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1 National Aeronautics and Space Administration Flow Quality Survey of the NASA Ames 11-by 11-Ft Transonic Wind Tunnel 114 th Meeting of the Supersonic Tunnel Association International Oct 3-7 2010 Japan https://ntrs.nasa.gov/search.jsp?R=20110008498 2018-07-16T08:30:12+00:00Z

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Page 1: Flow Quality Survey of the NASA Ames 11-by 11-Ft … · Flow Quality Survey of the NASA Ames ... Why conduct another Flow Quality Survey? 5 ... •Measure the background noise level

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National Aeronautics and Space Administration

Flow Quality Survey of the NASA Ames

11-by 11-Ft Transonic Wind Tunnel

114th Meeting of the

Supersonic Tunnel Association International

Oct 3-7 2010

Japan

https://ntrs.nasa.gov/search.jsp?R=20110008498 2018-07-16T08:30:12+00:00Z

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National Aeronautics and Space Administration

Ames UPWT became

operational in 1955 and consists

of three test section legs

• 11-By 11-Foot Transonic Leg

(0.2 ! Mach ! 1.5)

•9-By 7-Foot Supersonic Leg

(1.5 ! Mach ! 2.54)

•8-By 7-Foot Supersonic Leg

(2.5 ! Mach ! 3.5)……inactive

Variable pressure (0.2 to 2.2

Atm for the 11-by 11-Ft TWT)

IntroductionFacility Description

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National Aeronautics and Space Administration

• A detailed turbulence and acoustics survey was in the late 1990’s following

the modernization of the 11-ft TWT. This survey was limited to Mach < 1.0.

• Results showed a significant improvement in the turbulence levels and flow

uniformity both attributed to the addition of the turbulence reductions

system.

• Tunnel background noise levels also showed significant improvements

although no specific upgrades were made to address tunnel noise.

• Shortly after the survey, the composite compressor blades were removed

and replaced due to structural failure. They were replaced with the original

aluminum blades.

• A limited amount of data was published immediately following the survey.

Plans were in place to fully document the remaining data but several

factors prevented the plans from being executed.

Background

Post Modernization Survey

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National Aeronautics and Space Administration

• Recent trends in wind tunnel tested have indicated an interest in laminar

flow wing development and design of next generation spacecraft.

• These types of test place a significant importance on knowing the

turbulence and background noise levels of the 11-Ft TWT.

• Customers have expressed an interest in knowing the

- flow quality at supersonic Mach numbers; an area not documented, and

- detailed spectral content (PSD’s) at all Mach numbers; important for

separating model generated noise from tunnel background noise.

• Questions have arisen regarding the acoustics levels reported by the

facility based on P’ measurements made on customer models.

• Data from the post-modernization survey are no longer available.

• More recently, the turning vane set downstream of the test section (TV1)

was replaced due to stress cracks in the structure.

Why conduct another Flow Quality Survey?

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National Aeronautics and Space Administration

New Flow Quality Survey

In 2008, funding became available to conduct a new turbulence and

acoustics survey.

Objectives

• Measure free-stream turbulence and acoustics levels in the 11-ft TWT

- Perform a baseline survey from Mach 0.4 to 1.35 at Pt = 2200 psf.

- Measure at different tunnel total pressure.

- Evaluate off centerline levels.

• Measure the background noise level with a fairing attached to the strut

trailing edge.

- Assess the fairings’ effect on the spectra.

- Calculate the reduction in acoustics and turbulence.

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National Aeronautics and Space Administration

Flow Quality Test Plan

• Phase 1: Repeat 1999 Baseline measurements

- Unreliable Constant Temperature Anemometer (CTA) cast doubt on

the quality of the measurements.

- P’ measurements were higher but transducer referencing strategy was

in doubt.

• Phase 2: Acoustic survey to establish new Baseline

- Mach 0.4 to 1.35 using two rakes

- Evaluate different probes and referencing methodologies

- Analysis showed previous content thought to be associated with the

drive tone may actually be from the sting model support strut.

• Phase 3: Turbulence Survey with new CTA

- Mach 0.4 to 0.95.

- Measure the background noise level with a fairing attached to the strut

trailing edge.

- Assess the fairings’ effect on the spectra.

