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This chapter explores the fundamental concepts of radiation heat transfer, including the interaction of radiation with materials, the key properties such as emissivity, absorptivity, and reflectivity, and essential laws such as the Stefan–Boltzmann law. It also discusses practical applications, view factors, and methods for calculating radiative exchange between surfaces. The chapter concludes by highlighting the importance of radiation shields in thermal management.
References
Module IV_ Radiation Heat Transfer.pdfClass Notes
Memorization
What we have learnt
Final Test
Revision Tests
Term: Emissivity (ε)
Definition: The ratio of radiation emitted by a surface to that by a blackbody at the same temperature.
Term: Stefan–Boltzmann Law
Definition: A law describing the power radiated from a blackbody in terms of its temperature, represented as Eb = σT4.
Term: View Factors (Configuration Factors)
Definition: The fraction of radiation leaving one surface that strikes a second surface, crucial for calculating radiation exchange.
Term: Blackbody
Definition: An ideal emitter and absorber of radiation with emissivity equal to 1.
Term: Radiosity
Definition: The total energy leaving a surface, which includes both emitted and reflected energy.