AerE 344: Undergraduate Aerodynamics and Propulsion Laboratory. Lab Instructions

Similar documents
In this lecture... Subsonic and supersonic nozzles Working of these nozzles Performance parameters for nozzles

Lecture # 12: Shock Waves and De Laval Nozzle

A Propagating Wave Packet Group Velocity Dispersion

Why is a E&M nature of light not sufficient to explain experiments?

Brief Introduction to Statistical Mechanics

orbiting electron turns out to be wrong even though it Unfortunately, the classical visualization of the

4. Money cannot be neutral in the short-run the neutrality of money is exclusively a medium run phenomenon.

Hydrogen Atom and One Electron Ions

Answer Homework 5 PHA5127 Fall 1999 Jeff Stark

Electric (Rocket) Propulsion. EP Overview

5.80 Small-Molecule Spectroscopy and Dynamics

Coupled Pendulums. Two normal modes.

Chemical Physics II. More Stat. Thermo Kinetics Protein Folding...

A General Thermal Equilibrium Discharge Flow Model

COMPUTATIONAL NUCLEAR THERMAL HYDRAULICS

Higher order derivatives

y = 2xe x + x 2 e x at (0, 3). solution: Since y is implicitly related to x we have to use implicit differentiation: 3 6y = 0 y = 1 2 x ln(b) ln(b)

Principles of Humidity Dalton s law

Where k is either given or determined from the data and c is an arbitrary constant.

A Prey-Predator Model with an Alternative Food for the Predator, Harvesting of Both the Species and with A Gestation Period for Interaction

22/ Breakdown of the Born-Oppenheimer approximation. Selection rules for rotational-vibrational transitions. P, R branches.

Exam 1. It is important that you clearly show your work and mark the final answer clearly, closed book, closed notes, no calculator.

Lecture # 12: Shock Waves and De Laval Nozzle

10. The Discrete-Time Fourier Transform (DTFT)

Modeling of the Plasma Flow in High-Power TAL

Engineering 323 Beautiful HW #13 Page 1 of 6 Brown Problem 5-12

Basic Polyhedral theory

Lecture 37 (Schrödinger Equation) Physics Spring 2018 Douglas Fields

Supplementary Materials

Chapter 8: Electron Configurations and Periodicity

MATH 1080 Test 2-SOLUTIONS Spring

ME 300 Exam 1 October 9, :30 p.m. to 7:30 p.m.

University of Illinois at Chicago Department of Physics. Thermodynamics & Statistical Mechanics Qualifying Examination

Finite element discretization of Laplace and Poisson equations

Search sequence databases 3 10/25/2016

Human vision is determined based on information theory:

4 x 4, and. where x is Town Square

ANALYTICAL PARAMETRIC CYCLE ANALYSIS OF CONTINUOUS ROTATING DETONATION EJECTOR-AUGMENTED ROCKET ENGINE HUAN V. CAO

Elements of Statistical Thermodynamics

Differentiation of Exponential Functions

Title: Vibrational structure of electronic transition

Derivation of Eigenvalue Matrix Equations

The van der Waals interaction 1 D. E. Soper 2 University of Oregon 20 April 2012

Davisson Germer experiment

(1) Then we could wave our hands over this and it would become:

Intro to Nuclear and Particle Physics (5110)

Atomic energy levels. Announcements:

ATMO 551a Homework 6 solutions Fall 08

Two Products Manufacturer s Production Decisions with Carbon Constraint

4.2 Design of Sections for Flexure

Collisions between electrons and ions

Image Filtering: Noise Removal, Sharpening, Deblurring. Yao Wang Polytechnic University, Brooklyn, NY11201

INFLUENCE OF GROUND SUBSIDENCE IN THE DAMAGE TO MEXICO CITY S PRIMARY WATER SYSTEM DUE TO THE 1985 EARTHQUAKE

Addition of angular momentum

MA 262, Spring 2018, Final exam Version 01 (Green)

Precise Masses of particles

Rocket Thermodynamics

15. Stress-Strain behavior of soils

REGISTER!!! The Farmer and the Seeds (a parable of scientific reasoning) Class Updates. The Farmer and the Seeds. The Farmer and the Seeds

Difference -Analytical Method of The One-Dimensional Convection-Diffusion Equation

SIMPLE ONE-DIMENSIONAL CALCULATION OF HALL THRUSTER FLOWFIELDS

6.1 Integration by Parts and Present Value. Copyright Cengage Learning. All rights reserved.

u r du = ur+1 r + 1 du = ln u + C u sin u du = cos u + C cos u du = sin u + C sec u tan u du = sec u + C e u du = e u + C

PH300 Modern Physics SP11 Final Essay. Up Next: Periodic Table Molecular Bonding

2008 AP Calculus BC Multiple Choice Exam

ECE507 - Plasma Physics and Applications

Sec 2.3 Modeling with First Order Equations

Note If the candidate believes that e x = 0 solves to x = 0 or gives an extra solution of x = 0, then withhold the final accuracy mark.

