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ASTERN OF MODEL 5415
An Experimental and Computational Study of the Effects of
Propulsion on the Free-Surface Flow Astern of Model 5415
T.Ratcliffe (Naval Surface Warfare Center, Carderock Division, USA)
ABSTRACT
Experimental measurements of the Kelvin wake, and the near- and far-field wave field, both with and without the
model propeller operating, were obtained from a surface ship model representing the preliminary design of the DDG-51
hull form, represented by DTMB Model 5415. Wave height measurements were performed in the Carriage II basin at
David Taylor Model Basin (DTMB) using two different techniques. The first technique uses capacitance probes attached
to the side of the model basin to obtain longitudinal wave cuts. The second technique uses mechanical probes attached to
a traversing system at the stern of the model to measure the surface wave field behind the model. The data from the
mechanical probes are used to generate a wave height topography map. The results from both measurement techniques
are used as a basis for comparison with computational fluid dynamics (CFD) predictions. Free-surface predictions from
Mississippi State University's UNCLE code, with a. propeller body force-model incorporated, are documented and the
trends are compared with the experimental data.
INTRODUCTION
An ONR Free-Surface Flow Initiative for validating and transitioning to industry Reynold's Averaged Navier Stokes
and Potential Flow computational codes was begun in 1995. Model 5415 was chosen as a representative naval combatant
hull form on which a rigorous set of experimental data would, be obtained. The model has been tested both bare hull and
appended. The data base includes bare hull resistance and wave field measurements, nominal wake velocities obtained
with pitot tubes as well as velocities astern of the operating propeller measured with Laser Doppler Velocimetry The data
base can be accessed from the Model 5415 web site at http://www50.navy.mil/5415. This paper documents the free-
surface wave height data obtained on the appended model, both with and without the propellers operating.
As part of the ONR Free-Surface Initiative, computations of the free surface flow and sub-surface velocities were
obtained on the bare hull model with two RANS prediction codes, UNCLE and University of Iowa's CFDSHIP. In
addition to the RANS predictions, potential flow codes including SWAN, LAMP, and UMDELTA, were also used to
predict the free surface flow around the model. The results of this effort along with descriptions of the prediction codes
are documented in Ratcliffe (1998).
MODEL DESCRIPTION
Model 5415 was built of wood in 1980 to a linear scale ratio of 24.824 and is representative of a modern naval
combatant hull form. Electronic files representing the geometry of the hull form, both bare hull and with appendages can
be downloaded from the Model 5415 web site. Figure 1 shows a photograph of the stern of the model, fully outfitted for
this experiment with removable appendages (shafts and struts). The model has twin rudders which are set at an angle of
zero degrees relative to the model centerline. The model was not fitted with bilge keels. Turbulence stimulator studs 3.2
mm in diameter and 2.5 mm in height were fitted to the model in accordance with Hughes and Allen (1951).
Figure 1—Model 5415 with Removable Appendages (shafts and struts)
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During the propelled experiments, the model was fitted with design propellers designated as DTMB
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ASTERN OF MODEL 5415
propellers 4876 and 4877. These represent 5.49-meter full-scale diameter propellers. A photograph of the propellers on
the model is shown in Figure 2. Figure 3 shows an isometric view of the appended model. Table 1 provides model
dimensions and other particulars.
Figure 2—DTMB Propellers 4876 and 4877 on Model
Figure 3—Isometric View of Model 5415
EXPERIMENTAL PROCEDURES
The experiments described herein were obtained both with and without the propellers operating. To obtain the most
accurate free-surface measurements, in these experiments the model was mounted in a fixed trim condition corresponding
to the running trim of the model at a Froude number of either 0.28 (2.06 m/sec) or 0.41 (3.10 m/sec). When the
measurements were obtained with the propellers operating, the propeller RPM was set at the ship self-propulsion point. A
table of operating conditions of the propellers during the propelled experiments is presented in Table 2.
During these experiments, two techniques were used to measure wave heights generated by the model. The first
technique measures longitudinal wave cuts using stationary capacitance probes fixed to the side of the basin. The second
technique measures wave heights in a rectangular area aft of the stern using mechanical whisker probes attached to the
towing carriage aft, of the model.
