PROBLEM cos 30. With A 1 = A 2 = A 3 = A 4 = 10-3 m 2 and the incident radiation rates q 1-j from the results of Example 12.
|
|
- Ernest Stevenson
- 5 years ago
- Views:
Transcription
1 PROBLEM. KNON: Rate at which radiation is intercepted by each of three surfaces (see (Example.). FIND: Irradiation, G[/m ], at each of the three surfaces. ANALYSIS: The irradiation at a surface is the rate at which radiation is incident on a surface per unit area of the surface. The irradiation at surface j due to emission from surface is q j G j =. Aj ith A = A = A 3 = A 4 = 0-3 m and the incident radiation rates q -j from the results of Example., find. 0 3 G = =./m 0 3 m G 3 = = 8.0/m 0 3 m G 4 = = 9.8/m. 0 3 m COMMENTS: The irradiation could also be computed from Eq..5, which, for the present situation, takes the form Gj = Icosθjω j where I = I = 7000 /m sr and ω -j is the solid angle subtended by surface with respect to j. For example, G = Icosθω G = 7000/m sr 0 3 m cos60 cos 30 G =./m. ( 0.5m) Note that, since A is a diffuse radiator, the intensity I is independent of direction.
2 PROBLEM. KNON: A diffuse surface of area A = 0-4 m emits diffusely with total emissive power E = /m. FIND: (a) Rate this emission is intercepted by small surface of area A = m at a prescribed location and orientation, (b) Irradiation G on A, and (c) Compute and plot G as a function of the separation distance r for the range 0.5 r.0 m for zenith angles θ = 0, 30 and 60. ASSUMPTIONS: () Surface A emits diffusely, () A may be approximated as a differential surface area and that A r. ANALYSIS: (a) The rate at which emission from A is intercepted by A follows from Eq..5 written on a total rather than spectral basis. ( ) q = I e, θφ, Acosθdω. () Since the surface A is diffuse, it follows from Eq..3 that ( θφ) I e,, = Ie, = E π. () The solid angle subtended by A with respect to A is dω A cosθ r. (3) Substituting Eqs. () and (3) into Eq. () with numerical values gives 4 4 $ E A cosθ 5 0 m 5 0 m cos 30 q Acosθ = 0 m cos 60 sr (4) π r π sr ( 0.5m) q = 5,95 m sr 5 0 m.73 0 sr = ( ) = 4 $ ( ) (b) From section,.3, the irradiation is the rate at which radiation is incident upon the surface per unit surface area, 3 q G = = =.76 m (5) A m (c) Using the IHT workspace with the foregoing equations, the G was computed as a function of the separation distance for selected zenith angles. The results are plotted below. Continued...
3 PROBLEM. (Cont.) Irradiation, G (/m^) theta = 0 deg theta = 30 deg theta = 60 deg Separation distance, r (m) For all zenith angles, G decreases with increasing separation distance r. From Eq. (3), note that dω - and, hence G, vary inversely as the square of the separation distance. For any fixed separation distance, G is a maximum when θ = 0 and decreases with increasing θ, proportional to cos θ. COMMENTS: () For a diffuse surface, the intensity, I e, is independent of direction and related to the emissive power as I e = E/ π. Note that π has the units of [ sr ] in this relation. () Note that Eq..5 is an important relation for determining the radiant power leaving a surface in a prescribed manner. It has been used here on a total rather than spectral basis. (3) Returning to part (b) and referring to Figure.0, the irradiation on A may be expressed as Acosθ G = Ii,cosθ r Show that the result is G =.76 /m. Explain how this expression follows from Eq. (.5).
4 PROBLEM.3 KNON: Hot part, A p, located a distance x from an origin directly beneath a motion sensor at a distance L d = m. FIND: (a) Location x at which sensor signal S will be 75% that corresponding to x = 0, directly beneath the sensor, S o, and (b) Compute and plot the signal ratio, S/S o, as a function of the part position x for the range 0. S/S o for L d = 0.8,.0 and. m; compare the x-location for each value of L d at which S/S o = ASSUMPTIONS: () Hot part is diffuse emitter, () L d >> A p, A o. ANALYSIS: (a) The sensor signal, S, is proportional to the radiant power leaving A p and intercepted by A d, when Hence, S~qp d = Ip,e Apcosθp ωd p () Ld / cosθp = cosθd = = L d (Ld + x ) () R Ad cosθd 3/ ωd p = = A d L d (Ld + x ) (3) R L q d p d = Ip,e Ap Ad (Ld + x ) It follows that, with S o occurring when x= 0 and L d = m, S L d (Ld + x ) L = = d S o L d (Ld + 0 ) Ld + x so that when S/S o = 0.75, find, x = m (b) Using Eq. (5) in the IHT workspace, the signal ratio, S/S o, has been computed and plotted as a function of the part position x for selected L d values. (4) (5) Continued...
5 PROBLEM.3 (Cont.) 0.8 Signal ratio, S/So Part position, x (m) Sensor position, Ld = 0.8 m Ld = m Ld =. m hen the part is directly under the sensor, x = 0, S/S o = for all values of L d. ith increasing x, S/S o decreases most rapidly with the smallest L d. From the IHT model we found the part position x corresponding to S/S o = 0.75 as follows. S/S o L d (m) x (m) If the sensor system is set so that when S/S o reaches 0.75 a process is initiated, the technician can use the above plot and table to determine at what position the part will begin to experience the treatment process.