• Phase 4: Supersonic Turbulence Survey

- Mach 1.05 to 1.5

- 10º Laminar Flow Cone

- Free-stream turbulence levels in the 11-ft TWT (establish baseline)

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National Aeronautics and Space Administration

Test Section Instrumentation

•Turbulence, !u': single hot wires

• Fluctuating Static Pressures, p': 10° cone probes

• Total Temperature, Tt: RTD probes

Sensors located at TS 185

Ku02(2000)

Ku01(1995) T11-0196

8-Ft Span Rake (Mach < 0.95) 1-Ft Span Mini-Rake (Mach > 1.0)

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National Aeronautics and Space Administration

Data Acquisition and Reduction

Data acquired using both a steady state and dynamic system:

Tunnel Condition, rake position

• Standard Data System (SDS)

• Sample period: 1 sec

Hot Wire and P’ transducers

• HP® DAC Express

• Sample rate: 256000 samples/sec

• Sample period: 30 sec

• Signal AC coupled at 0.1 Hz

Data processed with custom software

Processing parameters• Bandwidth: 1 Hz to 10 kHz

• Window: Hanning

• PSD resolution: 1Hz

• Overlap: 50%

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National Aeronautics and Space Administration

Baseline TurbulencePt=2200 psf, z=0 in.

• % Turbulence (!u’/!U)is the metric used tocompare overallturbulence levels.

• Each symbolrepresents the averageof 5 data points.

• Centerline probe dataagree.

• Elevated level at y=36in a result of proximityto the walls.

Preliminary Data

0.00

0.10

0.20

0.30

0.40

0.50

0.60

0.70

0.80

0.90

1.00

0.30 0.40 0.50 0.60 0.70 0.80 0.90 1.00

Mach

Tu

rb,

[%]

y=-6 in.

y=0 in.

y=12 in.

y=36 in.

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National Aeronautics and Space Administration

Structure of TurbulencePt=2200 psf, z=0 in.

Processing: Bandwidth: 1 Hz to 10 kHz

Window: Hanning

PSD Resolution: 1 Hz

Overlap: 50%

Acquisition: Duration: 30 sec

Sample rate: 25.6 ksamples/s

AC coupled, 0.1 Hz

The Power Spectral Density

(PSD) plot offers a detailed

look into the components that

make up the total turbulence.

Major sources of flow

perturbation contributing to

turbulence (and noise)

1. SMSS Strut: 200-400 Hz

2. Compressor: 180-650 Hz

3. TS Wall Slots: 2.5-3 kHz1.E-13

1.E-12

1.E-11

1.E-10

1.E-09

1.E-08

1.E-07

1.E-06

1.E-05

1.E-04

1 10 100 1000 10000

Frequency, (Hz)

Am

pli

tud

e,

(V^

2/H

z)

M=0.4, Pt=2200 psfM=0.8, Pt=2200 psf

Series4Series6Preliminary Data

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National Aeronautics and Space Administration

Sting Model Support Strut Noise Reduction

Long Fairing

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National Aeronautics and Space Administration

Potential for Acoustic Reduction

• Cp’ is the metric used to

compare overall noise

levels.

• Each symbol represents

the average of 5 data

points.

• Fairing reduced the Cp’

by as much as 10%0

0.005

0.01

0.015

0.02

0.025

0.00 0.20 0.40 0.60 0.80 1.00

Mach

Cp

'

Baseline + Repeats

Ful l -Fa i r ing

Prel iminary Data

Pt = 2200 psf

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National Aeronautics and Space Administration

Potential for Acoustic Reduction - PSD

• Acoustics PSD is similar

in structure to the one for

turbulence.

• The lower Cp’ associated

with the fairing is a result

of the strut tone

suppression at 400 Hz.

• Turbulence levels also

decrease as a result of

this noise reduction.

1E-01

1E+00

1E+01

1E+02

1E+03

1E+04

1 10 100 1000 10000

Frequency, (Hz)

Am

pli

tud

e,

(ps

i^2

/Hz)

BaselineFull FairingMach=0.8, Pt=2200 psf

Preliminary Data

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National Aeronautics and Space Administration

Summary

• New baseline turbulence levels have been measured using a

new CTA and new hot-wire sensors.

-Levels remain the same as measured in 1999.

-Data and methodology documented (almost)

• New baseline acoustics levels have been measured up to

Mach 1.35

-Levels are higher than reported in 1999.

-Data and methodology documented (almost)

• Application of fairings to the strut trailing edge showed up to a

10% reduction in the tunnel background noise.

• Data analysis and documentation for publishing is ongoing.

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National Aeronautics and Space Administration

Future

• Perform the Supersonic turbulence survey to establish a baseline

- Manufacture a new 4-Ft Span Rake to hold more sensors

- Extend transonic measurement methodology to supersonic flow

- Design new acoustics probes

• Explore methods to reduce noise generated by slot tones and drive

tones.

• Collaboration with customers to determine application to testing

requirements.