Table 1—Model 5415 Dimensions and Particulars
Lambda 24.824
LBP, LWL 5.72 m
Displacement 548.8 kg
4.92 m2
Appended Wetted Surface
Sinkage at FP (Fn=0.28) −0.0027L
Sinkage at AP (Fn=0.28) −0.00086L
Sinkage at FP (Fn=0.41) −0.00054L
Sinkage at AP (Fn=0.41) −0.0083L
Propellers Port 4877
Starboard 4876
Propeller Diameter 22.10 cm
Table 2—Propeller Operating Conditions (KT and KQ determined from open water tests; D is propeller diameter, n is revolutions
per second)
KT=T/(pD4n2) KQ=Q/(ρD5n2)
Speed, V (m/sec) RPM J=V/nD
2.06 0.178 0.0461 436 1.28
3.10 0.232 0.0562 722 1.175
The following discussion of experimental procedures is divided by technique used, and then further divided into four
sections; theory of operation, experimental setup, calibration, and operating procedures.
LONGITUDINAL WAVE CUTS
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Theory of Operation
The sensing element of the capacitance probe is a 30-gauge (AWG) silver-plated copper wire with 0.11 mm kynar
insulation, 38.1 cm in length. Attached to the sensing element is a weighted 1.21-m length of mylar fishing line, used to
provide probe stability in waves. The sensing element is suspended with half its length submerged in the basin. The basin
water provides the ground reference for the sensing elements on
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ASTERN OF MODEL 5415
the circuit card. With the copper wire completely insulated from the water, the sensing element behaves as a capacitor
with one plate being the copper wire, the second plate the water, and the wire insulation acting as the dielectric. As waves
in the basin change the submerged height of the sensing element, they change the effective capacitor plate size, which
results in a change in capacitance. The change in capacitance is proportional to the wave height. By attaching the wave
wire, a varying capacitor, to a timing circuit, a d.c. voltage is generated that is directly proportional to the capacitance of
the probe and, therefore, the wave height being measured.
Experimental Setup
A wave boom (truss section), cantilevered from the basin wall over the water, provides a structure from which the
instrumentation is mounted. The wave boom extends 6.83 m from the basin wall. A motorized uni-slide with an attached
horizontal bar is mounted vertically on the wave boom. The capacitance probes' electronics are mounted on the horizontal
bar of the uni-slide. The uni-slide allows precise placements of the probes' vertical position, probe emergence, used
during static calibration of the probes. Figure 4 shows the longitudinal wave cut hardware in place in the basin.
Two probes were used for this experiment. The placements of the probes are referenced to centerline of the model,
with probe number 1 being inboard and probe number 2, outboard. The probe placements are provided in Table 3.
A photo sensor is set to trigger data collection when the forward perpendicular of the model reaches a predefined
distance from the wave probes. A 133 MHz Pentium-class computer, using an ADC488 16-bit analog to digital (A/D)
converter, collects and stores the data.
Table 3—Longitudinal Wave Cut Probe Locations
Probe Number Transverse Distance from Model Centerline (y) y/B
1 0.56 m 0.73
2 15.44 m 2.44
Calibration
Insitu calibrations are performed after the completion of the test setup. In order to calibrate the probes, the motorized
uni-slide is traversed in 2.54-cm increments for a total of ±7.62 cm. Data is collected at each increment for each of the
probes. A straight line fit is performed and a slope is calculated and stored for each probe. The insitu calibration permits
calibration of the probes, the signal conditioning amplifiers, and the A/D converter as a system.
Figure 4—Longitudinal Wave Cut Set Up
Operating Procedures
Probe zeroes are collected in calm water before each run. The model is then run past the probes at a constant speed.
As the model approaches the test section, a strip of reflective tape positioned on the carriage triggers a photosensor placed
at the side of the basin which starts data collection. The position of the photosensor and the duration of data collection is
adjusted to insure that the maximum amount of data is collected before tank wall reflections occur. Data is filtered at 10
Hz with a 3 pole Bessel filter and collected at a sampling rate of 100 Hz for 20 to 30 seconds depending on model speed
and photosensor position.