6 PROBLEM 3. KNON: Various geometric shapes involving two areas A and A. FIND: Shape factors, F and F, for each configuration. ASSUMPTIONS: Surfaces are diffuse. ANALYSIS: The analysis is not to make use of tables or charts. The approach involves use of the reciprocity relation, Eq. 3.3, and summation rule, Eq Recognize that reciprocity applies to two surfaces; summation applies to an enclosure. Certain shape factors will be identified by inspection. Note L is the length normal to page. (a) Long duct (L): By inspection, F =.0 By reciprocity, A RL 4 F = F =.0 = = 0.44 A ( 3/4) πrl 3π (b) Small sphere, A, under concentric hemisphere, A, where A = A Summation rule F + F + F3 = But F = F 3 by symmetry, hence F = 0.50 A A By reciprocity, F = F = 0.5 = 0.5. A A (c) Long duct (L): By inspection, F =.0 (d) Long inclined plates (L): By reciprocity, A RL F = F =.0 = = A πrl π Summation rule, F = F = 0.64 = Summation rule, F + F + F3 = But F = F 3 by symmetry, hence F = 0.50 A 0L By reciprocity, F = F = 0.5 = A / 0 L () (e) Sphere lying on infinite plane Summation rule, F + F + F 3 = But F = F 3 by symmetry, hence F = 0.5 A By reciprocity, F = F 0 since A. A Continued..
7 PROBLEM 3. (Cont.) (f) Hemisphere over a disc of diameter D/; find also F and F 3. By inspection, F =.0 Summation rule for surface A 3 is written as F3 + F3 + F33 =. Hence, F3 =.0. By reciprocity, A F 3 3 = F3 A πd π ( D/) D π F 3 = /.0 = By reciprocity, A π D πd F = F = / A 4 = Summation rule for A, F + F + F3 = or Note that by inspection you can deduce F = 0.5 (g) Long open channel (L): F = F F3 = = 0.5. Summation rule for A F + F + F3 = 0 but F = F 3 by symmetry, hence F = By reciprocity, A L 4 F = F = = 0.50 = A ( π )/4 L π COMMENTS: () Note that the summation rule is applied to an enclosure. To complete the enclosure, it was necessary in several cases to define a third surface which was shown by dashed lines. () Recognize that the solutions follow a systematic procedure; in many instances it is possible to deduce a shape factor by inspection.
8 PROBLEM 3. KNON: Geometry of semi-circular, rectangular and V grooves. FIND: (a) View factors of grooves with respect to surroundings, (b) View factor for sides of V groove, (c) View factor for sides of rectangular groove. ASSUMPTIONS: () Diffuse surfaces, () Negligible end effects, long grooves. ANALYSIS: (a) Consider a unit length of each groove and represent the surroundings by a hypothetical surface (dashed line). Semi-Circular Groove: A F = ; F = F = A ( π /) F = / π. Rectangular Groove: A4 F4,,3 ( ) = ; F(,,34 ) = F4,,3 ( ) = A+ A + A3 H+ + H F,,3 4 = / + H. ( ) ( ) V Groove: A F 3 3, ( ) = ; F(,3 ) = F A 3, ( ) = + A (b) From Eqs. 3.3 and 3.4, F = sin θ. (,) 3 From Symmetry, F3 = /. Hence, ( ) A F 3 = F3 = F 3. A / / + sinθ sinθ F = or F = sin θ. / /sinθ (c) From Fig. 3.4, with X/L = H/ = and Y/L, F 0.6. COMMENTS: () Note that for the V groove, F 3 = F 3 = F (,)3 = sinθ, () In part (c), Fig. 3.4 could also be used with Y/L = and X/L =. However, obtaining the limit of F ij as X/L from the figure is somewhat uncertain.
9 PROBLEM 3.0 KNON: Arrangement of perpendicular surfaces without a common edge. FIND: (a) A relation for the view factor F 4 and (b) The value of F 4 for prescribed dimensions. ASSUMPTIONS: () Diffuse surfaces. ANALYSIS: (a) To determine F 4, it is convenient to define the hypothetical surfaces A and A 3. From Eq. 3.6, A + A F, 3,4 = A F 3,4 + A F 3,4 ( ) ( )( ) ( ) ( ) where F (,)(3,4) and F (3,4) may be obtained from Fig Substituting for A F (3,4) from Eq. 3.5 and combining expressions, find A F3,4 = A F3 + A F4 ( ) F 4 = ( A A ) F (,)( 3,4) A F 3 A F ( 3,4). A + Substituting for A F 3 from Eq. 3.6, which may be expressed as A + A F, 3 = A F 3 + A F 3. ( ) ( ) The desired relation is then F 4 = ( A + A ) F (,)( 3,4) + A F 3 ( A + A ) F (,) 3 A F ( 3,4). A (b) For the prescribed dimensions and using Fig. 3.6, find these view factors: Surfaces (,)(3,4) L+ L L3 + L4 ( Y / X) = =, ( Z / X) = =.45, F(,)( 3,4) = 0. Surfaces 3 L L3 ( Y / X) = = 0.5, ( Z / X) = =, F3 = 0.8 Surfaces (,)3 L+ L L3 ( Y / X) = =, ( Z / X) = =, F(,) 3 = 0.0 Surfaces (3,4) L L3 + L4 ( Y / X) = = 0.5, ( Z / X) = =.5, F3,4 ( ) = 0.3 Using the relation above, find F4 = ( ) L + L ) 0. + ( L ) 0.8 ( L + L ) 0.0 ( L ) 0.3 ] L F4 = [ ( 0.) + ( 0.8) ( 0.0) ( 0.3) ] = 0.0.
