Upload
vincent-nicholson
View
215
Download
0
Tags:
Embed Size (px)
Citation preview
1The University of Manchester Aero-Physics Laboratory
Compressible Vortex Rings in a Shock Tube with Helium Driver
R. Mariani
Prof. K. Kontis
2The University of Manchester Aero-Physics Laboratory
Table of Contents
Project background Experimental facility Results and discussions Conclusions
Project Background
Aim: to evaluate the characteristics of compressible vortex loops where the physical properties of the driver and driven gas differ
Variation of the theoretical Mach number while keeping max pressure ratio constant
Real life applications where gas properties are not constant
3The University of Manchester Aero-Physics Laboratory
Experimental Facility
Open end shock tube:Driver gas: grade A heliumDriven gas: air at ambient conditions
Pressure ratios: 4/8/12Constant cross-section
Fixed driven lengthVariable driver length
Schlieren set up:Shimadzu HPV-1 high-speed cameraContinuous xenon light
Particle image velocimetry:TSI high-speed stereo PIV
4The University of Manchester Aero-Physics Laboratory
Results and DiscussionEffects on Shock Strength Non-homogeneous gases in the shock tube:
Mixture of gases affect propagation velocity or flow structure only negligibly(C.G. Miller)
A light driver gas increases shock wave strength for a given pressure ratio:Higher Mach number compared to air/air gas
combination
5The University of Manchester Aero-Physics Laboratory
P4/P1 Ms Mse
4 1.53 1.43
8 1.89 1.81
12 2.12 2.10
Results and DiscussionEffects on Vortex Ring Structure Pressure ratio ~4
Oblique shock system in the trailing jet
Embedded rearward facing shock
Presence of weak secondary vortex ringsCounter-rotatingWeaker compared to
main ringFormation threshold
possibly lowered by non-homogeneous gas physical properties
6The University of Manchester Aero-Physics Laboratory
Flow structure (above) and secondary VR (below)
Results and DiscussionEffects on Vortex Ring Structure Pressure ratio ~8
Shape of jet becomes curvilinear
Oblique shock system transitions into a MR with a large Mach diskFormation of a central
jetFormation of
secondary vortex rings ahead of main vortex ring
7The University of Manchester Aero-Physics Laboratory
Flow structure of the vortex ring at P4/P1 ~ 8
Results and DiscussionEffects on Vortex Ring Structure Pressure ratio ~12
Mach disk increases in size allowing a large central jet to be formedExpanding central
jet
Embedded rearward facing shock becomes straight
8The University of Manchester Aero-Physics Laboratory
Flow structure of the vortex ring at P4/P1 ~ 8
Results and DiscussionEffects on Vortex Ring Structure
Pressure ratio ~8Secondary vortex
rings formation
9The University of Manchester Aero-Physics Laboratory
Results and DiscussionEffects on Vortex Ring Structure
Pressure ratio ~12Mach disk formation:
Formation of a lower velocity central jet
10The University of Manchester Aero-Physics Laboratory
Results and DiscussionEffects on Vortex Ring Structure
Pressure ratio ~12Mach disk increases in size allowing a large central jet to
be formedExpanding central jetShear layer opposite to main ring circulation. Consistent with
secondary vortex ring circulation
11The University of Manchester Aero-Physics Laboratory
Conclusions
Lighter driver gas leads to an increase in Mach number for a given pressure ratio
Presence of secondary vortex rings below the expected thresholdCould be caused by the non-homogeneous physical gas
properties. Oblique shock system transitions from RR to MR
Formation of a lower velocity central jetFormation of a central shear layer of opposite direction
with main vortex ring. Consistent with circulation of secondary vortex ring
12The University of Manchester Aero-Physics Laboratory