Data analysis is performed on the PC after each run. First, calibrations are applied to the A/D voltages, and then the
probe zeroes are subtracted. The data from each probe is then plotted to ensure that the measurements are of good quality.
Further analysis on the longitudinal wave cut data is often performed in order to compute free wave spectra and wave
pattern resistance.
STERN TOPOGRAPHY
Theory of operation
The whisker probe is a vertically oriented, mechanical probe, that continuously searches for the free surface. The
sensing element of the probe is a 0.38 mm diameter, 5.08 cm long stainless steel wire. The wire is mounted in a copper
tube that makes up the body of the probe. A geared rack, attached to the probe body, allows the probe to be driven up and
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down, vertically, by a servomotor. Opening and closing a circuit between the probe and the water is sensed by an
electronic circuit which drives the servomotor. When the probe is not in contact with the water surface there is an open
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ASTERN OF MODEL 5415
circuit and the servomotor drives the probe down towards the surface of the water. Once contact is made between the
probe and the surface of the water, a closed circuit is sensed and the probe is driven up, out of the water. This process is
repeated continuously, causing the probe to oscillate around the free surface at approximately 20 Hz. The probe is
connected to a potentiometer that tracks its position along the z-axis (wave height). Probe position is recorded by a
sample and hold circuit during the instant the probe makes initial contact with the water surface. This manner of sampling
probe position alleviates position error from meniscus effects, due to surface tension.
Experimental Setup
To create a topography of the free surface at the stern of the model, four probes are mounted together on a bracket
attached to a uni-slide. The probes are oriented in the longitudinal direction, parallel to the centerline of the model, with a
5.08 cm spacing between probes. The probes operating behind Model 5415 can be seen in Figure 5. The array of probes
are attached to an XY-traverse that is mounted to the carriage at the stern of the model. Two string pots attached to the
traverse are used to track the longitudinal (X) and transverse (Y) positions of the probes. A 133 MHz 486 computer, using
an ADC488 16-bit A/D converter, collects and stores the data. The data collection computer is networked with a 350
MHz Pentium II laptop computer that is used for data analysis and plotting. Data are filtered at 10 Hz with a 3-pole Bessel
filter and collected at a sampling rate of 100 Hz.
Figure 5—Whisker probes operating behind Model 5415
Calibration
Static calibrations are performed on the whisker probes in the lab, prior to the experiment. The probes are positioned
over a container of water, and allowed to track the calm free surface as the uni-slide is traversed in 2.54-cm increments
for a total of ±7.62 cm. Data is collected at each increment for each of the probes. A straight line fit is performed and a
slope is calculated and stored for each probe.
Operating Procedures
The forward most probe is aligned longitudinally (X) and transversely (Y) with the aft perpendicular and centerline
of the model respectively. The longitudinal and transverse string pots are zeroed at this location, and all future
measurements are referenced to this position. In order to collect the data needed to generate a complete topography of the
stern area, the area is divided into a number of transverse cuts. One transverse cut collects an area of 15.24 cm by 1.32 m.
Starting as close to the stern of the model as possible (1.27 cm), successive transverse cuts are made with an advancement
of 20.32 cm along the x-axis between cuts. For this experiment the completed mapped area measured 1.32 m by 2.38 m.
The possible number of transverse cuts per run is dependent on model speed. Once the number of traverse cuts per
run is determined, a command file is generated which controls the positioning of the probes during the run. Prior to each
run a zero collection is performed. A zero run consists of performing an identical collection run of transverse cuts, but
with the model stationary. This procedure eliminates bias errors due to misalignment or sagging of the traverse's XY-
plane relative to the surface of the water, which should be parallel to one another. After the zero run is performed, the
model is brought up to a constant speed and a collection of transverse cuts are started. This process is repeated at
successive transverse locations until the desired area behind the model has been completely mapped.
Analysis of the stern topography data is done by applying the calibration factor to the A/D voltages from the at-speed
data and the zero-speed data, and then subtracting out the zero-speed data to produce a set of zero-compensated data.