10 PROBLEM 3. KNON: Coaxial, parallel black plates with surroundings. Lower plate (A ) maintained at prescribed temperature T while electrical power is supplied to upper plate (A ). FIND: Temperature of the upper plate T. ASSUMPTIONS: () Plates are black surfaces of uniform temperature, and () Backside of heater on A insulated. ANALYSIS: The net radiation heat rate leaving A i is N Pe = qij = AFσ T T + AF3σ T T3 j= ( ) ( ) ( ) ( ) Pe = Aσ F T T + F3 T T sur From Fig. 3.5 for coaxial disks (see Table 3.), R = r / L = 0.0 m / 0.0 m = 0.5 R = r / L = 0.0 m / 0.0 m =.0 + R + S = + = + = 9.0 R ( 0.5) () / / F = S S 4( r / r ) = 9 9 4( 0. / 0.) = From the summation rule for the enclosure A, A and A 3 where the last area represents the surroundings with T 3 = T sur, F + F3 = F3 = F = = Substituting numerical values into Eq. (), with A = π D / 4 = m, = m / m K T 500 K ( ) ( ) ( ) T 300 K = T T 300 ( ) find by trial-and-error that T = 456 K. COMMENTS: Note that if the upper plate were adiabatic, T = 47 K.
11 PROBLEM 3.53 KNON: Emissivities, diameters and temperatures of concentric spheres. FIND: (a) Radiation transfer rate for black surfaces. (b) Radiation transfer rate for diffuse-gray surfaces, (c) Effects of increasing the diameter and assuming blackbody behavior for the outer sphere. (d) Effect of emissivities on net radiation exchange. ASSUMPTIONS: () Blackbody or diffuse-gray surface behavior. ANALYSIS: (a) Assuming blackbody behavior, it follows from Eq ( ) π( ) ( ) ( ) ( ) 4 4 q = AF σ T T = 0.8 m / m K 400 K 300 K = 995. (b) For diffuse-gray surface behavior, it follows from Eq. 3.6 ( ) π( ) σ A T 4 T / m K m K 4 q = = = 9. ε r ε ε r (c) ith D = 0 m, it follows from Eq / m Kπ ( 0.8m) ( 400 K) ( 300 K ) q = = ith ε =, instead of 0.05, Eq. 3.6 reduces to Eq. 3.7 and ( ) ( ) ( ) ( ) 4 4 q = σaε T T = / m K π 0.8 m K 300 K = 998. Continued..
12 PROBLEM 3.53 (Cont.) (d) Using the IHT Radiation Tool Pad, the following results were obtained Net radiation exchange increases with ε and ε, and the trends are due to increases in emission from and absorption by surfaces and, respectively. COMMENTS: From part (c) it is evident that the actual surface emissivity of a large enclosure has a small effect on radiation exchange with small surfaces in the enclosure. orking with ε =.0 instead of ε = 0.05, the value of q is increased by only ( )/983 =.5%. In contrast, from the results of (d) it is evident that the surface emissivity ε of a small enclosure has a large effect on radiation exchange with interior objects, which increases with increasing ε.
PROBLEM L. (3) Noting that since the aperture emits diffusely, I e = E/π (see Eq ), and hence
PROBLEM 1.004 KNOWN: Furnace with prescribed aperture and emissive power. FIND: (a) Position of gauge such that irradiation is G = 1000 W/m, (b) Irradiation when gauge is tilted θ d = 0 o, and (c) Compute
More informationPROBLEM (a) Long duct (L): By inspection, F12. By reciprocity, (b) Small sphere, A 1, under concentric hemisphere, A 2, where A 2 = 2A
PROBLEM 3. KNON: Various geometric shapes involving two areas and. FIND: Shape factors, F and F, for each configuration. SSUMPTIONS: Surfaces are diffuse. NLYSIS: The analysis is not to make use of tables
More informationPROBLEM (a) Long duct (L): By inspection, F12. By reciprocity, (b) Small sphere, A 1, under concentric hemisphere, A 2, where A 2 = 2A
PROBLEM 3. KNON: Various geometric shapes involving two areas and. FIND: Shape factors, F and F, for each configuration. SSUMPTIONS: Surfaces are diffuse. NLYSIS: The analysis is not to make use of tables
More informationb( ) ) ( ) PROBLEM = W / m = 1991 W / m. = W / m 4 m = 3164 W.