MAE4700/5700 Finite Element Analysis for Mechanical and Aerospace Design

1973 AP Calculus AB: Section I

Southern Taiwan University

Exam 2 Thursday (7:30-9pm) It will cover material through HW 7, but no material that was on the 1 st exam.

Classical Magnetic Dipole

Determination of Vibrational and Electronic Parameters From an Electronic Spectrum of I 2 and a Birge-Sponer Plot

General Notes About 2007 AP Physics Scoring Guidelines

Calculus Revision A2 Level

Middle East Technical University Department of Mechanical Engineering ME 413 Introduction to Finite Element Analysis

Quasi-Classical States of the Simple Harmonic Oscillator

Definition1: The ratio of the radiation intensity in a given direction from the antenna to the radiation intensity averaged over all directions.

CE 530 Molecular Simulation

are given in the table below. t (hours)

PHA 5127 Answers Homework 2 Fall 2001

Exergy Analysis of a Combined Power and Ejector Refrigeration Cycle

Electromagnetism Physics 15b

Lecture Outline. Skin Depth Power Flow 8/7/2018. EE 4347 Applied Electromagnetics. Topic 3e

2. Background Material

COHORT MBA. Exponential function. MATH review (part2) by Lucian Mitroiu. The LOG and EXP functions. Properties: e e. lim.

Davisson Germer experiment Announcements:

The Open Economy in the Short Run

u 3 = u 3 (x 1, x 2, x 3 )

Gamma-ray burst spectral evolution in the internal shock model

AS 5850 Finite Element Analysis

MCE503: Modeling and Simulation of Mechatronic Systems Discussion on Bond Graph Sign Conventions for Electrical Systems

P3-4 (a) Note: This problem can have many solutions as data fitting can be done in many ways. Using Arrhenius Equation For Fire flies: T(in K)

First derivative analysis

ANALYSIS OF FLOW IN A DE LAVAL NOZZLE USING COMPUTATIONAL FLUID DYNAMICS

Addition of angular momentum

as a derivative. 7. [3.3] On Earth, you can easily shoot a paper clip straight up into the air with a rubber band. In t sec

Contemporary, atomic, nuclear, and particle physics

Evaluating Reliability Systems by Using Weibull & New Weibull Extension Distributions Mushtak A.K. Shiker

Transcription:

ArE 344: Undrgraduat Arodynamics and ropulsion Laboratory Lab Instructions Lab #08: Visualization of th Shock Wavs in a Suprsonic Jt by using Schlirn tchniqu Instructor: Dr. Hui Hu Dpartmnt of Arospac Enginring Iowa Stat Univrsity Offic: Room 51, How Hall Tl: 515 94 0094 Email: huhui@iastat.du 1

ArE344 Lab09: Visualization of Shock Wavs in a Suprsonic Jt by using Schlirn tchniqu Why look at flow through a nozzl? Th nozzl is on of th most important physical systms on a rockt. Whatvr tchnology drivs th propllant, th nozzl is whr that combustion nrgy is turnd into thrust, and th rockt is ultimatly dpndnt on th nozzl for its prformanc. A givn nozzl will produc th most thrust at a spcific altitud: only whn th xit prssur of th nozzl and th ambint prssur ar matchd dos th nozzl rach its pak prformanc. At this point, calld third critical, flow xits smoothly from th nozzl with no shock wavs. At altituds abov or blow th dsign altitud, shock wavs will dvlop outsid, or insid th nozzl, rspctivly. This would prsnt no difficulty if rockts wr mainly usd at on altitud, but nozzl fficincy will drop off svrly abov or blow th altitud for which it was dsignd. This problm of matching th xit prssur to th ambint prssur is why th ara ratios of th Shuttl Main Engin and th Solid Rockt Boostrs ar so diffrnt. Th SRBs, which run through th lowr portion of th ascnt hav an ara ratio of about 7:1, whil th main ngins, which fir th ntir ascnt, hav a much highr dsign altitud and thus a highr ara ratio of ~77:1. This also th rason for th translatabl skirt som rockts mploy. Ths allow th nozzl to hav mor than on dsign altitud, and thus, travl furthr and fastr with lss propllant. hoto courtsy of NASA GSFC