Next, filter coefficients are calculated for a Butterworth filter with an optional number of poles, chosen by the user (in this
case, 3 poles were specified.) The zero compensated probe data is then filtered in both directions to eliminate data phase
shifts. The next step before plotting, is to extract data from the data, set. A grid pattern is established with an x-value at
every longitudinal probe position and a y-value which starts at the beginning of each transverse probe position and
extends to the ending probe position, in increments of 0.5 cm. Probe data closest to the desired grid locations are extracted
from the data set and saved. These data are then placed into a format for
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ASTERN OF MODEL 5415
plotting the stern topography contour maps, using TECPLOT software. It is important to note that these contour maps
represent the average of a time-varying data set with an RMS variation about the mean contour level.
PRESENTATION OF RESULTS
The coordinate system for the measurements is difined with the x-axis being parallel to the model centerline, the y-
axis athwartships and the z-axis perpendicular to the calm water surface. All data and axes have been non-
dimensionalized using the model length. The forward perpendicular is denoted at x/L=0, and the aft pependicular as x/
L=1.0.
Longitudinal Wave Cut Measurements
Longitudinal wave cuts for Model 5415 with and without propellers operating, at Froude numbers of 0.28 and 0.41,
are shown in Figures 6 and 7. A longitudinal wave cut can be characterized by four waves or wave systems. The first
wave is the “bow wave,” generated by the bow and shoulder. The bow wave is followed by the waves generated along the
mid-body, followed by a “stern wave,” generated by the stern. Lastly a set of transverse waves decaying behind the model
are observed. At a Froude number of 0.28, at the inner probe location of y/B of 0.73, the effect of propulsion is dominant
in the transverse wave system aft of the model. With the propellers operating at 436 RPM, there is a 10 percent increase
in the transverse wave heights over the unpropelled case. The effect of the operating propeller is particularly noticeable in
the amplitude of the stern wave, which is augmented by 20 percent. At the outer probe location (y/B is 2.44) the effect of
propulsion on the stern wave is less; only accounting for an increase of 10 percent. There is also a noticeable phase shift
in the transverse wave system between the unpropelled and propelled condition. The transverse wave system of the
propelled model is shifted aft by 12 percent of the transverse wave length (2πV2/g). This phase shift is more evident at
large values of x/L.
At a Froude number of 0.41, where the propellers operate at 722 RPM, propulsion has a minimal effect on the wave
system, accounting for only a 6 percent increase in the stern wave amplitude and 2 percent increase in the amplitude of
the transverse wave system at the inner probe location. At the outer probe location, propulsion accounts for a 9 percent
increase in the stern wave amplitude and a negligible increase in the amplitudes of the transverse wave system. At this
speed, the large stern wake is dominated by the flow around the transom stern, so the effect of the operating propellers is
less evident than at a Froude number of 0.28.
The effect of propulsion on the longitudinal wave cuts generated by a model representing another combatant hull
form has been shown to be larger than seen here for Model 5415. This data set is presented in Lindenmuth and Ratciffe
(1989).
Stern Topography
A comparison of the propelled and unpropelled near-field wave systems at a Froude number of 0.28, measured with
the whisker probe, is shown in Figure 8. The difference between, the two conditions has been quantified in Figure 9.
Propulsion increases the wave amplitudes along the stern wave crest line on the order of 35 percent. In the region behind
the stern, between an x/L of 1.05 and 1.15, propulsion effects account for local increases in wave heights of 25 to 35
percent. At this Froude number the flow is still attached to the transom.
At a Froude number of 0.41, the transom is completely clear (dry) and the flow converges in a highly turbulent
region covering an area of 0.15 ship lengths, longitudinally by 0.05 ship lengths, transversely. Figure 10 shows the
differences due to propulsion in the wave field behind the transom at a Froude number of 0.41. Figure 11 serves to
quantity those differences. The differences due to propulsion at this
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Figure 6—The Effect of Propulsion on the Far-field Wave System as Measured with Stationary Capacitance Probes, at a
Froude number of 0.28
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ASTERN OF MODEL 5415
higher Froude number are more scattered over the complete stern area than was the case for the Froude number of 0.28.
The effect of propulsion accounts for differences on the order of 20 percent in two regions; along the stern wave crest
and, aft of the transom. The area aft of the transom, located at an x/L of 1.2 is farther downstream than the affected area at
a Froude number of 0.28. At this higher Froude number, the propellers have a smaller effect on the stern wave system
than they do at a Froude number of 0.28.
