Shell/Integral Balances (SIB)

Similar documents
3.8 The First Law of Thermodynamics and the Energy Equation

Objectives. Conservation of mass principle: Mass Equation The Bernoulli equation Conservation of energy principle: Energy equation

vector H. If O is the point about which moments are desired, the angular moment about O is given:

Analyzing Mass and Heat Transfer Equipment

Where does Bernoulli's Equation come from?

where = rate of change of total energy of the system, = rate of heat added to the system, = rate of work done by the system

MOMENTUM PRINCIPLE. Review: Last time, we derived the Reynolds Transport Theorem: Chapter 6. where B is any extensive property (proportional to mass),

150A Review Session 2/13/2014 Fluid Statics. Pressure acts in all directions, normal to the surrounding surfaces

Angular momentum equation

Chapter Four fluid flow mass, energy, Bernoulli and momentum

COURSE NUMBER: ME 321 Fluid Mechanics I 3 credit hour. Basic Equations in fluid Dynamics

Heat and Mass Transfer Prof. S.P. Sukhatme Department of Mechanical Engineering Indian Institute of Technology, Bombay

Principles of Convection

MAE 224 Notes #4a Elements of Thermodynamics and Fluid Mechanics

Shell Balances in Fluid Mechanics

Conservation of Momentum using Control Volumes

Friction Factors and Drag Coefficients

Basic Fluid Mechanics

FE Exam Fluids Review October 23, Important Concepts

M E 320 Professor John M. Cimbala Lecture 10. The Reynolds Transport Theorem (RTT) (Section 4-6)

MAE 3130: Fluid Mechanics Lecture 7: Differential Analysis/Part 1 Spring Dr. Jason Roney Mechanical and Aerospace Engineering

Chapter 6: Momentum Analysis

FLUID MECHANICS PROF. DR. METİN GÜNER COMPILER

CHAPTER 7 SEVERAL FORMS OF THE EQUATIONS OF MOTION

Differential relations for fluid flow

FLOW IN PIPES. Mark J McCready University of Notre Dame July 24, chemeprof.com

Interpreting Differential Equations of Transport Phenomena

Page 1. Neatly print your name: Signature: (Note that unsigned exams will be given a score of zero.)

For example an empty bucket weighs 2.0kg. After 7 seconds of collecting water the bucket weighs 8.0kg, then:

Elementary Non-Steady Phenomena

Overall Heat Transfer Coefficient

M E 320 Professor John M. Cimbala Lecture 10

Advanced Hydraulics Prof. Dr. Suresh A. Kartha Department of Civil Engineering Indian Institute of Technology, Guwahati

Introduction to Heat and Mass Transfer. Week 10

FE Fluids Review March 23, 2012 Steve Burian (Civil & Environmental Engineering)

Chapter 6: Incompressible Inviscid Flow

MASS, MOMENTUM, AND ENERGY EQUATIONS


Basic Fluid Mechanics

Advanced Chemical Reaction Engineering Prof. H. S. Shankar Department of Chemical Engineering IIT Bombay. Lecture - 03 Design Equations-1

12/21/2014 7:39 PM. Chapter 2. Energy and the 1st Law of Thermodynamics. Dr. Mohammad Suliman Abuhaiba, PE

FLUID MECHANICS. Chapter 9 Flow over Immersed Bodies

Fluid Mechanics Prof. S. K. Som Department of Mechanical Engineering Indian Institute of Technology, Kharagpur

Department of Mechanical Engineering

Module 2 : Convection. Lecture 12 : Derivation of conservation of energy

Convection. forced convection when the flow is caused by external means, such as by a fan, a pump, or atmospheric winds.

10.52 Mechanics of Fluids Spring 2006 Problem Set 3

Section 2: Lecture 1 Integral Form of the Conservation Equations for Compressible Flow

Chapter 6: Momentum Analysis of Flow Systems

V (r,t) = i ˆ u( x, y,z,t) + ˆ j v( x, y,z,t) + k ˆ w( x, y, z,t)

Empirical Co - Relations approach for solving problems of convection 10:06:43

CEE 3310 Control Volume Analysis, Oct. 7, D Steady State Head Form of the Energy Equation P. P 2g + z h f + h p h s.