PROBLEM.6 KNOWN: rea, temperature, irradiation and spectral absorptivity of a surface. FIND: bsorbed irradiation, emissive power, radiosity and net radiation transfer from the surface. SCHEMTIC: SSUMPTIONS:
More informationProblem One Answer the following questions concerning fundamental radiative heat transfer. (2 points each) Part Question Your Answer
Problem One Answer the following questions concerning fundamental radiative heat transfer. ( points each) Part Question Your Answer A Do all forms of matter emit radiation? Yes B Does the transport of
More informationAdvanced Heat and Mass Transfer by Amir Faghri, Yuwen Zhang, and John R. Howell
Advanced Heat and Mass Transfer by Amir Faghri, Yuwen Zhang, and John R. Howell 9.2 The Blackbody as the Ideal Radiator A material that absorbs 100 percent of the energy incident on it from all directions
More informationME 476 Solar Energy UNIT TWO THERMAL RADIATION
ME 476 Solar Energy UNIT TWO THERMAL RADIATION Unit Outline 2 Electromagnetic radiation Thermal radiation Blackbody radiation Radiation emitted from a real surface Irradiance Kirchhoff s Law Diffuse and
More informationNumerical Heat and Mass Transfer
Master Degree in Mechanical Engineering Numerical Heat and Mass Transfer 11-Radiative Heat Transfer Fausto Arpino f.arpino@unicas.it Nature of Thermal Radiation ü Thermal radiation refers to radiation
More informationReading Problems , 15-33, 15-49, 15-50, 15-77, 15-79, 15-86, ,
Radiation Heat Transfer Reading Problems 15-1 15-7 15-27, 15-33, 15-49, 15-50, 15-77, 15-79, 15-86, 15-106, 15-107 Introduction The following figure shows the relatively narrow band occupied by thermal
More informationRadiation Heat Transfer. Introduction. Blackbody Radiation
Radiation Heat Transfer Reading Problems 21-1 21-6 21-21, 21-24, 21-41, 21-61, 21-69 22-1 21-5 22-11, 22-17, 22-26, 22-36, 22-71, 22-72 Introduction It should be readily apparent that radiation heat transfer
More informationRadiation Heat Transfer. Introduction. Blackbody Radiation. Definitions ,
Radiation Heat Transfer Reading Problems 5-5-7 5-27, 5-33, 5-50, 5-57, 5-77, 5-79, 5-96, 5-07, 5-08 Introduction A narrower band inside the thermal radiation spectrum is denoted as the visible spectrum,
More informationChapter 1 Solar Radiation
Chapter 1 Solar Radiation THE SUN The sun is a sphere of intensely hot gaseous matter with a diameter of 1.39 10 9 m It is, on the average, 1.5 10 11 m away from the earth. The sun rotates on its axis
More informationG α Absorbed irradiation
Thermal energy emitted y matter as a result of virational and rotational movements of molecules, atoms and electrons. The energy is transported y electromagnetic waves (or photons). adiation reuires no
More informationFundamental Concepts of Radiation -Basic Principles and Definitions- Chapter 12 Sections 12.1 through 12.3
Fundamental Concepts of Radiation -Basic Principles and Definitions- Chapter 1 Sections 1.1 through 1.3 1.1 Fundamental Concepts Attention is focused on thermal radiation, whose origins are associated
More informationAutumn 2005 THERMODYNAMICS. Time: 3 Hours
CORK INSTITUTE OF TECHNOOGY Bachelor of Engineering (Honours) in Mechanical Engineering Stage 3 (Bachelor of Engineering in Mechanical Engineering Stage 3) (NFQ evel 8) Autumn 2005 THERMODYNAMICS Time:
More informationPROBLEM Node 5: ( ) ( ) ( ) ( )
PROBLEM 4.78 KNOWN: Nodal network and boundary conditions for a water-cooled cold plate. FIND: (a) Steady-state temperature distribution for prescribed conditions, (b) Means by which operation may be extended
More informationThe Planck Distribution. The Planck law describes theoretical spectral distribution for the emissive power of a black body. It can be written as
Thermal energy emitted y matter as a result of virational and rotational movements of molecules, atoms and electrons. The energy is transported y electromagnetic waves (or photons). adiation reuires no
More information11. Advanced Radiation
. Advanced adiation. Gray Surfaces The gray surface is a medium whose monochromatic emissivity ( λ does not vary with wavelength. The monochromatic emissivity is defined as the ratio of the monochromatic
More informationIndo-German Winter Academy
Indo-German Winter Academy - 2007 Radiation in Non-Participating and Participating Media Tutor Prof. S. C. Mishra Technology Guwahati Chemical Engineering Technology Guwahati 1 Outline Importance of thermal
More informationSOLUTIONS. Question 6-12:
Federal University of Rio Grande do Sul Mechanical Engineering Department MEC0065 - Thermal Radiation Professor - Francis Name: Márleson Rôndiner dos Santos Ferreira Question 6-1: SOLUTIONS (a) A circular
More informationQUESTION ANSWER. . e. Fourier number:
QUESTION 1. (0 pts) The Lumped Capacitance Method (a) List and describe the implications of the two major assumptions of the lumped capacitance method. (6 pts) (b) Define the Biot number by equations and
More informationMASSCHUSETTS INSTITUTE OF TECHNOLOGY ESG Physics. Problem Set 8 Solution
MASSCHUSETTS INSTITUTE OF TECHNOLOGY ESG Physics 8.0 with Kai Spring 003 Problem : 30- Problem Set 8 Solution Determine the magnetic field (in terms of I, a and b) at the origin due to the current loop
More informationIntroduction to Computer Vision Radiometry
Radiometry Image: two-dimensional array of 'brightness' values. Geometry: where in an image a point will project. Radiometry: what the brightness of the point will be. Brightness: informal notion used
More informationME 315 Final Examination Solution 8:00-10:00 AM Friday, May 8, 2009 CIRCLE YOUR DIVISION
ME 315 Final Examination Solution 8:00-10:00 AM Friday, May 8, 009 This is a closed-book, closed-notes examination. There is a formula sheet at the back. You must turn off all communications devices before
More informationChapter 22. Dr. Armen Kocharian. Gauss s Law Lecture 4
Chapter 22 Dr. Armen Kocharian Gauss s Law Lecture 4 Field Due to a Plane of Charge E must be perpendicular to the plane and must have the same magnitude at all points equidistant from the plane Choose
More information( ) PROBLEM C 10 C 1 L m 1 50 C m K W. , the inner surface temperature is. 30 W m K
PROBLEM 3. KNOWN: Temperatures and convection coefficients associated with air at the inner and outer surfaces of a rear window. FIND: (a) Inner and outer window surface temperatures, T s,i and T s,o,
More informationC ONTENTS CHAPTER TWO HEAT CONDUCTION EQUATION 61 CHAPTER ONE BASICS OF HEAT TRANSFER 1 CHAPTER THREE STEADY HEAT CONDUCTION 127
C ONTENTS Preface xviii Nomenclature xxvi CHAPTER ONE BASICS OF HEAT TRANSFER 1 1-1 Thermodynamics and Heat Transfer 2 Application Areas of Heat Transfer 3 Historical Background 3 1-2 Engineering Heat
More informationRadiation Heat Transfer Experiment
Radiation Heat Transfer Experiment Thermal Network Solution with TNSolver Bob Cochran Applied Computational Heat Transfer Seattle, WA rjc@heattransfer.org ME 331 Introduction to Heat Transfer University
More informationRadiative heat transfer
Radiative heat transfer 22 mars 2017 Energy can be transported by the electromagnetic field radiated by an object at finite temperature. A very important example is the infrared radiation emitted towards
More informationSolutions Mock Examination
Solutions Mock Examination Elena Rossi December 18, 2013 1. The peak frequency will be given by 4 3 γ2 ν 0. 2. The Einstein coeffients present the rates for the different processes populating and depopulating
More informationWhat is it good for? RT is a key part of remote sensing and climate modeling.
