NON-LINEAR MOTIONS OF
SURFACE EFFECT SifiPS
J. Moulijn
Report 1Ï26-P
December 1997
Published in: International Conference on Air
Cushion Vehicles (ACVs), Royal Institution of
Naval Architects, London, December 3, 1997.
TU Deift
Faculty of Mechanical Engineering and Marine Technology Ship Hydromechanics LaboratoryINTERNATIONAL CONFERENCE
on
AIR CUSHION VEHICLES
(ACVs)
3 DECEMBER 1997 LONDON
PROCEEDINGS
THE ROYAL INSTITUTION OF NAVAL
ARCHITECTS
RINA
in association with the
ROYAL AERONAUTICAL SOCIETY & THE HOVERCRAFT SOCIETY
RAPID MARINE TRANSPORT GROUP & SMALL CRAFT GROUP
INTERNATIONAL CONFERENCE
AIR CUSHION VEHICLES
(ACVs)
at the
Weir Lecture Hall, RINA, London SWI
3 December 1997
© 1997 The Royal Instjtútion of Naval Architects
The Institution is not, as a body, responsible for the opinions expressed by the individual authors or speakers.
THE ROYAL INSTITUTION OF NAVAL ARCHITECTS
10 Upper BelgraveStreet,
London, SW1X 8BQ
Telephone: 0171-235-4622 Fax: 0171-245-6959 ISBN No: 0 903055 35 X
CONTENTS
SESSION i - ACV TECHNOLOGY - THE STATE OF THE ART
1. ADVANCED HOVERCRAFr - SKIRT TECHNOLOGY
by D R Lavis, B G Forstell, and C Jiang, Band, Lavis & Associates1 Inc. (USA)
2.* AEROEISTIC AND HYDROELASTIC DYNAMIC DESIGN PRINCIPLES
OF HO VERCRAFTRESPONSI VE SKIRT
by M Tao, Marine Design & Research Institute of China and P A Sullivan,
University of Toronto (China & Canada)
3. FANS AND PROPELLERS FOR AIR CUSHION: VEHICLES - PAST, PRESENT
AND FUTURE
by M J Ccx, Hovercraft Consultants Ltd, and C B Eden, Air Vehicles Ltd (UK)
SESSION II- DESIGN
4. AIR CUSHION PASSENGERNEHICLE FERRIES FOR WEST BALTIC ROUTES - A PROPOSAL
by T Jastrzebski, R Michalski and WChadzynski, Technical University of Szczecin (Poland)
5. NON-LINEAR MOTIONS OF SURFACE EFFECT SHIPS
by J MoUlijn, DeIft University of Technolögy (Netherlands)
6. AERODYNAMICAL LIFT-FAN SYSTEM PROBLEMS AND DYNAMIC STABILITY OF ACVs
by A A Dolgopolov, L A Maslov, V V Mitrofovich and S A Isakovich, Central
SESSION III
- MILITARY ACVs
NAVAL HOVERCRAFT - WHAT NAVAL HOVERCRAFT?
by B J Russell, Hovercraft Society
(UK)
THIRD GENERATION, MEDIUM-LIFTHOVERCRAFT FOR MODERN AMPHIBIOUS OPERATIONS
by S E Southby-Tailyour, Ewen SouthbyTaiIyourAssociates - Amphibious Consultants
(UK)
9. MCM SYSTEM DEVELOPMENT FOR THE SWEDISH NAVY BASED ON
AIR CUSHION TECHNOLOGY
by M Örnfelt, Swedish Defence Materiel Administration
11. EFFECT OF ECONOMICAL ASPECTS
ON FAST SPEED CRAFT
DESIGN PARAMETERS
by V A Abrarnovsky, Central Marine Design Bureau 'Almaz', Saint-Petersburg and A V Abrarnovsky1 Saint-Petersburg State Marine Technical University
(Sweden)
10. THE SRN4 HOVERCRAFT SO FAR - TECHNICAL & OPERATIONAL ASPECTS
by L Heatley- Hoverspeed Ltd
(UK)
(Russia)
12. SUMMARY REPORT OF DISCUSSIONS
by E C Tupper
PAPER NO.5
NON-LINEAR MOTIONS OF SURFACE EFFECT SHIPS
by J Moulijn, Deift University of Technology, The Netherlands
Paper presented at the
International Conference
AIR CUSHION VEHICLES
(ACVs)
Joøst Moulijnstudied!Naval Architecture at Deift University
of Technology. He obtained his MSc degree in 1994 on
a theses about the trailing vortex wake of marine
propellers. He is currently a PhD student at the Ship
Hydromechanics Laboratory in Deift.
