Heat Transfer RADIATION HEAT TRANSFER FUNDAMENTALS.

Slides:



Advertisements
Similar presentations
RADIO WAVES, MICROWAVES, INFRARED, VISIBLE, ULTRAVIOLET, X-RAYS, GAMMA RAYS HIGH< wavelength LOW.
Advertisements

The Radiance Equation.
Radiation: Overview Radiation - Emission Radiation - Absorption
LECTURE 25 – RADIATION VIEW FACTORS. VIEW FACTORS THE EQUIVALENT FRACTION OF RADIATION FROM ONE SURFACE THAT IS INTERCEPTED BY A SECOND SURFACE ALSO CALLED.
Radiation Heat Transfer
Chapter 12 : Thermal Radiation
Momentum Heat Mass Transfer
Electromagnetic Radiation Electromagnetic Spectrum Radiation Laws Atmospheric Absorption Radiation Terminology.
OC3522Summer 2001 OC Remote Sensing of the Atmosphere and Ocean - Summer 2001 Review of EMR & Radiative Processes Electromagnetic Radiation - remote.
1. 2 Definition 1 – Remote sensing is the acquiring of information about an object or scene without touching it through using electromagnetic energy a.
Radiation: Processes and Properties Basic Principles and Definitions 1.
Radiation Heat Transfer
Light. Photons The photon is the gauge boson of the electromagnetic force. –Massless –Stable –Interacts with charged particles. Photon velocity depends.
Solar Radiation Emission and Absorption
METO 621 LESSON 8. Thermal emission from a surface Let be the emitted energy from a flat surface of temperature T s, within the solid angle d  in the.
Satellites Observations Temperature and albedo. What we need to do How do we get values of temperature and albedo (reflectance) using the instruments.
Radiation Heat Transfer. The third method of heat transfer How does heat energy get from the Sun to the Earth? There are no particles between the Sun.
Light and Electrons October 27, 2014.
Radiation Definitions and laws Heat transfer by conduction and convection required the existence of a material medium, either a solid or a.
Laws of Radiation Heat Transfer P M V Subbarao Associate Professor Mechanical Engineering Department IIT Delhi Macro Description of highly complex Wave.
Radiation: Processes and Properties -Basic Principles and Definitions- Chapter 12 Sections 12.1 through 12.3.
Chapter 18 Bose-Einstein Gases Blackbody Radiation 1.The energy loss of a hot body is attributable to the emission of electromagnetic waves from.
Radiation Heat Transfer
Attenuation by absorption and scattering
Sun path diagrams For practical purposes, instead of using the preceding equations, it is convenient to have the sun’s path plotted on a horizontal plane,
Advanced Heat Transfer - Prof. Dr.-Ing. R. Weber - Winter 2005/ Lecture 1 (Governing Laws) Lecture-1. Governing Laws for Thermal Radiation Contents.
Photon Statistics Blackbody Radiation 1.The energy loss of a hot body is attributable to the emission of electromagnetic waves from the body. 2.The.
Radiation Fundamental Concepts EGR 4345 Heat Transfer.
Radiation Heat Transfer EGR 4345 Heat Transfer. Blackbody Radiation Blackbody – a perfect emitter & absorber of radiation Emits radiation uniformly in.
CHAPTER 12 RADIATION HEAT TRANSFER. Electromagnetic Radiation – electromagnetic waves (brought upon by accelerated charges or changing electric currents)
Chapter 21 RADIATION HEAT TRANSFER Copyright © 2012 The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Fundamentals of Thermal-Fluid.
CSCE 641 Computer Graphics: Reflection Models Jinxiang Chai.
Chapter 5 – Electrons in Atoms text pages
Introduction to Thermal Radiation and Radiation Heat Transfer.
Physics 1202: Lecture 30 Today’s Agenda Announcements: Extra creditsExtra credits –Final-like problems –Team in class HW 9 next FridayHW 9 next Friday.
Introduction to Thermal Radiation
Radiation Heat Transfer
Radiation (Ch 12 YAC) Thermal energy is emitted by matter as a result of vibrational and rotational motion of molecules, atoms and electrons. The energy.
Chapter 12: Fundamentals of Thermal Radiation
NATS 101 Section 13: Lecture 5 Radiation. What causes your hand to feel warm when you place it near the pot? NOT conduction or convection. Why? Therefore,
Vocabulary Review New radiation electromagnetic radiation wavelength
RADIATION HEAT TRANSFER The Nature and Characteristics of Thermal Radiation.
1 Teaching Innovation - Entrepreneurial - Global The Centre for Technology enabled Teaching & Learning D M I E T R, Wardha DTEL DTEL (Department for Technology.
Blackbody. Kirchhoff’s Radiation  Radiated electromagnetic energy is the source of radiated thermal energy. Depends on wavelengthDepends on wavelength.
Remote sensing: the collection of information about an object without being in direct physical contact with the object. the collection of information about.
Damian Luna Yetziel Sandoval – Alberto Gonzales – 80546
Physical Principles of Remote Sensing: Electromagnetic Radiation
The temperature of a lava flow can be estimated by observing its color
G.H PATEL COLLEGE OF ENGINEERING & TECHNOLOGY
AHMEDABAD INSTITUTE OF TECHNOLOGY
Basic Science in Remote Sensing
RADIATION AND COMBUSTION PHENOMENA
Chapter 6 Electronic Structure of Atoms
Energy Flow Concept Image Sensor Energy Source
ERT 216 HEAT & MASS TRANSFER
Chapter 12 FUNDAMENTALS OF THERMAL RADIATION
REMOTE SENSING Fundamentals of Remote Sensing
Radiation Process and Properties
Radiation Thermal energy emitted by matter as a result of vibrational and rotational movements of molecules, atoms and electrons. The energy is transported.
Radiation  = 1 for blackbody (emissivity) Qr = T4
Black Body Radiation Mr. Sonaji V. Gayakwad Asst. professor
Remote Sensing Remote sensing includes techniques to derive information from a site at a known distance from the sensor.1 Remote sensing is the science.
Quantum Physics Interaction of matter with energy
Section 1: Light and Quantized Energy
Introduction and Basic Concepts
Radiation Thermal energy emitted by matter as a result of vibrational and rotational movements of molecules, atoms and electrons. The energy is transported.
17.2 – Heating the atmosphere – Part I
Elementary Quantum Mechanics
Radiation Heat Transfer
Section 1: Light and Quantized Energy
Presentation transcript:

