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Radiation to Emission

Radiation to Emission. P M V Subbarao Associate Professor Mechanical Engineering Department IIT Delhi. Development of Design Ideas …. Radiation Heat Flux. The spectral heat flux associated with emission into hypothetical hemisphere above dA 1.

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Radiation to Emission

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  1. Radiation to Emission P M V Subbarao Associate Professor Mechanical Engineering Department IIT Delhi Development of Design Ideas …..

  2. Radiation Heat Flux The spectral heat flux associated with emission into hypothetical hemisphere above dA1 Total (hemispherical) heat flux associated with dA1

  3. Relation to Emission Spectral emissive power is defined as the rate at which radiation of wavelength l is emitted in all directions form a surface per unit wavelength dl about l. The total hemispherical emissive power: The term emissive power implies emission in all directions, the adjective hemispherical is redundant. E is called total emissive power.

  4. Diffuse Emitter • The directional distribution of surface emission varies according to the nature of the surface. • Diffuse emitter is a surface for which the intensity of emitted radiation is independent of direction.

  5. Similarly If this emission incidents on another surface, then it is called as incident radiation or irradiation.

  6. Irradiation • The intensity of radiation is related to radiation flux incident on a surface called irradiation. • Irradiation encompasses radiation incident from all directions. • The spectral irradiation is defined as rate at which radiation of wavelength l is incident on a surface, per unit area of the surface and per unit wavelength interval dl about l. Total Irradiation:

  7. If the incident radiation is diffuse

  8. Blackbody Radiation • The characteristics of a blackbody are : • It is a perfect emitter. • It is a diffuse emitter • At any prescribed temperature it has the highest monochromatic emissive power at all wave lengths. • A blackbody absorbs all the incident energy and there for. • It is non reflective body. • It is opaque.

  9. Isothermal Pinhole Cavity Black body inside A Cavity Synthesis of A Black Body

  10. Gl,r Gl Gl,a Gl,t Response of A General Surface to Irradiation • Consider a semi-transparent sheet that receives incident radiant energy flux, also known as irradiation, G . • Let Glrepresent the irradiation in the waveband l to l + dl. • Part of it may be absorbed, part of it reflected at the surface, and the rest transmitted through the sheet. • Define monochromatic properties.

  11. Monochromatic Absorptivity : Total (hemispherical) Absorptivity : Monochromatic reflectivity : Total reflectivity : Monochromatic Transmissivity : Total Transmissivity :

  12. Conservation of Irradiation The total Irradiation =

  13. How to Make Things to Look Beautiful

  14. How to Make Things to Look Beautiful

  15. Radiosity • The radiosity of a surface is the rate at which radiation energy leaves a surface per unit area. Spectral Radiosity: Total Radiosity

  16. Radiative Heat Transfer Consider the heat transfer between two surfaces, as shown in Figure. What is the rate of heat transfer into Surface B? To find this, we will first look at the emission from A to B. Surface A emits radiation as described in This radiation is emitted in all directions, and only a fraction of it will actually strike Surface B. This fraction is called the shape factor, F.

  17. The amount of radiation striking Surface B is therefore: The only portion of the incident radiation contributing to heating Surface B is the absorbed portion, given by the absorptivity αB: Above equation is the amount of radiation gained by Surface B from Surface A. To find the net heat transfer rate at B, we must now subtract the amount of radiation emitted by B:

  18. The net radiative heat transfer (gain) rate at Surface B is

  19. Shape Factors • Shape factor, F, is a geometrical factor which is determined by the shapes and relative locations of two surfaces. • Figure illustrates this for a simple case of cylindrical source and planar surface. • Both the cylinder and the plate are infinite in length. • In this case, it is easy to see that the shape factor is reduced as the distance between the source and plane increases. • The shape factor for this simple geometry is simply the cone angle (θ) divided by 2π

  20. Shape factors for other simple geometries can be calculated using basic theory of geometry. • For more complicated geometries, the following two rules must be applied to find shape factors based on simple geometries. • The first is the summation rule. • This rule says that the shape factor from a surface (1) to another (2) can be expressed as a sum of the shape factors from (1) to (2a), and (1) to (2b). • The second rule is the reciprocity rule, which relates the shape factors from (1) to (2) and that from (2) to (1) as follows:

  21. Thus, if the shape factor from (1) to (2) is known, then the shape factor from (2) to (1) can be found by: If surface (2) totally encloses the surface 1:

  22. Geometrical Concepts in Radiation Heat Transfer

  23. Human Shape Factors Wherever artificial climates are created for human occupation, the aim of the design is that individuals experience thermal comfort in the environment. Among other factors thermal comfort depends on mean radiant temperature.

  24. Flame to Furnace Wall Shape Factors

  25. Radiative Heat Exchange between Two Differential Area Elements • The elements dAi and dAj are isothermal at temperatures Ti and Tj respectively. • The normals of these elements are at angles qi and qj respectively to their common normal. • The total energy per unit time leaving dAi and incident upon dA2 is:

  26. The monochromatic energy per unit time leaving dAi and incident on dA2 is

  27. The total energy per unit time leaving dAi and incident upon dA2 is: The monochromatic energy per unit time leaving dAi and incident on dA2 is:

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