1. INTRODUCTION
In recent years, the interest in large Surface Effect Ships (SES) sailing in open sea has raised. Therefore an
adequate computational method for seakeeping of SES must be developed and validated. This paper describesa
computational method for motions of a SES in waves. The method is validated using experimental results of
MARIN. When the motions of a SES can be calculated accurately, important aspects such as added resistance due to ambient waves and wave loads on the structure can be calculated. These aspects are subject to further
research.
A Surfäce Effect Ship is a hybrid of a catamaran and a hovercraft. An air cushion is enclosed by the side hulls,
the deck, the water surface and flexible seals forward and aft (Fig. 1). Most of the vessels weight is carried by the air cushion. The rest is carried by the hulls. The air cushion is pressurised by a system of fans, as air leaks from the cushion under the seals.
Compared to catamaran SES have a low resistance.
Advantages of SES with respect to hovercraft are water
born propulsion, a smaller amount of air leakage and
bettor manoeuvring characteristics Astheside hullsof a SES provide stability, there is no need to have several compartments in the air cushion. A major disadvantage of SES with respect to hovercraft is of course the loss of the amphibious capabilities.
When studying seakeeping of Surface Effect Ships two
frequency ranges of interest occur: the "normal frequency
range up to a frequency of about 1 Hz, and the high
frequency range. In the normal frequency range the
motions of a SES are small compared to a catamaran In
the high frequencyrangethed isplacement amplitudes are only small, but the acceleration level can be quite high
resulting in a poor ride quality. These high frequent
oscillations are caused by acoustic resonances of the air in cushion as was pointed out by Nakos et aI [1 1 This
NON-LINEAR MOTIONS OF SURFACE EFFECT SHIPS
Joost Moulijn
Deltt University of Technology
SUMMARY
Results of a currently running four year research project on seakeeping of Surface Effect Ships (SES) ara presented. A nonlinear computationalmethod for the motions of a Surface Effect Ship in waves isdescribed. The resuitsof the method are compared wh experimental data of MARIN The agreement is good The effect of simplifications of the methodon
the results is investigated.
AUTHOR'S BIOGRAPHY
1
phenomenon is usually referred to as cobblestone effect.
The cobblestone effect was studied extensively by Søresen[2], Steen[3] and Ulstein[4].
The present method deals with the normal frequency
range. The excess pressure in the air cushion is always assumed to be constant in space so acoustic resonance cannot be resolved. Air compressibility is taken into
account, so the spatially constant pressure resonance of
the air cushion (Helmholtz resonance) is resolved. Motions of SES werefirst studied by Kaplan and Davis[5].
In Kaplan et aI[6] a non-linear six degree of freedom
motion program is presented. An extensive overview of the hydrodynamics of ACV's and SES' was presented by
Doctors(7].
By many authors air leakage is considered important and
highly non-linear ([1], [8], [9]). Nevertheless air leakage is often linearised or even neglected ([1], [81). Steon[3]
shows the importance of air leakage for cobblestone
effect. Wlstein[4] carried out extensive air leakage
computations using a non-linear panel method. He found that a simple one dimensional approach also yields good results as long as the contraction of the escape air jet is taken into account.
The bag-type seal common!y usedto closethe air cushion
at the aft end is also considered to have an important
effect on the motions of SES. The bag is pressurised at a slightly higher pressure than the air cushion. Lee[1O]
developed a two dimensional model. He neglects
gravitational and inertial forces and the dynamic pressure
distribution under the seal due to air leakage.
Steen[3] presented a two dimensional model. He also
neglects gravitational and inertial forces on the flexible bag membrane, but he does take the dynamic pressure
distribution due to air leakage into account. Steen
showed the. importance of the seal model with respect to
cobblestone effects.