ME 144: Heat Transfer Introduction to Convection. J. M. Meyers

Mechanical Engineering Science for Medical Engineers Level: 4 Credit value: 8 GLH: 62 TQT: 80

PHYSICAL MECHANISM OF CONVECTION

Chemical and Biomolecular Engineering 150A Transport Processes Spring Semester 2017

UNIT II CONVECTION HEAT TRANSFER

Lecture-4. Flow Past Immersed Bodies

Part A: 1 pts each, 10 pts total, no partial credit.

CHAPTER 4 BOUNDARY LAYER FLOW APPLICATION TO EXTERNAL FLOW

Fluid Mechanics. du dy

Lesson 6 Review of fundamentals: Fluid flow

7 The Navier-Stokes Equations

Chapter 3 NATURAL CONVECTION

4.1 LAWS OF MECHANICS - Review

CEE 3310 Control Volume Analysis, Oct. 10, = dt. sys

CHAPTER 3 BASIC EQUATIONS IN FLUID MECHANICS NOOR ALIZA AHMAD

CHAPTER 8 ENTROPY GENERATION AND TRANSPORT

High Speed Aerodynamics. Copyright 2009 Narayanan Komerath

HOW TO GET A GOOD GRADE ON THE MME 2273B FLUID MECHANICS 1 EXAM. Common mistakes made on the final exam and how to avoid them

Physics 3 Summer 1990 Lab 7 - Hydrodynamics

Fundamentals of Fluid Dynamics: Elementary Viscous Flow

CONVECTIVE HEAT TRANSFER

CONVECTIVE HEAT TRANSFER

Chapter 14. Fluid Mechanics

ROAD MAP... D-0: Reynolds Transport Theorem D-1: Conservation of Mass D-2: Conservation of Momentum D-3: Conservation of Energy

PEMP ACD2505. M.S. Ramaiah School of Advanced Studies, Bengaluru

Detailed Outline, M E 320 Fluid Flow, Spring Semester 2015

(Refer Slide Time 1:25)

PROBLEM SET 6. SOLUTIONS April 1, 2004

PROBLEM SET 3 - SOLUTIONS

Introduction to Transport Processes

Nicholas J. Giordano. Chapter 10 Fluids

Chapter 14. Lecture 1 Fluid Mechanics. Dr. Armen Kocharian

Lecture 2 Flow classifications and continuity

Unit B-1: List of Subjects

ME3560 Tentative Schedule Spring 2019

Fundamentals of compressible and viscous flow analysis - Part II

6.041SC Probabilistic Systems Analysis and Applied Probability, Fall 2013 Transcript Tutorial:A Random Number of Coin Flips

APPH 4200 Physics of Fluids. Introduction Lecture 1

CLASS Fourth Units (Second part)

BERNOULLI EQUATION. The motion of a fluid is usually extremely complex.

AA210A Fundamentals of Compressible Flow. Chapter 5 -The conservation equations

meters, we can re-arrange this expression to give

INSTRUCTOR: PM DR MAZLAN ABDUL WAHID

ME3560 Tentative Schedule Fall 2018

Applied Thermodynamics for Marine Systems Prof. P. K. Das Department of Mechanical Engineering Indian Institute of Technology, Kharagpur

Vectors Part 1: Two Dimensions

E80. Fluid Measurement The Wind Tunnel Lab. Experimental Engineering.

Thermal Systems. What and How? Physical Mechanisms and Rate Equations Conservation of Energy Requirement Control Volume Surface Energy Balance

Transcription:

Shell/Integral Balances (SIB) Shell/Integral Balances Shell or integral (macroscopic) balances are often relatively simple to solve, both conceptually and mechanically, as only limited data is necessary. At the same time, many problems require only the level of detail that may be extracted from these types of balances and thus they represent powerful tools. Perform control volume (or macroscopic) balances # Derive and use a macroscopic mass balance (continuity equation) [4.1, 4.2] [notes] # Derive and use a macroscopic momentum balance [5.1, 5.2] [notes] # Derive and use a macroscopic energy balance [6.1, 6.2] [notes] Use the General Mechanical Energy Balance Equation to perform calculations on simple pipe networks and/or process problems [6.3] # Explain the connection between a macroscopic energy balance and Bernoulli's Equation # Use Bernoulli's Equation to calculate velocities, pressures, or height changes in flowing fluid systems [notes] # Extend the Bernoulli's Equation for more general cases (i.e., write and use the mechanical form of the macroscopic energy balance equation) [notes] Solve heat transfer problems on macroscopic bodies [p241-243] # Determine the efficiency of a fin [notes] # Calculate the heat flow through a fin from the fin's efficiency [notes]