Read Bohren and Clothiaux Ch.; Ch 4.-4. Thomas and Stamnes, Ch..-.6; 4.3.-4.3. Radiative Transfer Applications What is it good for? RT is a key part of remote sensing and climate modeling. Remote sensing:
More informationRadiometry HW Problems 1
Emmett J. Ientilucci, Ph.D. Digital Imaging and Remote Sensing Laboratory Rochester Institute of Technology March 7, 007 Radiometry HW Problems 1 Problem 1. Your night light has a radiant flux of 10 watts,
More informationThermal Radiation Effects on Deep-Space Satellites Part 2
Thermal Radiation Effects on Deep-Space Satellites Part 2 Jozef C. Van der Ha www.vanderha.com Fundamental Physics in Space, Bremen October 27, 2017 Table of Contents Mercury Properties & Parameters Messenger
More informationHeat Transfer: Physical Origins and Rate Equations. Chapter One Sections 1.1 and 1.2
Heat Transfer: Physical Origins and Rate Equations Chapter One Sections 1.1 and 1. Heat Transfer and Thermal Energy What is heat transfer? Heat transfer is thermal energy in transit due to a temperature
More informationTFAWS 2005 Short Course
C&R ECHNOLOGIES FAWS 005 Short Course Non-Grey and emperature Dependent Radiation Analysis Methods im Panczak Additional Charts & Data Provided by Dan Green Ball Aerospace Corporation djgreen@ball.com
More information( )( ) PROBLEM 9.5 (1) (2) 3 (3) Ra g TL. h L (4) L L. q ( ) 0.10/1m ( C /L ) Ra 0.59/0.6m L2
PROBEM 9.5 KNOWN: Heat transfer rate by convection from a vertical surface, 1m high by 0.m wide, to quiescent air that is 0K cooler. FIND: Ratio of the heat transfer rate for the above case to that for
More informationPROBLEM 1.3. dt T1 T dx L 0.30 m
PROBLEM 1.3 KNOWN: Inner surface temperature and thermal conductivity of a concrete wall. FIND: Heat loss by conduction through the wall as a function of outer surface temperatures ranging from -15 to
More informationRadiation in the atmosphere
Radiation in the atmosphere Flux and intensity Blackbody radiation in a nutshell Solar constant Interaction of radiation with matter Absorption of solar radiation Scattering Radiative transfer Irradiance
More informationqxbxg. That is, the heat rate within the object is everywhere constant. From Fourier s
PROBLEM.1 KNOWN: Steady-state, one-dimensional heat conduction through an axisymmetric shape. FIND: Sketch temperature distribution and explain shape of curve. ASSUMPTIONS: (1) Steady-state, one-dimensional
More informationThermal Radiation By: Prof. K M Joshi
Thermal Radiation By: Prof. K M Joshi Radiation originate due to emission of matter and its subsequent transports does not required any matter / medium. Que: Then what is the nature of this transport???
More informationECE309 INTRODUCTION TO THERMODYNAMICS & HEAT TRANSFER. 10 August 2005
ECE309 INTRODUCTION TO THERMODYNAMICS & HEAT TRANSFER 0 August 2005 Final Examination R. Culham & M. Bahrami This is a 2 - /2 hour, closed-book examination. You are permitted to use one 8.5 in. in. crib
More information12.815/12.816: RADIATIVE TRANSFER PROBLEM SET #1 SOLUTIONS
12.815/12.816: RADIATIVE TRANSFER PROBLEM SET #1 SOLUTIONS TA: NIRAJ INAMDAR 1) Radiation Terminology. We are asked to define a number of standard terms. See also Table 1. Intensity: The amount of energy
More informationChapter 24 Solutions The uniform field enters the shell on one side and exits on the other so the total flux is zero cm cos 60.