Masset and Morel[9],[11] developed and validated a
similar model. Ulstein(4] developed a model that includes
the inertia of the bag membrane. The finger type seal
commonly used to close the air cushion at the fore side is
considered less important for motions of SES. The seal
does not need to be pressurised, and the forces acting on
Some confusion appears to exjst about the importance of the interaction of the air cushion and the wave surface in the cushion. Kaplan etaI[5].[6] only consider undisturbed incident waves in the air cushion; Kaplan[12] claims that the waves induced by the vessel are small and only have
a minor effect on the overall motions; According to
Doctors[13] and Kim and Tsakonas[14] this
is anoversimplified procedure.
McHenry et aI [8] report only a small effect of cushion
induced waves but Nakos at al [1] show
that the inclusionj of cushion induced waves damps the Helmholtz resonance and also shifts the Helmhottzresonance to a higher frequency. Moran[15],
Kapsenberg[1'6] and Masset et al [9] found from model
tests that the amplitude of the free surface waves is
affected by the air cushion.
Another important aspect of SES is the air supply system.
In all existing methods for SES motions, including the present method, steady fan characteristics are used.
Durkin and Luehr[1 7], Sullivan at aI [18], Masset et al [9] and Witt[1 9] show that the fans respond in a dynamical way to the oscillating pressure in the air cushion. Sullivan et al [18] also show that the dynamic behaviour of the lift fan has a large damping effect on the heave motions of a
hovering box.
Scale effects play an important role in model testing of
ACV and SES (see for instance Lavis et aI [20]). For
Froude scaling of the air compressibility the ambient pressure also should be multiplied by the scale factor, otherwise the stiffness of the air cushion is much too
large. Kapsenberg[2 1] performed oscillation experiments in a depressurised towing tank. He found an important effect of the ambient pressure on the added mass and
damping coefficients. Kapsenberg and Blume[22]
performed modeltests atdifferent scaleratios with models
equipped with a flexible membrane on top of the air
cushion; This membrane (usually referred
to as
diaphragm) also reduces the cushion stiffness as ft
supplies some extra volume when the cushionpressure
increases. They found good agreement and concluded
that the diaphragm technique is a valid way of scaling cushion dynamics.
In the present method the cushion dynamicsare retained
in full non-linear form; Non-linear air leakage is included. The motions 'and cushion excess pressure are solved in
a time simulation procedure. A two-dimensional non-linear model for the bag-type stern seal is implemented.
This model is similar to the models of Steen[3) and
Masset and Morel[1 1].
A linear three-dimensional Rankine source panel method is used to compute the hydrodynamic forces on the side hulls and the wave height in the cushion. Interaction of
the air cushion and the wave surface is taken into
account. Results of the method are presented àndcomparedto experimental data of MARIN. The effects of cushion-surfaceinteraction, the sternseal, air leakage and
the
fan system on the
computational results areinvestigated. The importance of scale effects during
experimènts is demonstrated.
2
DEFINITION OF COORDINATE SYSTEMS,
DISPLACEMENTS AND EXCESS PRESSURES
Two right-handed coordinate systems will be used. One
system is fixed to the vessel, that sails at a mean velocity
U. This system is called the body fixed system; O-XYZ The X-axis points in the direction of the bow,.the Y-axis points to the port side, the Z-axis points upwards. The origin Odoes not necessarily coincide with the centre of gravity of the vessel. This system is used to define the geometry of the vessel. The other system advances with a constant velocity Um positive x-direction. This system is called the directionally fixed system; o-xyz. The x- and
y-axis are located in the undisturbed free surface, and the z=axis points vertically upwards; The displacement of the
body fixed system with respect to the directionally fixed system is only small; The displacement is described by
three translations: and,' in x-, y- and z-direction respectively, and three rotations: 114, 15and 116 around the
x-, y- and z-axis respectively.
The six small displacements i ...i1 are the actual
unknowns of the problem. Two additional unknowns will occur: the excess pressure in the air cushion plenum
and the excess pressure in the bag stern seal plenum p3.
Up to now heave (ib) and pitch
(115) are the onlydisplacements that are considered iñ the actual program,
so it is only suitable for head and following seas.