Figure 8—The Effect of Propulsion on the Near-field
Wave System of Model 5415 as Measured with Whisker
Probes, at a Froude Number of 0.28.
Figure 7—The Effect of Propulsion on the Far-field
Wave System as Measured, with Stationary Capacitance
Probes, at a Froude number of 0.41
Figure 9—Stern Topography Differences (Propelled-
Unpropelled) in the Near-field Wave System of Model
5415 at a Froude number of 0.28
Figure 11—Stern Topography Differences (Propelled-
Figure 10—The Effect of Propulsion on the Near-field Unpropelled) in the Near-field Wave System of Model
Wave System of Model 5415 as Measured with Whisker 5415 at a Froude Number of 0.41.
Probes, at Froude Number of 0.41.
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ASTERN OF MODEL 5415
MEASUREMENT UNCERTAINTY
Measurement uncertainty has been determined for both the longitudinal wave cut and whisker probe data, at each of
the two speeds where data were obtained. The analysis is in accordance with standard uncertainty analysis practices of the
“Guide to the Expression of Uncertainty in Measurement” as documented in 1993 by the International Organization for
Standardization (ISO), and explained further in ANSI/ASME (1998) and the AIAA Standard (1998). Detailed
explanations and examples of the uncertainty analysis are given Coleman and Steele (1998).
For each speed and condition at which wave cuts were conducted, a mean wave was calculated from the repeat
passes that were collected. The mean wave from these repeat passes was calculated by averaging Z/L (the wave heights),
at each X/L, (the longitudinal distance from the aft perpendicular). Seven repeat passes were collected at a Froude number
of 0.28 for the propelled and unpropelled condition, and eight repeat passes were collected at a Froude number of 0.41.
For the whisker probe data, transverse cuts were used to calculate the mean waves in the transverse direction (Y/L). Six
repeat runs were obtained at a Froude number of 0.28 and nine at a Froude number of 0.41.
The precision limits are based on the standard deviations of the wave. The standard deviation at each X/L or Y/L
location is calculated when the mean wave is averaged from the repeat passes. The standard deviations across the whole
wave are multiplied by the proper student-t value scalar from the 95% certainty curve to produce the precision limits.
These precision limits, vary with the position in the wave, usually greater at the crests and troughs of the wave than at the
zero-crossings.
The bias limit is determined by calibrations done insitu and are a scalar applied across the entire mean wave. The
uncertainty is computed by the root-sum-square of the bias and precision limits (also commonly referred to as the
systematic and random errors).
The combined uncertainty for the propelled and unpropelled condtions are presented in Table 4.
COMPUTATIONS
Computations were performed with the UNCLE code from Mississippi State University. This time-accurate, steady
incompressible RANS code has been used extensively to compute the free-surface flow field around surface ship models.
(Beddhu, 1998).
A propeller body force model was introduced in the code to compute the free-surface elevations with an operating
propeller. This body force-model was run for the Froude number of 0.28 condition. The body force propulsor module in
UNCLE is based on the model of Yang, Hartwich and Sundram (Yang, 1990). The prescribed body forces are based on
the thrust and torque coefficients as well as an assumed circulation distribution. An adequate number of grid points must
be present in the propeller plane to ensure good results. The results are shown in Figure 12. In the region aft of
Table 4—Summary of Measurement Uncertainty for Longitudinal Wave Cuts and Stern Topography at Two Froude Numbers
Bias Error (% of total Precision (Random) Error (% Total Uncertainty (% of largest
uncertainty) of total uncertainty) value)
Fn=0.28 86.0 14.0 2.73
Longitudinal Wave cuts
64.8 35.2 4.60
Stern Topography
Fn=0.41 66.4 33.6 3.54
Longitudinal Wave cuts
32.4 67.6 9.20
Stern Topography
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Figure 12—UNCLE Free-surface Computations at Fn=0.28 Without (Top) and With (Bottom) Propeller Body Force
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ASTERN OF MODEL 5415
the stern there is an increase in the amplitude of the waves, although not over as great an extent as is seen in the
experimental data. The body force-model also predicts an increase in the amplitude of the stern wave crest. The
magnitude of this increase is consistent with that seen in the measurements obtained at a similar Froude number.