SIB: Mass Balance For our balance, we will choose an arbitrary fixed (in space) control volume. Thus, it is an open system (i.e., one through which mass may flow). Because of this, the total material within our control volume can change with time as stuff flows in and out. A "word equation" for this process may be written as: rate of change of mass in CV = net rate of mass flow into CV We note that the amount of mass contained in a small section of volume, dv, can be written as dv. In order to calculate all of the material in our control volume we simply add all of the contributions from each section dv (i.e., we integrate), so that the rate of change of mass in the CV is: The easiest way to capture the amount of material flowing into/out of the CV is to watch the stuff that crosses the boundaries. That is, if we look at the velocity of the mass and see what portion of that velocity is perpendicular to the surface, we can then add up all the contributions of stuff crossing the surfaces, so that our final equation can be written as: Functionally, what this equation means is that, in order to perform a macroscopic mass balance, we simply look at the inlets and outlets of a process and multiply the (area) average velocity times the density and the cross-sectional area of that orifice. OUTCOME: Derive and use a macroscopic mass balance (continuity equation)

SIB: Conservation of Momentum: Basic System Statement If we now choose an arbitrary system of material (for a Lagrangian outlook on the problem): we can write a "word equation" for the changes in momentum of this system as: Writing this mathematically we get: where denotes the sum of the forces acting on the fluid element within our system. In order to mathematically translate between a control system and a control volume one uses the Reynolds Transport Theorem that stipulates that: so that our momentum balance equation can be written as: It was easier to rationale the balance of momentum using a system -- since we are all familiar with the equation. It might have also helped when we did a material balance, as a material balance on a system would simply have been

Recalling from earlier in the course, we know that the potential forces that act on fluids are the following: Pressure force at inlets and outlets (a surface force): Pressure and shear force exerted by wall surfaces on fluid in CV (surface forces): Gravitational force exerted on all fluid within CV (a body or volumetric force): Combining these we can write a general form of the momentum balance equation as: Recall that the shear stresses affect only the walls of the CV; the pressure affects all surfaces (including inlets and outlets); and the gravitational forces affect the entire CV. IMPORTANT: This is a vector equation so that, in practice, there will be three momentum balances equations to write; one in each of the coordinate directions! OUTCOME: Derive and use a macroscopic momentum balance.

SIB: Energy Balance For our balance, we will choose an arbitrary fixed (in space) control volume. Thus, it is an open system (i.e., one through which mass may flow). Accounting for energy within that volume (and transfer with surroundings) we get: rate of accumulation of energy in CV = net rate of energy transport into CV (by flow) + net rate of energy transferred to material in CV We denote e as the total energy per unit mass, and note that energy can be transferred to the material in the CV through both heat (thermal energy) flow and work. Therefore, we can write this in equation form as: NOTATION: - e, the total energy per unit mass, is comprised of mechanical (kinetic and potential) as well as internal (thermal) energy - q represents the heat that is transferred to the material within the volume - W represents any work done on or by the system (the chosen sign convention is that work done on the system is positive). We note that the energy per unit mass may have an internal energy component as well as a kinetic and potential energy component, so that we can write it as: We further note that the work can have several components: where W s is the shaft work and the other two components ( and ) correspond to stresses at the boundaries (both normal and shear). If we extract the pressure from the normal stresses we can write our work in the form: where the pressure stresses now make up what is typically called the "flow work" term, and remaining viscous stresses are lumped into the term, which is only non-zero if we have a non-zero shearing velocity on the control surfaces. Combining these observations into a final form of the macroscopic energy balance equation, we get