EQUATIONS OF MOTION
The equationsof motion followfrom Newton second law:
6
d2'rlk
= F1
j = i...6,
(1)k-1 dt2
where MJk is the generalised mass matrix, t denotes time
and F...,F6 are the total force acting on the vessel in x-,
y- and z-direction and the total moment acting on the vessel around the x-, y- and z-axis respectively. For conveniencethe moments around the x-, y-and z-axis will
be designated force in 4, 5" and 6th direction. The total force in
f
direction acting on the vessel can be divided into several components:F1 = F°+ F?»+ F4'+
a) (2)where the affix denotes gravitational force (g), propulsive force (p), hydromechanic force (h), air cushion force (a) and seal force (s) respectively. The propulsive force is assumed to be balanced by the resistance of the vessel. The hydromechanic force, the air cushion force and the seal force Will be treated in following Sections.
CUSHION AND SEAL DYNAMICS
In this' section two additiönal equations for the two
equations follow from the equations of continuity for the
air cuhion and stern seal plena.
The equation ofcontinuity for a plenum reads:
p(Q(fl) Q(OUI))
= _.(pV),
(3)where d" is the air volume flux into the plenum, d"u is the air leakage volume flux from the plenum, p is the density of air, and V is the volume of the plenum. The
equation of state for the air in the plenum isgiven by the 'isentropic gas law:
Pa + P
______ = constant,
piC
where Pa S the ambient pressure, p is the (spatially
constant) excess pressure in the plenum, and = 1.4 is
the ratio of specific heats for
air. The equation ofcontinuity and the equation of statecan be combined and rearranged to:
V dp (Q(ifl) - 0(01)1)) -
f.
'«PPa) dt
dt(4)
(5)
The air volume flux through a fan into
a plenum d is
appoxirnated by the stationary fan characteristic
linearised in the design operation point:
0(in)
=
5
+ (6)where S is the design flux through the fan, and ¡s the design excess pressure in the plenum. Sullivan eta([1'81 showed the importance of a dynamic model for the fan of
air cushions. They determined the 'linear dynamic response of a fan from experiments. The dynamic characteristics of full scale fans is not known however. The author is not aware of any theoretical dynamic fan
model.
The air leakage volüme flux from a plenum dohlt) ¡s
calculated from the orifice flow formula:
= (7)
where c is the orifice coefficient, A1 is the leakage area
and tip is the pressure Jump across the orifice. The
orifice coefficient depends on the local geometry of the
orifice. For a sharply edged orifice like the leakage gap
3
under the front seal it can be set to 0.61, while for a
smoothly rounded orifice like the leakage gap under the stern seal it may be set to 1.0. A derivation of equation
(7) and an elaborate discussion on the choice ofc1 can be
found in Ulstein[4]. Theleakage areas under the fore and
aft seals follows from the seal modéls. Thisarea is highly
non-linear in the relative motions.
The system of plenaof a SES and the volume fluxes 'into
and out of these plena are presented in Fig. 1. The equations for the cushion excess pressure p and the seal
excess pressure p5 are now written as:
V dp (Q(lfl) Q(OU1)) dV
+ Pa) dt
V dp5 (Qfl) Q(OU1)) dV5
+ Pa) dt
(in) (in) (in)
where Q = + which is the sum of the flux through the cushion fan and the leakage flux frOm the
(ouf) (out) (ouf)
stern seal, and = Qe,, , which is the sum
of the leakage flux under the foré seal and the leakage flux under the stern seal, (see Fig. 1). The air cushion volume V5is expressed (up to linearorder:jn i 1,...,r6) as:
VC = C - V5 +
ff(13 +
14 + Xii5) dS + dS,,deck FS
(9)
where V is the design cushion volume, V5is the part of
the cushion volume that is taken up by the stern seal, Ç is
the wave height in the air cushion and FS is the part of the free surface that is covered by the air cushion. The volume of the stern seal plenum V and the volume of the air cushion that is taken up by the stern seal V5 follow
from the stern seal model, which is treated in the next
section. The wave height in the air cushion Ç is calculated
by means of a three-dimensional panel method.
The air cushion force follows from integration of the air cushion excesspressure pover the deck and the side
'hulls.
