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GSFC· 2015 Focused Schlieren Imaging for Supersonic Film Cooling Chandan Kittur, Colin Adamson, Jung Lee, Salman Verma, Christopher Cadou, Arnaud Trouve University of Maryland Joseph Ruf NASA Marshall Space Flight Center
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Page 1: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

GSFC· 2015

Focused Schlieren

Imaging for Supersonic

Film Cooling

Chandan Kittur, Colin Adamson, Jung

Lee, Salman Verma, Christopher

Cadou, Arnaud Trouve

University of Maryland

Joseph Ruf

NASA Marshall Space Flight Center

Page 2: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Outline

• Background

• Objectives and Methodology

• Results and Conclusions

2TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Page 3: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Introduction to Film Cooling

What is Film Cooling?

Technique where a cooler gas is injected

along critical surfaces, creating an

insulating layer that protects the walls from

hot combustion exhaust.

Applications

• Gas Turbines

Combustor liner

Turbine blades

• Rockets

Nozzle extension

Gas turbine combustor

Rocket thrust chamber

Adapted from

(Sutton, 1986)J-2X Concept

Hot

Cold

Film Cooled Wall

Mainstream

Coolant

Figure Adapted from

Cruz (2008)

Page 4: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

J-2x Nozzle film Cooling

4TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

• J-2X nozzle extension

• UMD tunnel

– J-2X analogue

– Various film flow cases:

• Case 0 – no film

• Case 1 – Mfilm = 0.5

• Case 2 – Mfilm = 0.7

• Case 3 – Mfilm = 1.2

M2= 1.84,

T2 = 539 K,

P02 = 2.4 atm

M1= 3.74,

T1 = 3767 K,

P01= 82 atm

x

y

𝑑𝑃

𝑑𝑥= 0

Core Inlet:

T0= 300 K

P0= 1 atm

Twall=340 K

Twall=340 KFilm Inlet:

T0= 330 K

Mcore = 2.4

Page 5: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Physics of Film Cooling

Parameters characterizing the mixing of the film

Blowing ratio, BR = (U)s / (U)∞

Velocity ratio, VR = Us / U∞

Slot Reynolds number, Res=(Us s)/

Inlet turbulence intensity, Iu = Urms/U, Iv = Vrms/U

Important Flow Features

• Large Shear

• Wall-bounded flow

• Initial turbulence

• Intense mixing and heat

transfer

• Low pressure region

behind louver lip

Film Cooling effectiveness

c

awaw

TT

TT

y1

y2

2

1

y

x

Zone II

(coolant zone)

b(x)

Zone I

(mixing zone)

X=

0

X=X

1

Coolant Stream

Hot Gas Stream

Initial region Developed region

vU ,T ,I ,

s s v,sU ,T ,IS

Taw(x)

Wall Wake (WW) – VR < 1

Minimum Shear (MS) – VR

~ 1

Wall Jet (WJ) – VR > 1

Figure Adapted from

Dellimore (2010)

Page 6: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Regular vs Focused Schlieren Schematic

Regular

Focused

Page 7: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Depth of Focus

Regular Focused

The resulting image will be the average of all planes within depth of

focus. Will only be able to see turbulent structures with focused

schlieren

Page 8: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Field of View

• Focused Schlieren has a much smaller Field of view

8TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Imaging region

Film Flow

Core

Flow

Imaging region

Film Flow

Core

Flow

Regular

Focused

Page 9: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Previous Work

• VanDercreek1

was able to visualize a turbulent

boundary layer on a sharp nosed cone in a hypersonic

wind Tunnel

• Lawson 2 was able to measure velocity of supersonic

turbulent boundary layer using focusing-schlieren PIV

with a pulsed LED

9TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Page 10: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Outline

• Background

• Objectives and Methodology

• Results and Conclusions

10TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Page 11: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Objectives

• A non-Intrusive method to resolve velocity field and flow

structures

– Use regular schlieren to visualize shocks and expansions

– Used focused schlieren to visualize turbulent structures in the

boundary layer

– Use a pulsed LED for focused schlieren PIV

• Freeze flow to move only 0.1 mm

• Compare experimental velocity and flow structures to

CFD for validation

11TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Page 12: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

UMD Supersonic Wind Tunnel

12TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

• Basic Specs

– Transient facility (6-10 sec run time)

– Working fluid: Air

– Total P, T: Ambient

– Test section Dimension: 12”x6”x26”

• The tunnel cannot directly match J-2X conditions so special care must be

taken to design analogous experiments.