OUTCOME: Derive and use a macroscopic energy balance

SIB: Bernoulli Equation A very special form of the energy balance equation will arise under certain limiting assumptions. DEFINITIONS: The Bernoulli equation is obtained from the energy balance equation when we have a steady, incompressible, and inviscid flow in which there is no shaft work, no heat transfer, and no change in internal energy occurs. DEFINITIONS: An inviscid flow is one in which viscous losses are negligible (i.e., the fluid viscosity is very small). Let's look at each of these limitations in turn: Steady Flow: the left-hand side becomes zero as the d/dt term vanishes Incompressible Fluid: the density remains constant everywhere Inviscid Flow: there are no viscous work losses ( ) and the flow is everywhere a "plug flow" (i.e., velocities are constant perpendicular to the main flow -- this also means that the shear stresses are zero!) No Heat Transfer (adiabatic): q=0 No Change in Internal Energy: drops out of the equation Under these simplifications our macroscopic energy balance becomes: Because of our constant velocities and constant densities, we can simplify this further to be The Bernoulli Equation (sometimes called Bernoulli's Law) is typically used because it is true along a streamline (i.e., for a CV that encircles a single streamline), although it will clearly also work for more complex CVs that satisfy the above criteria. OUTCOME: Explain the connection between a macroscopic energy balance and Bernoulli's Equation

SIB: Mechanical Energy Balance Equation Perhaps the most common way to write the Bernoulli equation is:. If you allow for frictional losses in the Bernoulli equation, then this equation becomes: When you include frictional losses it is no longer correct to assume that you have a plug flow, so you need to use the average value of the term at each point. where represents the frictional losses in the system. Recall that we learned to calculate the calues earlier in the term. One last tweak to the Mechanical Energy Balance equation is to note the following: To allow the simplified statement above to be most conveniently used, one will often define a value as so that you may write: OUTCOME: Extend the Bernoulli's Equation for more general cases (i.e., write and use the mechanical form of the macroscopic energy balance equation)

SIB: Fins A few lectures ago we looked at how for the case of a cylinder we could, in fact, increase the rate of heat transfer by adding insulation (i.e., making the diameter larger). Upon reflection, we realized that this happens because by adding the insulation (or making the diameter larger) we increased the area available for convective heat transfer! When we figured that out it seemed that everyone was happy with what was a confusing issue. If we had instead resorted to thinking about finned surfaces (like the radiator in your car, the little do-dads in your computer, etc.) we may have realized earlier that sometimes adding material increases heat transfer (as long as the increase in surface area is sufficient to cause the convection to overcome the added conductive resistance). This will be our topic for a short while. Having said that, I am sure that it is perfectly clear that often, when we need to increase the rate of heat transfer through a material, we may add fins! Some typical fin configurations are shown below. As I am sure that you can imagine, fins are tremendously technologically important items (as Chem. E's we would certainly be interested in their use in heat exchangers!). So, how do we handle these things?

SIB: Using the Fin Efficiency The more practical use of the fin efficiency lies in the fact that, once it is calculated, the resulting dimensionless expression can be used to easily determine the actual heat flow from any similar fin. In other words, we can rearrange the fin efficiency definition to yield: so that simply "looking up" the efficiency value yields our solution. OUTCOME: Calculate the heat flow through a fin from the fin's efficiency TEST YOURSELF Let's look at an example... You are evaluating the introduction of "pin"-type fins onto the surface of your company's new heat exchanger. You suggest that, in order to compare the two scenario's realistically, you need to calculate the heat flow both with and without the fin. As long as you get at least a 10% increase in heat flow, you will go ahead and do it. Should you do it? (Your proposal is to put 25 aluminum (k=200w/mk) pins that are 3 cm long fins of 1 cm diameter on every 100 cm 2 of surface. Your heat transfer coefficient is 10 W/m 2 K.) Since the heat flow off the unfinned surface and the fins themselves are in parallel, we simply add them to get the total heat flow, so where A o is the area of the unfinned surface.

We can therefore think of the fin efficiency as a correction factor for the amount of the surface area of the fin that is actually "useful" (as useful as the unfinned surface, that is). One final important issue to note is that the simple expression for fin heat flow, lends itself quite easily to our resistor analysis, to yield Be careful to remember that the fin heat flow (and therefore the fin resistance) accounts for both conduction and convection through/off the fin.