The equations of motion ('1)
and the equations of
continuity for the cushion and stern seal (8) plena are
solved simultaneously in a time simulation procedure. A Runge-Kutta scheme is used. The simulations result in time traces'Ofthedisplacements, velocities, aelerations, excess pressures and air leakage areas.
5. SEAL MODELS
A two-dimensional model ('x-z-plane) for the flexible
bag-type stern seals of' SES' hasbeendeveloped. Usually
a stern seal has two or three lobes. Each lobe consists of a loop of thin flexible, material. These loops are open to the sides, where the bag is closed by the hulls of the SES. The bag is pressurised by a fan at a slightly higher pressure than the air cushion pressure. The wave height
and wave slope are assumed to be constant over the width of the ir cushion. The gravitational and inertial forces on the bag are neglected. The following variables determine the bag geometry: heave and pitch
displacement, excess pressures in the cushion and the seal plena, and wave height and wave slope at the seal. The bag geometry is calculated in a static way. However,
the complete seal: model is not static through the cushion
and seal dynamics.
The three-dimensional bag membrane is analysed as a two-dimensional cable.
The cable has no bending
stiffness and only transmits tension. Force equilibrium for a cable segment yields the following relation:
where T is the tension in the cable, p is the pressure differenc6 across the seal and Ris the radius of'curvature of the cable.
When the seal does not touch the water surface, air will
leak from the cUshion will. This air flow results in a
pressure distribution under the seal. This air leakage flow has been studied elaborately by Ulstein[4]. He 'foundthat a simple one-dimensional analysis gives good results.
This one-dimensional analysis leads to the following
pressure distribution:
where p(x) is the spatially varying excess pressure under the seal, p is the excess pressure in the air cushion, h, is
the height of the air leakage area, and h(x) is the local
height of the seal above the wave surface (see Fig 2).
The derivation of the set of non-linear eqUations that
govern the bag geometry is quite lengthy, and is therefore
omitted in this paper. The equations can be found in
Moulijn[23]. Newton-Raphson's method is used for
solving the non-linear system.
V24 = O
g_ +
-
2U.!
+ U2.! + !(.
-
U.E) = Oàz 7
axat ax2p at
àxVil,= Un1
6 °'Ik + (._._ + k.1 4When the geometry of the bag and the tension in the bag membrane, which is also a part of the stern seal solution, are known, the seal force F!5' , the volumeof the seal V5,
the volume of the cushion t(iat is taken up by the seal V
and the air leakage area can easily e calculated. A
typical solution of the bag geometry is presented by Fig.
2.
In the equations (8) the time derivatives of V5 and V5
occurred. Direct evaluation of dV5/dt and dV5/dt is
difficult. Lee[1O] uses a finite difference scheme using previous time steps. He needs a filtering technique to preventamplification.ofthetruncation errori Thereforethe following expression for dV/dt will be used:
dV
av.
av.
av.
=___3
+_75+_
+dt & ai15 ap
av
av.
(10) Ps + - +
(12)
where Vis either V5 or V5, Ç and Ç are the mean wave
height and wave slope at the seal and a dot denotes
differentiation with respect to time. The partial derivatives
of V5 and V5 can be found from finite differences, as 113,
115' p6, Ç and Ç are 'input variables of the seal model.
The fore seal of SES is usually of the finger type. The
fingers consist of vertical loops of thin flexible material. The loops are open lo 'the cushion side When the local
deck height is smaller than the height of the seal, the
lower part of the fingers' is simply bent backwards at the water'surface, and no air will leak under the seals. When the local deck height is larger than the height of the seal, the seal will leave a gap above the free surface, and air
will leak from the cushion. The frictional forces of the
water on the fore seal are neglected.
6. HYDRODYNAMICS
The hydrodynamic problem is solved by means of a
3-dimensional Rankine' source panel method. The flow is
assumed to be incompressible and nonrotatiönal, so
potential flow theory can be used
The boundaryconditions on the hulls añd the free surface are linearised around the undisturbed flow (Neumann-Kelvin
linearisation) This leads to the following boundary value
problem:
field equation
on the free suilace
on the hulls
whereg is thegravitational acceleration constant, is the perturbation velocity potential, p is the excess pressure at the free surface (equals zero outside the air cushion) and
F is the normal vector pointing into the fluid domain.