Chapter 24 Solutions 24.1 (a) Φ E EA cos θ (3.50 10 3 )(0.350 0.700) cos 0 858 N m 2 /C θ 90.0 Φ E 0 (c) Φ E (3.50 10 3 )(0.350 0.700) cos 40.0 657 N m 2 /C 24.2 Φ E EA cos θ (2.00 10 4 N/C)(18.0 m 2 )cos
More informationConduction and radiation Prof. C. Balaji Department of Mechanical Engineering Indian Institute of Technology, Madras
Conduction and radiation Prof. C. Balaji Department of Mechanical Engineering Indian Institute of Technology, Madras Module No. #01 Lecture No. #03 Solid angle, spectral radiation intensity In yesterday
More information3 Chapter. Gauss s Law
3 Chapter Gauss s Law 3.1 Electric Flux... 3-2 3.2 Gauss s Law (see also Gauss s Law Simulation in Section 3.10)... 3-4 Example 3.1: Infinitely Long Rod of Uniform Charge Density... 3-9 Example 3.2: Infinite
More informationSOLUTIONS. F 0 λ1 T = (1) F 0 λ2 T = (2) ε = (6) F 0 λt = (7) F 0 λt = (11)
Federal University of Rio Grande do Sul Mechanical Engineering Department MEC0065 - Thermal Radiation Professor - Francis Name: Márleson Rôndiner dos Santos Ferreira SOLUTIONS Question 2-5: The total hemispherical
More informationpoint, corresponding to the area it cuts out: θ = (arc length s) / (radius of the circle r) in radians Babylonians:
Astronomische Waarneemtechnieken (Astronomical Observing Techniques) 1 st Lecture: 1 September 11 This lecture: Radiometry Radiative transfer Black body radiation Astronomical magnitudes Preface: The Solid
More informationRadiation from planets
Chapter 4 Radiation from planets We consider first basic, mostly photometric radiation parameters for solar system planets which can be easily compared with existing or future observations of extra-solar
More informationCOVENANT UNIVERSITY NIGERIA TUTORIAL KIT OMEGA SEMESTER PROGRAMME: MECHANICAL ENGINEERING
COVENANT UNIVERSITY NIGERIA TUTORIAL KIT OMEGA SEMESTER PROGRAMME: MECHANICAL ENGINEERING COURSE: MCE 524 DISCLAIMER The contents of this document are intended for practice and leaning purposes at the
More informationGoal: The theory behind the electromagnetic radiation in remote sensing. 2.1 Maxwell Equations and Electromagnetic Waves
Chapter 2 Electromagnetic Radiation Goal: The theory behind the electromagnetic radiation in remote sensing. 2.1 Maxwell Equations and Electromagnetic Waves Electromagnetic waves do not need a medium to
More informationChapter 2 Gauss Law 1
Chapter 2 Gauss Law 1 . Gauss Law Gauss law relates the electric fields at points on a (closed) Gaussian surface to the net charge enclosed by that surface Consider the flux passing through a closed surface
More informationApplied Thermodynamics HEAT TRANSFER. Introduction What and How?
LANDMARK UNIVERSITY, OMU-ARAN LECTURE NOTE: 3 COLLEGE: COLLEGE OF SCIENCE AND ENGINEERING DEPARTMENT: MECHANICAL ENGINEERING PROGRAMME: ENGR. ALIYU, S.J Course code: MCE 311 Course title: Applied Thermodynamics
More informationRADIATIVE VIEW FACTORS
RADIATIVE VIEW ACTORS View factor definition... View factor algebra... Wit speres... 3 Patc to a spere... 3 rontal... 3 Level... 3 Tilted... 3 Disc to frontal spere... 3 Cylinder to large spere... Cylinder
More information1. ELECTRIC CHARGES AND FIELDS
1. ELECTRIC CHARGES AND FIELDS 1. What are point charges? One mark questions with answers A: Charges whose sizes are very small compared to the distance between them are called point charges 2. The net
More informationAT622 Section 2 Elementary Concepts of Radiometry
AT6 Section Elementary Concepts of Radiometry The object of this section is to introduce the student to two radiometric concepts intensity (radiance) and flux (irradiance). These concepts are largely geometrical
More informationASSUMPTIONS: (1) Homogeneous medium with constant properties, (2) Negligible radiation effects.
PROBEM 5.88 KNOWN: Initial temperature of fire clay bric which is cooled by convection. FIND: Center and corner temperatures after 50 minutes of cooling. ASSUMPTIONS: () Homogeneous medium with constant
More informationPhysics 3211: Electromagnetic Theory (Tutorial)
Question 1 a) The capacitor shown in Figure 1 consists of two parallel dielectric layers and a voltage source, V. Derive an equation for capacitance. b) Find the capacitance for the configuration of Figure
More informationChapter 21 Chapter 23 Gauss Law. Copyright 2014 John Wiley & Sons, Inc. All rights reserved.
Chapter 21 Chapter 23 Gauss Law Copyright 23-1 What is Physics? Gauss law relates the electric fields at points on a (closed) Gaussian surface to the net charge enclosed by that surface. Gauss law considers
More informationUNIT FOUR SOLAR COLLECTORS
ME 476 Solar Energy UNIT FOUR SOLAR COLLECTORS Flat Plate Collectors Outline 2 What are flat plate collectors? Types of flat plate collectors Applications of flat plate collectors Materials of construction
More informationASSUMPTIONS: (1) One-dimensional, radial conduction, (2) Constant properties.
PROBLEM 5.5 KNOWN: Diameter and radial temperature of AISI 00 carbon steel shaft. Convection coefficient and temperature of furnace gases. FIND: me required for shaft centerline to reach a prescribed temperature.