CONCLUSIONS
This data provides a comprehensive documentation of the effect of propulsion on the wave system around a naval
combatant hull form. The use of both near- and far-field measurement systems results in a thorough mapping of the wave
field around this hull form. The data presented here shows that there is a greater effect of propulsion on the wave system
near the model at Froude number of 0.28 than at a Froude number of 0.41. It is likely that this is due to the different
nature of the hydrodynamic flow at each of these Froude numbers. At a Froude number of 0.28, the flow is still attached
to the transom and the effect of the operating propellers is to change the character of the local wave system. This change
is manifested as an increase in the maximum wave heights along the stern wave crest line and an increase in the wave
heights behind the model. At a Froude number of 0.41, where the transom is dry, the flow field is dominated by the flow
at the edges of the transom converging astern, and the effects of the operating propulsor are smaller than were observed at
a Froude number of 0.28.
UNCLE computations with propeller body force show similar trends of the effect of propulsion on the wave system
as the experimental data. There is a visible increase in the amplitude of the stern wave crest and an increase in the
amplitudes of the waves in the region astern of the model.
It is hoped that this data will continue to provide an insight into the effect of propulsion on the hydrodynamic flow
around transom stern models, and will be used to evaluate the way in which computational fluid dynamics prediction
codes model propulsors in the computations.
ACKNOWLEDGEMENTS
The author wishes to thank Jim Rice and Ian Mutnick for their support during the collection of these data sets. Scott
Percival and Steve Fisher helped prepare the figures for this paper. Much appreciation goes to William Boston and Peter
Congedo documented the hull form and the hydrodynamic flow, photographically. Finally, I would like to thank Edwin
Rood at the Office of Naval Research for his vision which recognized the contributions that CFD predictions could make
to ship design and his commitment to obtaining the best possible experimental data for validation of these prediction codes.
REFERENCES
AIAA (1998), AIAA Standard S-071–1005, Assessment of Wind Tunnel Data Uncertainty.
ANSI/ASME (1998) Standard PTC 19, Test Uncertainty.
Beddhu, M., Y.Jiang,, D.L.Whitfield, L.K.Taylor, and A.Arabshahi (1998) “CFD Validation of the Free-surface Flow Around DTMB Model 5415
Using Reynolds Averaged Navier-Stokes Equations,” Third Osaka Colloquium on Advanced CFD Applications to Ship Flow and Hull Design,
Osaka, Japan.
Coleman, H. C, and W.G.Steele, (1998) Experimentation and Uncertainty Analysis for Engineers, 2nd Ed.
Hughes, C. and J.F.Allen (1951) “Turbulence Stimulation on Ship Models,” SNAME Transactions, Vol. 59.
Lindenmuth, W., and T.J.Ratcliffe (1989) “Kelvin Wake Measurements Performed on Five Surface Ship Models,” DTRC-89/038.
Ratcliffe, T. (1998) “Validation of Free-Surface Reynold's Averaged Navier Stokes (RANS) and Potential Flow Codes,” 21st Symposium on Naval
Hydrodynamics, Washington, D.C., 1998.
Yang, C-I, P.M.Hartwich, and P.Sundram (1990) “A Navier-Stokes Solution for Hull-Ring Wing-Thruster Interaction,” Eighteenth Naval
Hydrodynamics Symposium, University of Michigan, Ann Arbor, MI.
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ASTERN OF MODEL 5415
DISCUSSION
H.Chun
Pusan National University, Korea.
When you measured the wave profiles, were the models free or fixed? If the models were free, were the sinkages and
trims of the two model conditions with and without the propellers the same as each other? If they are the same, how did
you adjust them?
AUTHOR'S REPLY
Thank you for your important questions regarding the sinkage and trim of Model 5415. For both the longitudinal
wave cut experiments and the stern topography experiments, the model was fixed at a sinkage and trim corresponding to
the trim the model would achieve at a given Froude number. The fixed trim was chosen to be that assumed by the
unpropelled model.. The model was then fixed at this same trim when the propellers were operating. Obtaining data
around the model at the same trim condition, with and without propellers operating provided a self-consistent set of data
for CFD validation.
the authoritative version for attribution.