Further, T (n1,n2,n3)
= n
(n41,n5,n6).TØ
(mi,m2.m3.)T (m4,,m5,m6)T= (O,Un,Un2)T,
where X is the vector to some point ori the hulls. A
radiàtion condition is 'imposed ensuring, that no other waves than the prescribed incident waves propagate
towards the vessel.
Application of Green's second identity to the unknown
potential and the Rankine source potential G(.f)ioads to a Fredholm integral equation of the second 'kind
=
_J
f5
G(Z )dS' +
2it an"
Lff) .L
G(Z)
2lts
where S is the boundary of the fluid domain, and aia n denotes differentiation in the direction of the normal
vector.
fle normal derivative of
follows from the appropriate boundary condition (13). The hulls and ¿ part of the free surface are panelled using flat quadrilateral panels having a constant source and dipole distribution.In the middle of each. panel. a collocation point is defined
where the integral equation is satisfied. This leads tothe following, linear system of equations:
Òi=-._
ff.i')dS'
' paneli (14) (15)+j_.jf _G(')dS'
panoli anwhere j = i...N and N is the number of panels. The
tangential derivatives of the potential, that occur in the freesurface boundarycondition, followfrom differentiation of a bi-quadratic splirie approximation, of . Nakos[24J
also uses this spline scheme, but 'he uses a quadratic
singularity distribution on the panels.
When the boundary valúe problem for is solved, the pressure pand the wave height follow from:
p-= -p(.. -
u.P_ + gz)(.16)
ç =
- U.)
gat
ax5
The hydrodynamic forces follow from integration of the pressure overthe hulls. Details of the panel method can be found in Moulijn(25].
The hydrodynamic problem is solved in the frequency domain, thus avoiding a complicated time stepping
algorithm and saving muchcomputational time. However,
as non-linear cushion dynamics will. be implemented, the motions have to be solved in a time simulation procedure.
Therefore the theory of Cummins(26] and Ogilvie[27] is used to transform the frequency domain results of the panel method to the time domain.
7 RESULTS
In this section the results of the computational method will
be presented and compared to experimental data. All
results concern the target vessel of the HYDROSES project (see Kapsenberg and Blúme[22]). The main dimensions of this vessel are can be found in Table 1..
TABLE i Main dimensions
The Rit to weight ratio of the vessel is about 0.85. The vessel sails in head waves at a speed of' 45 Kn. In the
experiments a diaphragm was used to obtain a proper
scaling of the air cushion dynamics (Kapsenberg and
Blume[22fl. In the computations' the full scale ship was
modelled. The hydromechanics 'are linearised around the mean sinkage and trim of the higher frequency
experiments. This position corresponds to = 0.0 m and 115 = -0.0115 rad.
Figure 3' presents the time traces of a simulation in
regular 'head waves The figure presents the following traces incident wave height at station 10 (Ç, in m) heave displacement (1 in m) pitch displacement ( in rad),
cushion and stern seal excess pressure (p and PS ri
kPa) air leakage gap height at the front and at the stern seal (hI,and h!5 in rn) and vertical acceleration at station
O (A0 in m/s2), station 10 (A10 in m/s2) and station 20 (A20
in mis2). No higher harmonics can be observed in the
displacements signals. In the pressure and acceleration signals higher harmonics, caused by non-linearities, are clearly present. The signals of the escape height under the fore and stern seal illustrate the non-linear nature of air leakage. Note that the cushion excesspressure signal
is strongly' correlated to the vertical acceleration at station
10. The air cushion gives the 'largest contribution to the
vertical force, which is proportional' to the vertical acceleration of. the vesseL
L0
.1 530Om L 144.0CmB 35.00m
26.00m
Figures 4 and 5 present the Response Amplitude
Operators (RAO's) for heave and pitch displacement of the vessel. These RAO's give the amplitude of the
displacement divided by the wave amplitude. Theyare
based on the first harmonic component of the, time
signals. Results for several levels of wave steepness
(kA)are shown.