Heat Transfer RADIATION HEAT TRANSFER FUNDAMENTALS

BASIC RADIATION PHYSICS RADIATION IS A FORM OF ELECTROMAGNETIC ENERGY TRANSFER MAY BE WAVE TRANSFER MAY BE PHOTONS OR QUANTA SURFACE OR VOLUMETRIC PHENOMENON CAN BE GENERATED FROM A SOLID OR LIQUID SURFACE CAN BE GENERATED IN A GAS

BASIC RADIATION PHYSICS PRIMARY RELATIONSHIPS ARE WAVELENGTH AND FREQUENCY WHERE Co IS THE SPEED OF LIGHT IN A VACUUM ENERGY OF A PHOTON IS BASED ON PLANCK’S CONSTANT.

THERMAL RADIATION OVERALL ELECTROMAGNETIC SPECTRUM

THERMAL RADIATION DEFINED OVER A RANGE OF THE ELECTROMAGNETIC SPECTRUM FROM λ = 0.1 μm TO λ = 100 μm VISIBLE IS A SECTION OF THE THERMAL SPECTRUM sers.com/media/upl oad/image/EMwave( 2).jpg

THE ELECTROMAGNETIC SPECTRUM space.stsci.edu/news/archive/2005/03/graphics/em_chart.gif

WAVELENGTH RESONANCE MICROWAVE ENERGY IS USED FOR COOKING HAS A WAVELENGTH RANGE OF 102 < λ < 105 IS ABSORBED WITH A HIGH EFFICIENCY BY WATER MOLECULES IN THIS RANGE

