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3 - Radiative Heat Transfer Analysis

Published online by Cambridge University Press:  19 June 2020

Eric A. Silk
Affiliation:
University of Maryland, College Park
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Summary

In Chapter 1 the Stefan‒Boltzmann Law (shown in equation 3.1) was presented as the relation used to determine the amount of radiative thermal energy emitted from a surface.

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Publisher: Cambridge University Press
Print publication year: 2020

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References

Serway, R.A., 1986, Physics for Scientists and Engineers, 2nd edn, Saunders College PublishingGoogle Scholar
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Siegel, R., and Howell, J., 2002, Thermal Radiation Heat Transfer, 4th edn, Taylor & Francis, New York, NYGoogle Scholar
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Beckman, W.A., 1968, “Temperature Uncertainties in Systems with Combined Radiation and Conduction Heat Transfer,” Proceedings of ASME Annual Aviation and Space Conference, Beverly Hills, CAGoogle Scholar
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  • Radiative Heat Transfer Analysis
  • Eric A. Silk, University of Maryland, College Park
  • Book: Introduction to Spacecraft Thermal Design
  • Online publication: 19 June 2020
  • Chapter DOI: https://doi.org/10.1017/9781108149914.003
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  • Radiative Heat Transfer Analysis
  • Eric A. Silk, University of Maryland, College Park
  • Book: Introduction to Spacecraft Thermal Design
  • Online publication: 19 June 2020
  • Chapter DOI: https://doi.org/10.1017/9781108149914.003
Available formats
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Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

  • Radiative Heat Transfer Analysis
  • Eric A. Silk, University of Maryland, College Park
  • Book: Introduction to Spacecraft Thermal Design
  • Online publication: 19 June 2020
  • Chapter DOI: https://doi.org/10.1017/9781108149914.003
Available formats
×