For those waves having a larger
steepness than kA = 0.01 it was impossible to findproper
solutions for the stern seal in a range around the pitch resonant frequency, because ofthe large relative motions
at the stern seal. The effect of wave steepnesson the RAO's appears to be very limited. The computed heave displacement agrees very well with the experiflentaldata. The computed pitch displacement agrees well with the
experiments in the intermediate and high frequency range.
In the low frequency range the computational resultsare much larger. At first, when no stern seal model was
implemented, the stern seal was expected to dampthe
pitch resonance. This prcved to be wrong; the sternseal
only shifts the pitch resonance frequency to a slightly higher frequency. Now this discrepancy is attributed to
the hydrodynamics. Probably the poor modelling of the flow around the transomsof the side hullscauses the lack of damping. Viscous effects also might play sorne role.
On the other hand the experimental results might be
affected by the connections between the model and the
carriage (cables and flexible hoses of the air supply
system).
Figures 6 and 7 present the RAOs for the first harmonic
component of the cushion and the seal excess pressure.
The computational and experimental results for the
cushion excess pressure agreequite well. The correlation
for the seal excess pressure is rather poor. In the experiments the seal pressure appears to follow the
cushion pressure. This might be attributed to a difference
in the air supply system of the stern seal.
In theexperimental model the air from the aft fan is fed into an
air supply box, which distributes the air over the seal and the cushion. Air also flows from the seal via.special ducts
to thecushion. In the computational model allair from the aft fan is fed into the seal. Again air flows from the seal
to the cushion, but not via special ducts.
Figure 8 presents the RAO for the vertical accelerationat station 10. However, this RAO is not based on the first harmonic component of the acceleration signal. Il gives the peak accelerationjevel divide&by thewave amplitude.
The RAO based on the first harmoniccomponent would have shown only a small dependence on wave height, just
like the RAO for the cushion excess pressure (Fig. 6). The RAO based on the peak level shows considerable
dependence on wave height. As the first harmonic
component is not very sensitive to wave, height, this has to be caused by higher harmonic components.
Figure 9 presents the sinkage of the vessel. Waveheight
has an important effect on the amount of air leakageand
hence on cushion excess pressure. A decrease in cushion pressure. causes the draught
of the SES to
increase. The experimental data in this figure are
selected from the total set of'
data, to have a wavesteepness (kA) that differs not too much from 0.05. The
6
experimental and computational data differ considerai
but the Irend is the same. The difference might caused by a poor prediction of the steady hydrodynar lift force on the side hulls. Another likely explanation ¡
somewhat :10w cushion excess pressure during I
experiments.
Figures 10 and 11 present the effect of sev
simplifications and scaling on the computed h02
displacement and cushion excess pressure. The effect
pitch motion is generally very small.
The first simplification was the linearisation of the st seal around a mean posftion When the air leakage ai under the stern seal gets negative it is set equal to ze
so air leakage is retained in non-linear form. The effect
this simplification appears to be very small, afthoug
should be mentioned that the effect on sinkage and higi
harmonics is much larger. This simplification is vi
attractive; the computational burden is reduced a lot, a
the method gets more robust, as no difficult stern si
solutions have to be found for every time step.
The second curve is
the result of a simple 11mfrequency domain:calculation. In this calculation the st
seal and air leakage where neglected. The results
poor, and the method of course gives no informati
about sinkage. and higher harmonics.
The third curve is a result of a non-linear simulation, I the interaction of the air .cushion and thewave surf 2
was neglected. This implies that the waves generated the oscillating cushion pressure are neglected and ti
theincident waves are assumed toipropagateund isturb
through the air cushion. The effect of this simplificati
appears to be limited. However, when the resoni
frequency of the air cushion is not damped as much the fan system and air leakage under the stern seal, ti effect becomes much more important. Inprevious studi neglecting cushion surface interaction appeared to sI
the resonant frequency of the air cushion downwar
(Moulijn[25]). The hypotheses of Kaplan[12J that t
vessel induced waves only have a minor effect on t motions cannot be confirmed
The fourth simplification implies neglecting the fan slot
i.e. assuming that the volume flux through the fans
constant. The effect appears to be very large. The f system appears to have a large damping effecton the
cushion resonance. This shows that the fan system h an important effect on the motions of SES Perhap5
more sophisticated fan model should be implement
Finally the effect of scaling is shown.