More informationME 476 Solar Energy UNIT THREE SOLAR RADIATION
ME 476 Solar Energy UNIT THREE SOLAR RADIATION Unit Outline 2 What is the sun? Radiation from the sun Factors affecting solar radiation Atmospheric effects Solar radiation intensity Air mass Seasonal variations
More informationCh 24 Electric Flux, & Gauss s Law
Ch 24 Electric Flux, & Gauss s Law Electric Flux...is related to the number of field lines penetrating a given surface area. Φ e = E A Φ = phi = electric flux Φ units are N m 2 /C Electric Flux Φ = E A
More informationChapter 11 FUNDAMENTALS OF THERMAL RADIATION
Chapter Chapter Fundamentals of Thermal Radiation FUNDAMENTALS OF THERMAL RADIATION Electromagnetic and Thermal Radiation -C Electromagnetic waves are caused by accelerated charges or changing electric
More information- 1 - θ 1. n 1. θ 2. mirror. object. image
TEST 5 (PHY 50) 1. a) How will the ray indicated in the figure on the following page be reflected by the mirror? (Be accurate!) b) Explain the symbols in the thin lens equation. c) Recall the laws governing
More informationSolar radiation / radiative transfer
Solar radiation / radiative transfer The sun as a source of energy The sun is the main source of energy for the climate system, exceeding the next importat source (geothermal energy) by 4 orders of magnitude!
More informationHandout 6: Rotational motion and moment of inertia. Angular velocity and angular acceleration
1 Handout 6: Rotational motion and moment of inertia Angular velocity and angular acceleration In Figure 1, a particle b is rotating about an axis along a circular path with radius r. The radius sweeps
More informationAppendix A. Longwave radiation in a canopy stand
213 Appendix A. ongwave radiation in a canopy stand The longwave radiation transfer equations can be written as (Ross, 1981): di ld (,r) d cosθ = G(,r)i ld (,r)+η,r ( ) (A.1) di lu ( ),r d cosφ = G,r (
More informationinnova-ve entrepreneurial global 1
www.utm.my innova-ve entrepreneurial global 1 The science of how heat flows is called heat transfer. There are three ways heat transfer works: conduction, convection, and radiation. Heat flow depends on
More informationCalculating equation coefficients
Solar Energy 1 Calculating equation coefficients Construction Conservation Equation Surface Conservation Equation Fluid Conservation Equation needs flow estimation needs radiation and convection estimation
More informationChapter 2: Steady Heat Conduction
2-1 General Relation for Fourier s Law of Heat Conduction 2-2 Heat Conduction Equation 2-3 Boundary Conditions and Initial Conditions 2-4 Variable Thermal Conductivity 2-5 Steady Heat Conduction in Plane
More informationdt Now we will look at the E&M force on moving charges to explore the momentum conservation law in E&M.
. Momentum Conservation.. Momentum in mechanics In classical mechanics p = m v and nd Newton s law d p F = dt If m is constant with time d v F = m = m a dt Now we will look at the &M force on moving charges
More informationDr. Linlin Ge The University of New South Wales
GMAT 9600 Principles of Remote Sensing Week2 Electromagnetic Radiation: Definition & Physics Dr. Linlin Ge www.gmat.unsw.edu.au/linlinge Basic radiation quantities Outline Wave and quantum properties Polarization
More informationLecture Notes Prepared by Mike Foster Spring 2007
Lecture Notes Prepared by Mike Foster Spring 2007 Solar Radiation Sources: K. N. Liou (2002) An Introduction to Atmospheric Radiation, Chapter 1, 2 S. Q. Kidder & T. H. Vander Haar (1995) Satellite Meteorology:
More informationFIND: (a) Sketch temperature distribution, T(x,t), (b) Sketch the heat flux at the outer surface, q L,t as a function of time.
PROBLEM 5.1 NOWN: Electrical heater attached to backside of plate while front surface is exposed to convection process (T,h); initially plate is at a uniform temperature of the ambient air and suddenly
More informationReview: Conduction. Breaking News
CH EN 3453 Heat Transfer Review: Conduction Breaking News No more homework (yay!) Final project reports due today by 8:00 PM Email PDF version to report@chen3453.com Review grading rubric on Project page
More informationObserver-Sun Angles. ), Solar altitude angle (α s. ) and solar azimuth angle (γ s )). θ z. = 90 o α s
Observer-Sun Angles Direction of Beam Radiation: The geometric relationships between a plane of any particular orientation relative to the earth at any time and the incoming beam solar radiation can be
More information1 Conduction Heat Transfer
Eng6901 - Formula Sheet 3 (December 1, 2015) 1 1 Conduction Heat Transfer 1.1 Cartesian Co-ordinates q x = q xa x = ka x dt dx R th = L ka 2 T x 2 + 2 T y 2 + 2 T z 2 + q k = 1 T α t T (x) plane wall of
More informationINTRODUCTION TO MICROWAVE REMOTE SENSING - II. Dr. A. Bhattacharya
1 INTRODUCTION TO MICROWAVE REMOTE SENSING - II Dr. A. Bhattacharya The Radiation Framework The information about features on the Earth s surface using RS depends on measuring energy emanating from the
More informationHeriot-Watt University
Heriot-Watt University Distinctly Global www.hw.ac.uk Thermodynamics By Peter Cumber Prerequisites Interest in thermodynamics Some ability in calculus (multiple integrals) Good understanding of conduction
More informationPROBLEM 9.3. KNOWN: Relation for the Rayleigh number. FIND: Rayleigh number for four fluids for prescribed conditions. SCHEMATIC:
PROBEM.3 KNOWN: Relation for the Rayleigh number. FIND: Rayleigh number for four fluids for prescribed conditions. ASSUMPTIONS: (1 Perfect gas behavior for specified gases. PROPERTIES: Table A-4, Air (400K,
More informationChapter 1: 20, 23, 35, 41, 68, 71, 76, 77, 80, 85, 90, 101, 103 and 104.