– Heat walls to ensure that the heat flux vector always points into the flow

– Heat film to ensure temperature “cascade” is preserved

Page 13: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Schlieren System

13TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

• Z configuration

• Nikon D-90 with Nikon 70-300mm f/4-5.6G lens

Top down view of tunnelMain Flow

Louver

Mirror 1

Mirror 2

Horizontal Schlieren Stop

Camera

Aperture

LED

f = 59.75 in

f = 78.625 in

Page 14: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Focused Schlieren Lengths

• Everything was kept symmetric

– L=l’ =1219 mm

– l =L’ = 240 mm. Determined by focal length of schlieren Lens

14TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Page 15: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Cut-off grid Calculations

𝜖𝑚𝑖𝑛 = 20626 ∗𝑏

2∗

𝐿

𝐿′ ∗ 𝐿 − 𝑙= 10 𝑎𝑟𝑐𝑠𝑒𝑐𝑜𝑛𝑑𝑠

𝐷𝑠 =4 ∗ 𝑙2 ∗ 𝑙′ − 𝐿′ ∗ 𝜆

𝐴𝑠 ∗ 𝑏 ∗ 𝑙′= 1 𝑚𝑚

15TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Cut-Off grid

𝝀 = wavelength of light =

𝟓𝟐𝟏 ∗ 𝟏𝟎−𝟔 𝒎𝒎As = Schlieren lens diameter

= 100 mm

𝒃 = 𝒄𝒖𝒕𝒐𝒇𝒇 𝒈𝒓𝒊𝒅 𝒘𝒊𝒅𝒕𝒉 =𝟏𝒎𝒎

Page 16: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Generating Source Grid

• System is symmetric. So able to

run system in reverse in order to

determine size of source grid

• Both cut-off and source grid

printed on transparency paper

Page 17: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Focused Schlieren System

Fresnel Lens and

Source Grid

Schlieren Lens and

cut-off grid

17TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Page 18: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Expected Focused Schlieren Images

18TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Can view Density Gradients :

𝛻𝜌 > 0.88𝑘𝑔

𝑚4

𝒌 = 𝑮𝒍𝒂𝒅𝒔𝒕𝒐𝒏𝒆 − 𝑫𝒂𝒍𝒆 𝒄𝒐𝒆𝒇𝒇𝒊𝒄𝒊𝒆𝒏𝒕 = 𝟎. 𝟐𝟑𝒄𝒎𝟑

𝒈𝒏𝟎 = 𝟏. 𝟎𝟎𝟎𝟐𝟗𝟐 𝒇𝒐𝒓 𝒂𝒊𝒓

𝝐𝒚 =𝒌 ∗ 𝑳

𝒏𝟎

𝝏𝝆

𝝏𝒚;

Page 19: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Pulsed Light Source

19TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

• Based on a high intensity LED with an advertised response

time < 25 ns

• Based on Wilert’s design 3 which used a pulse width of 5𝜇𝑠

• Circuit triggered using a square wave generated by an

Arduino

– Arduino provides inexpensive triggering flexibility

Page 20: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Outline

• Background

• Objectives and Methodology

• Results and Conclusion

20TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Page 21: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Flow Structure: Case 0 (Mfilm = 0)

21TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Film Louver

Flow

Page 22: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Flow Structure: Case 1 (Mfilm = 0.5)

22TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Mfilm< 1

Mcore> 1

Shear layer

Louver Slip line

Boundary layers

Wall

Shock

Exp

Film Louver

Flow

Page 23: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Flow Structure: Case 2 (Mfilm = 0.7)

23TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Mfilm< 1

Mcore> 1

Shear layer

Louver Slip line

Boundary layers

Wall

Shock

Exp

Film Louver

Flow

Page 24: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Flow Structure: Case 3 (Mfilm = 1.2)

24TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Mfilm > 1

Mcore > 1

Louver Slip line

Boundary layers

Shock

Reflected Shock

Shear layer

Shock

Wall

Exp

Film Louver

Flow

Page 25: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

• Schlieren Image of full test section: No Film

25TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

• Shear layer appears completely mixed out after x/s = 8

• Lip shock reflects off upper wall at x/s = 22.5

• Numerous blotches are window scratches

Page 26: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Automated Angle Detection

• Able to detect lines in an image using the Hough

transform matlab functions

26TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Case 0 (Mfilm = 0)

Page 27: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Comparison to CFD

TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD 27

• Schlieren and CFD are qualitatively similar

– Both show lip and reattachment shocks

– Evidence of recirculation region

• Shock angles consistent within 5%

– Lip shock 𝜃 = 30°

– Reattachment shock 𝜃 = 21°

Page 28: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Depth of Focus

28TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

In focus10 mm

out of focus

• Target is an 8-32 bolt

• Depth of Sharp focus is on the order of 10 mm

• Much smaller than tunnel width (152 mm)

• Insufficient to resolve small scale structures

• But much better than regular schlieren

Page 29: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Focused Schlieren Sensitivity

29TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

• Focused schlieren video

of butane gas stream in

the test section

No Film Case Focused Schlieren

Minimum verifiable density gradient

~ 𝟐𝟔𝒌𝒈

𝒎𝟒

Page 30: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Power/Pulse Width Tradeoff

30TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

• The 70 𝝁𝒔 pulse provided enough power to illuminate the

test section

Regular

Schlieren

Intensity

Page 31: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Amplifier Transistor

- Yellow is the output of the amplifier (the gate input of

the transistor) and green is the output of the transistor

- 1μs scale on left and 4μs scale on right

- Delayed response of transistor seems to be related to

delayed rise to peak voltage in the amplifier (amplifier

might need to be replaced)

Page 32: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Pulsed Light Source

• Pulse width needs to be dropped 3 orders of magnitude

for PIV

Page 33: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Conclusions

• Status of current system :

– Insufficient sensitivity to resolve turbulent density fluctuations

– Insufficient depth of sharp focus to resolve turbulent structures

– Insufficient temporal response to freeze flow

33TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Expected Actual Required

Sensitivity:

Density

Gradient (𝑘𝑔

𝑚4)

0.88 26 5

Depth of

Sharp Focus

(mm)

1 10 1

LED Pulse

Width (𝜇𝑠)5 70 0.1

Page 34: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Next Steps

• Regular Schlieren

– Obtain more downstream images

• Main problem with focused schlieren system is rigidity

– Focused schlieren very difficult to align precisely

– Will provide better frame for Fresnel lens and source grid

• LED power supply

– Some components don’t seem to behave as advertised

– Will test with new components

– Looking into alternative circuits

34TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Page 35: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

Acknowledgements

• The authors would like to thank the National Aeronautics

and Space Administration and Melinda Nettles of the

Marshall Space Flight Center for their support under

NRA NNM13AA13G.

35TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD

Page 36: Focused Schlieren Imaging for Supersonic Film CoolingAIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition (2009). 3. Willert, C., B. Stasicki,

References

1. Vandercreek, Colin, Michael Smith, and Kenneth Yu. "Focused

Schlieren and Deflectometry at AEDC Hypervelocity Wind Tunnel

No. 9." 27th AIAA Aerodynamic Measurement Technology and

Ground Testing Conference (2010):.

2. Lawson, Michael, Michael Hargather, Gary Settles, Leonard

Weinstein, and Sivaram Gogineni. "Focusing-Schlieren PIV

Measurements of a Supersonic Turbulent Boundary Layers." 47th

AIAA Aerospace Sciences Meeting including The New Horizons

Forum and Aerospace Exposition (2009).

3. Willert, C., B. Stasicki, J. Klinner, and S. Moessner. "Pulsed

Operation of High-power Light Emitting Diodes for Imaging Flow

Velocimetry."Measurement Science and Technology Meas. Sci.

Technol. 21.7 (2010): 075402.

36TFAWS 2015 – August 3-7, 2015 – Silver Spring, MD


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