RADIATION DIRECTIONALITY RADIATION IS NORMALLY EMITTED IN ALL DIRECTIONS FROM A SOURCE, THOUGH IT MAY HAVE A PREFERENTIAL DIRECTION RADIATION ALSO IS EMITTED IN PREFERRED WAVELENGTHS, PRODUCING SPECTRA THAT CAN BE USED TO IDENTIFY MATERIALS

BLACKBODY RADIATION THE BLACKBODY IS THE IDEAL EMITTER THE INTENSITY OF BLACKBODY RADIATION AS A FUNCTION OF WAVELENGTH IS DEFINED BY PLANCK’S LAW:

MAXIMUM RADIATION INTENSITY THE MAXIMUM INTENSITY AT ANY WAVELENGTH IS OBTAINED BY DIFFERENTIATING PLANCK’S LAW WITH RESPECT TO λ AND CALCULATING THE ROOT FOR THE MAXIMUM THIS IS WIEN’S DISPLACEMENT LAW THIS RELATIONSHIP CAN BE USED TO CALCULATE THE TEMPERATURE OF STARS USING THE HIGHEST INTENSITY WAVELENGTH

TOTAL BLACKBODY EMISSIVE POWER INTEGRATION OF PLANCK’S LAW OVER THE RANGE OF λ, YIELDS THE TOTAL BLACKBODY EMISSIVE POWER FOR A GIVEN TEMPERATURE

EMISSION BY WAVELENGTH INTENSITY FOR DIFFUSE BLACKBODY RADIATION BAND EMISSION OVER A RANGE OF WAVELENGTHS CAN BE CALCULATED WITH PLANCK’S LAW IS SUMMARIZED IN TABLE 12-2 AS A FUNCTION OF λT

EMISSION BY WAVELENGTH RANGE

BLACKBODY EMISSION BY λ THE RELATIONSHIP FOR THE FRACTION OF EMISSIVE ENERGY FOR A BLACKBODY WITHIN A SPECIFIC RANGE OF WAVELENGTHS IS:

SOLID ANGLES EMISSION IN A PARTICULAR DIRECTION FROM A SOURCE, dA, IS EVALUATED RELATIVE TO THE ZENITH θ AND AZIMUTH φ ANGLES THE SOLID ANGLE, ω, IS DEFINED BY THE SECTION, dS, SWEPT OUT ON A HEMISPHERE AT A SPECIFIC RADIUS, r.

DIFFERENTIAL SOLID ANGLE DEFINED IN TERMS OF THE ANGLES AS:

DIFFERENTIAL EMISSIVITY THE SOLID ANGLE HAS UNITS OF STERADIANS THE PROJECTION OF dA AT A DISTANCE r FROM THE SOURCE AND ON A ZENITH OF φ IS A COSINE RELATIONSHIP

RADIATION INTENSITY THE BLACKBODY, DIFFUSE EMITTED INTENSITY IS DEFINED IN TERMS OF THE SOLID ANGLE IRRADIATION, INCIDENT RADIATION, SEE FIGURE IS A FUNCTION OF WAVELENGTH AND THE INCIDENT ANGLE: OVER THE ENTIRE SPECTRUM OF WAVELENGTHS:

RADIATION INTENSITY IF THE INCOMING RADIATION IS DIFFUSE, THEN IT IS INDEPENDENT OF θ AND φ, SO THE EQUATIONS BECOME:

RADIOSITY REPRESENTS ALL THE RADIANT ENERGY LEAVING A SURFACE (SEE FIGURE 12-21) INCLUDES REFLECTED AND EMITTED ENERGY CAN BE EXPRESSED IN TERMS OF WAVELENGTH AND ANGLES AS: TOTAL RADIOSITY CAN THEN BE EXPRESSED AS:

DIFFUSE SURFACE IF THE SURFACE IS A DIFFUSE REFLECTOR AND A DIFFUSE EMITTER, THEN RADIOSITY IS INDEPENDENT OF θ AND φ, SO THE EQUATIONS BECOME (SEE CHAP 13)