Chapter 1: 0, 3, 35, 1, 68, 71, 76, 77, 80, 85, 90, 101, 103 and 10. 1-0 The filament of a 150 W incandescent lamp is 5 cm long and has a diameter of 0.5 mm. The heat flux on the surface of the filament,
More informationPhysics Lecture 13
Physics 113 Jonathan Dowling Physics 113 Lecture 13 EXAM I: REVIEW A few concepts: electric force, field and potential Gravitational Force What is the force on a mass produced by other masses? Kepler s
More informationSimplified Collector Performance Model
Simplified Collector Performance Model Prediction of the thermal output of various solar collectors: The quantity of thermal energy produced by any solar collector can be described by the energy balance
More informationClassical Mechanics. Luis Anchordoqui
1 Rigid Body Motion Inertia Tensor Rotational Kinetic Energy Principal Axes of Rotation Steiner s Theorem Euler s Equations for a Rigid Body Eulerian Angles Review of Fundamental Equations 2 Rigid body
More informationPC4262 Remote Sensing Scattering and Absorption
PC46 Remote Sensing Scattering and Absorption Dr. S. C. Liew, Jan 003 crslsc@nus.edu.sg Scattering by a single particle I(θ, φ) dφ dω F γ A parallel beam of light with a flux density F along the incident
More informationFundametals of Rendering - Radiometry / Photometry
Fundametals of Rendering - Radiometry / Photometry Physically Based Rendering by Pharr & Humphreys Chapter 5: Color and Radiometry Chapter 6: Camera Models - we won t cover this in class Realistic Rendering
More informationThermal conversion of solar radiation. c =
Thermal conversion of solar radiation The conversion of solar radiation into thermal energy happens in nature by absorption in earth surface, planetary ocean and vegetation Solar collectors are utilized
More informationChapter 28. Gauss s Law
Chapter 28. Gauss s Law Using Gauss s law, we can deduce electric fields, particularly those with a high degree of symmetry, simply from the shape of the charge distribution. The nearly spherical shape
More informationInfrared Earth Horizon Sensors for CubeSat Attitude Determination
Infrared Earth Horizon Sensors for CubeSat Attitude Determination Tam Nguyen Department of Aeronautics and Astronautics Massachusetts Institute of Technology Outline Background and objectives Nadir vector
More informationInfrared Earth Horizon Sensors for CubeSat Attitude Determination
Infrared Earth Horizon Sensors for CubeSat Attitude Determination Tam Nguyen Department of Aeronautics and Astronautics Massachusetts Institute of Technology Outline Background and objectives Nadir vector
More informationDIRECT RADIOMETRIC TECHNIQUES
EMISSIVITY AND OTHER INFRARED-OPTICAL PROPERTIES MEASUREMENT METHODS DIRECT RADIOMETRIC TECHNIQUES Measuring principle The principle of direct radiometric techniques is shown schematically in the figure
More informationTo remain at 0 K heat absorbed by the medium must be removed in the amount of. dq dx = q(l) q(0) dx. Q = [1 2E 3 (τ L )] σ(t T 4 2 ).
294 RADIATIVE HEAT TRANSFER 13.7 Two infinite, isothermal plates at temperatures T 1 and T 2 are separated by a cold, gray medium of optical thickness τ L = L (no scattering). (a) Calculate the radiative
More informationSEAFLOOR MAPPING MODELLING UNDERWATER PROPAGATION RAY ACOUSTICS
3 Underwater propagation 3. Ray acoustics 3.. Relevant mathematics We first consider a plane wave as depicted in figure. As shown in the figure wave fronts are planes. The arrow perpendicular to the wave
More informationLecture 9: Introduction to Diffraction of Light
Lecture 9: Introduction to Diffraction of Light Lecture aims to explain: 1. Diffraction of waves in everyday life and applications 2. Interference of two one dimensional electromagnetic waves 3. Typical
More informationAdvanced Heat and Mass Transfer by Amir Faghri, Yuwen Zhang, and John R. Howell
Heat Transfer Heat transfer rate by conduction is related to the temperature gradient by Fourier s law. For the one-dimensional heat transfer problem in Fig. 1.8, in which temperature varies in the y-
More informationRelationship to Thermodynamics. Chapter One Section 1.3
Relationship to Thermodynamics Chapter One Section 1.3 Alternative Formulations Alternative Formulations Time Basis: CONSERVATION OF ENERGY (FIRST LAW OF THERMODYNAMICS) An important tool in heat transfer
More informationQ ( q(m, t 0 ) n) S t.
THE HEAT EQUATION The main equations that we will be dealing with are the heat equation, the wave equation, and the potential equation. We use simple physical principles to show how these equations are
More informationE d. h, c o, k are all parameters from quantum physics. We need not worry about their precise definition here.
The actual form of Plank s law is: b db d b 5 e C C2 1 T 1 where: C 1 = 2hc o 2 = 3.7210 8 Wm /m 2 C 2 = hc o /k = 1.3910 mk Where: h, c o, k are all parameters from quantum physics. We need not worry
More informationChapter 2: Heat Conduction. Dr Ali Jawarneh Department of Mechanical Engineering, Hashemite University
Chapter : Heat Conduction Equation Dr Ali Jawarneh Department of Mechanical Engineering, Hashemite University Objectives When you finish studying this chapter, you should be able to: Understand multidimensionality
More informationIntroduction to Infrared Radiation.
Introduction to Infrared Radiation. 1. Starting at the source the Heating Coil. 2. Electrical Issues some basic calculations. 3. The basics of Heat Transfer 4. The Electromagnetic Spectrum 5. Infrared
More information