The amu
pressure was raised a factor ten in order to simulate t motions of a t:10 scale model Without a device to sci the air cushion dynamics. The scale of models is usu2
much smaller than 1:10, so much care must be taken the proper scaling of cushion dynamics.
8. CONCLUSIÓN
The results of the computational method are generally
although some discrepancies occur. The linearisalion of.
the stern seal model only has a small effect on the results. Air leakage appears tobe an important effectthat cannot be. neglected. The effect of the interaction of. the
air cushion and the wave surface. is limited, but this
interaction cannot be neglected.. The fan system appears
to have an important effect on the results; Scale effects that occur during experiments are important.
ACKNOWLEDGEMENT
The author would like to thank the Royal Netherlands
Navy and the Matime Research Institute Netherlands for their financial support of this research project.
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STEEN, S: 'Cobblestone.Effect onSES', PhD thesis, Norwegian Institute of Technology, 1:993.
ULSTEIN, T: 'Nonlinear Effects of a Flexible Stern Seal Bag on Cobblestone Oscillations of an SES',
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7
1.0. LEE, G J: 'On the Motions of High Speed
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-7
Transverse Section
Q(OUl)
Q(l)
Longitudinal Section
Fig. i Transverse and longitudinal section of a Surface Effect Ship
deck
wave surface
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8
Fig. 2 Typical solution for a 3-lobe flexible stern seal
JcJ
cushion plenum
('s'
i
% I I I I'
l
I I % I ,1\
j
I I\
hi1!
\
,I IJ
9 5 1:0 15 20 t [s]173
RAO'
[rn/rn]
1.21-
0.8-
0.6-
0.4-
0.2-o 00.03
0.025
0.02
-1/50.015
-Erad/ml
0.0'l
-Pc[kPa/rn]
65-
4-9 1 o+
simulation kA = 0.01
simulation kA = 0.05
simulation kA
0.10
simulation kA = 0.15
MARIN experiments
+
I Isimulation kA = 0.01
simulation kA = 0.05
--simulation kA = 0.10
simulation kA = 0.15
MARIN experiments
+
simulation kA = 0.01
simulation kA = 0.05
simulation kA = 0.10
simulation kA = 0.15
MARIN experiments
+
+
2 3[rad/s]
lo
4Fig. 5 Response amplitude operator for pitch
5
O 1 3 4 5
We
[rad/sJ
Fig. 6 Response amplitude operator for cushion excess pressure
0.005-(J
O
i
i 2 3 4
We
[rad/s]
Fig. 4 Response amplitude operator for heave
PS
kPà/rn]
A}0RAO
sinkage
[m]0.4
0.2
o-
-0.2-
-0.4-
-0.6-
-0.8-
-1--5+
simulation kA = 0.01
simulation kA = 0.05
simulation kA = 0.10
simulation kA = 0.15
+
1+ I 11 1 2 3 4 5w [radis]
Fig. 9 Sinkage (positive üpwards)
simulation kA
simulation kA =
simulation kA
simulation kA =
experiments kA
I001
0.050.10
---0.15 0.05+
i
2 3 4 We[rad/s]
Fig. 7 Response amplitude operator for seal excess pressure
1 2 3
4
5We
[rad/s]
Fig. 8 Response amplitude operator for acceleration at station 10
+
I Isimulation kA = 0.01
simuiation kA = 0.05
simulatión kA = 0.10
simulation kA = 0.15
= =MARTh experiments
+
13
RAO'
{m/m]
PcRAO'
[kPa/ m]
1.2
10.8-
0.6-
0.4-
0.2-0 1210-
8-
6-I Ilinearised stern seal
linear frequency domain ----
-no cushion-surface interaction
no fan slope
scale effect (1:10. model)
MARIN experiments
+
+
I I
linearised stern seal
linear frequency domain
no cushion-surface interaction
no fan slope
scale effect (1:10 model)
MARIN experiments
+
.5.-
5.S/
+
o O 12 o 1 2 3 4 5w [rad/s]
Fig. lo
Effect of several simplifications on heave RAO, kA = 0.05'S * 't