Quasi 1D Nozzl Rviw Exampl: Want to find,t,m, tc. givn o,, and nozzl shap. Quasi Ara is allowd to vary along x coordinat, but flow variabls ar functions of x only. Start out with govrning consrvation quations: Mass: V ρ dv + ρu nds = 0 t (1.1) S Momntum: t V S S V Enrgy: U U q ρ + dv + ρ + U nds = pu nds + ρ dv + ρ( f U ) dv t t V S S V V (1.3) Assuming: 1. stady. inviscid 3. no body forcs 4. D flow ρudv + ρ( U n ) UdS = pds + ρ fdv + Fviscous (1.) Quasi 1D: Ara is allowd to vary but flow variabls ar a function of x only Mass: A, u, ρ A+dA,u+du, ρ +dρ 3

( )( )( ) 0 ρua + u + du ρ + d ρ A + da = (1.4) ρua + ρua + ρuda + ρdua + d ρua + highr ordr trms = 0 (1.5) Dividd by through ρ ua da du d ρ + + = 0 A u ρ or (1.6) d( ρua) = 0 Momntum: da ρu A + ( ρ + d ρ)( u + du)( u + du)( A + da) = A ( + d)( A + da) + (1.7) ρu A+ ρu A+ ρu da + u Ad ρ + ρuadu + ρuadu = A A da Ad + da (1.8) ( ) uadu Ad u ρuda+ uadρ + ρadu + ρ = (1.9) d = ρudu (1.10) d d d ρ d udu a ρ dρ ρ dρ = = = (1.11) dρ u = du ρ a (1.1) Substituting quation (1.1) into (1.6) to gt: da du u + 0 du = A u a (1.13) which can b rarrangd to gt: da du u da du + 1 = + ( 1 M ) = 0 A u a A u (1.14) da du = ( M 1) A u (1.15) s which can b usd to dtrmin gnral flow bhavior in a convrging divrging nozzl, as blow: 4

M da du < 1 < 0 > 0 da <0 > convrging subsonic < 1 > 0 < 0 da >0 > divrging du <0 > suprsonic> 1 < 0 < 0 dclrating > 1 > 0 > 0 du >0 > acclrating Enrgy: W will not go through th drivation for th nrgy quation but, applying analysis as bfor will giv: dh + udu = 0 or c dt = udu (1.16) Total Static Mach Rlations Isntropic Rlations: ρ T = = ρ T 1 1 1 γ γ (1.17) Static Total From Enrgy Equation with u o =0 (total) c T Rarranging To T γ R using c = 1, γ u1 = c T + (1.18) o 1 u = 1+ (1.19) c T 5

Insrting a To = γ RT and M = uagivs T u = 1+ (1.0) γ RT o T o = + M (1.1) T 1 = 1+ M γ 1 o 1 M γ ρ = 1+ ρ Givn Eq. s (1.1),(1.), and (1.3) w can now: (1.) (1.3) Find any static proprty in an isntropic flow givn Mach #, o,t o, o. Us/control known total conditions to find mach # through nozzl Ara Mach Rlations From mass u at A M = = 1 u = a, giving a ρ ua = ρua (1.4) A ρ a = A ρ u or A ρ ρo a = A ρo ρ u using isntropic rlations for th dnsity trms A 1 = 1+ M A M γ + 1 Mach # is a function of this ara ratio only. Must find A*. γ + 1 (1.5) (1.6) (1.7) 6

Compltly Subsonic Flow = atm (1.8) From isntropic rlation γ o M = 1 (1.9) Can now dtrmin A* and ntir Mach # distribution o If: 1 = Thn: A M = 0,, A = 0 NO FLOW A o A As incrass, M incrass, dcrass, A* incrass A Not that A/A* < 1 is not physically possibl. That is, aftr 1 st critical is rachd, must hav Amin = A* Suprsonic Flow Subsonic Flow ahad of throat. Follow suprsonic A/A* branch aftr throat. A = A t (1.30) A M = f A (1.31) γ 1 γ = o 1+ M (1.3) 7

Suppos w pick o so that = atm If w dcras o, thn < atm bcaus M is unchangd. Nd wak obliqu shocks to gt a small prssur jump. As o dcrass, nd strongr obliqu shocks until normal shock at xit, nd critical. As o dcrass, shock movs up th nozzl. Evntually gt to 1st critical. Incrasing o from 3 rd critical, > atm. Gt randtl Myr xpansion fan to gt prssur dcras Summary: For th nozzl usd in th lab: o,3rd o,nd o,1st 60 psig 0 psig 8psig 8

Visualization of Shock Wavs in a Suprsonic Jt by using Schlirn tchniqu (a). Bfor turning on th Suprsonic jt (b). Aftr turning on th Suprsonic jt Schmatic of th Z typ Schlirn systm usd in th prsnt xprimnt 9

Schlirn imags of th shock wavs in th suprsonic jt flow ArE344 Lab 09: Visualization of Shock Wavs in a Suprsonic Jt by using Schlirn tchniqu Writup Guidlins This is a dmonstration xprimnt. Thr is no lab rport rquird for this lab! 10