice
shapes. Currently, most icing codes provide simplified roughness
modeling through the use of empirical correlations. The most widely
employed correlation is that of Shin and Bond [7], which gives a
Presented as Paper 2009-4126 at the 1st AIAA Atmospheric and Space
Environments Conference, San Antonio, TX, 22–25 June 2009; received 11
September 2009; revision received 31 December 2009; accepted for
publication 12 January 2010. Copyright © 2010 by W.G. Habashi. Published
by the American Institute of Aeronautics and Astronautics, Inc., with
permission. Copies of this paper may be made for personal or internal use, on
condition that the copier pay the $10.00 per-copy fee to the Copyright
Clearance Center, Inc., 222 Rosewood Drive, Danvers, MA 01923; include
the code 0021-8669/10 and $10.00 in correspondence with the CCC.
*
Professor, Department of Mechanical Engineering, Via delle Scienze 208.
†
Ph.D. Candidate, Department of Mechanical Engineering, Via delle
Scienze 208.
‡
Professor, Director of the Computational Fluid Dynamics Laboratory,
Department of Mechanical Engineering, 688 Sherbrooke Street West, Fellow
AIAA.
§
Honors Summer Student, Computational Fluid Dynamics Laboratory,
Department of Mechanical Engineering, 688 Sherbrooke Street West.
¶
Vice President Operations, 680 Sherbrooke Street West.
**
Director of Product Development, 680 Sherbrooke Street West. Member
AIAA.
††
Chief, Consulting Services, 680 Sherbrooke Street West.
JOURNAL OF AIRCRAFT
Vol. 47, No. 4, July–August 2010
1283