1. Introduction to Thermal Radiation and Radiation Heat Transfer

2. Thermal Radiation Occurs in solids, liquids, and gases Occurs at the speed of light Has no attenuation in a vacuum Can occur between two bodies with a colder medium in between Occurs in combination with conduction and convection, and significant where large temperature differences occur Applications: Furnace with boiler tubes, radiant dryers, oven baking, designing heaters for manufacturing, estimating heat gains through windows, infrared cameras, metal cooling during manufacturing, Greenhouse effect, thermos design, among others.

3. Background Electromagnetic radiation – energy emitted due to changes in electronic configurations of atoms or molecules where =wavelength (usually in  m), =frequency In a vacuum c=c o =2.998x10 8 m/s Other media: c=c o /n where n=index of refraction

4. Background, cont. Radiation – photons or waves? Max Planck (1900): each photon has an energy of h=Planck ’ s constant=6.625 x 10 -34 Js Shorter wavelengths have higher energy

5. Radiation Spectrum

6. Types of Radiation Two categories –Volumetric phenomenon – radiation emitted or absorbed throughout gases, transparent solids, some fluids –Surface phenomenon – radiation to/from solid or liquid surface Thermal radiation – emitted by all substances above absolute zero Includes visible & infrared radiation & some UV radiation.

7. Radiation Properties Magnitude of radiation varies with wavelength – it ’ s spectral. –The wavelength of the radiation is a major factor in what its effects will be. –Earth/sun example Radiation is made up of a continuous, nonuniform distribution of monochromatic (single-wavelength) components. Magnitude & spectral distribution (how the radiation varies with wavelength) vary with temp & type of emitting surface.

8. Emission Variation with Wavelength

9. Blackbody Radiation Blackbody – a perfect emitter & absorber of radiation; it absorbs all incident radiation, and no surface can emit more for a given temperature and wavelength Emits radiation uniformly in all directions – no directional distribution – it ’ s diffuse Example of a blackbody: large cavity with a small hole

10. Stefan-Boltzmann Law Joseph Stefan (1879) – total radiation emission per unit time & area over all wavelengths and in all directions:  =Stefan-Boltzmann constant =5.67 x10 -8 W/m 2 K 4 Tmust be in absolute scale.

11. Planck ’ s Distribution Law Sometimes we care about the radiation in a certain wavelength interval For a surface in a vacuum or gas Integrating this function over all gives us

12. Radiation Distribution Radiation is a continuous function of wavelength Magnitude increases with temp. At higher temps, more radiation is at shorter wavelengths. Solar radiation peak is in the visible range.

13. Wien ’ s Displacement Law Wavelength of radiation with the largest magnitude can be found for different temps using Wien ’ s Displacement Law: Note that color is a function of absorption & reflection, not emission.

14. What is your favorite wavelength?

15. More Radiation Properties Directional distribution – a surface doesn ’ t emit the same in all directions. Hemispherical – refers to all directions

16. Emissive Power E: amount of radiation emitted per unit area Spectral hemispherical emissive power E (often leave out the word “ hemispherical ” ) W/m 2 –Rate of emission per unit area of radiation of a given wavelength in all directions per unit wavelength interval Total (hemisperical) emissive power E (W/m 2 ) –Rate of emission per unit area of radiation of all wavelengths and in all directions; this is

17. Diffuse emitters Diffuse emitter: intensity is the same in all directions

18. Irradiation Irradiation: radiation incident on (hitting) a surface per unit area

19. Radiosity Radiosity: all radiation leaving a surface per unit area, both emitted and reflected

23. Emmisivity and Kirchoff ’ s law  = E/E b  irchoffs’ Law 

24.  T1T1 T2T2 T3T3 Energy e Ideal EmitterSchematic T 3 > T 2 > T 1

25. In general: Opaque material:  = absorptivity  = reflectivity  = transmissivity

26. Mechanism of Radiation Heat Transfer Thermal energy of hot source ( furnace wall at T1) is converted into radiant energy. These waves travel through the intervening space in straight lines and strike a cold object at T2 such as a furnace tube The electromagnetic waves that strike the body are absorbed and converted back to thermal energy.

27. Black Body and Gray Body Black Body –absorptivity =  –emissivity =  –ideal emissive power = E b Gray Body –absorptivity < 1 –emissivity < 1 (independent of wavelength) –emissive power<1

29. Radiation of a small object from surrounding A1A1 T2T2 T1T1 T 2 > T 1

30. Combined radiation and convection heat transfer

31. View factor View Factor: F ij = fraction of radiation from surface i intercepted by surface j. 1 2

32. Summation rule (View factor)

33. Reciprocity rule (View factor)

34. Superposition rule

35. Symmetry rule

36. Radiation heat transfer between black surfaces

37. (surfaces forming an enclosure)

38. Net radiation from heat transfer to or from a surface

39. Electrical analogy Surface resistance

40. Net Radiation Transfer between two surfaces space resistance

41. Radiation heat transfer in two- surface enclosures

42. Consider the radiation heat transfer between two infinite parallel plates 1 2 1

47. Application:Radiation shield Highly reflective thin plate to reduce radiation heat transfer between two surfaces

50. Radiation effect on temperature measurement