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Understanding Heat Transfer by Radiation: Solar Energy and Electromagnetic Waves, Lecture notes of Thermodynamics

ThermodynamicsHeat TransferElectromagnetism

The concept of heat transfer by radiation, focusing on solar energy and the electromagnetic spectrum. It discusses how radiation is a form of energy transfer through electromagnetic waves, and how objects emit and absorb radiation. The document also includes a data table and graph for temperature readings, as well as examples and analysis questions.

What you will learn

  • How do objects emit and absorb radiation?
  • How does heat transfer by radiation differ from other forms of heat transfer?
  • What is the role of electromagnetic waves in heat transfer by radiation?

Typology: Lecture notes

2021/2022

Uploaded on 09/12/2022

jesus33
jesus33 🇺🇸

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Download Understanding Heat Transfer by Radiation: Solar Energy and Electromagnetic Waves and more Lecture notes Thermodynamics in PDF only on Docsity! 1 Student Sheet 1 All of the energy from the Sun that reaches the Earth arrives as solar radiation, part of a large collection of energy called the electromagnetic radiation spectrum. Solar radiation includes visible light, ultraviolet light, infrared, radio waves, X-rays, and gamma rays. The Electromagnetic Spectrum Radiation is one way to transfer heat. To “radiate” means to send out or spread from a central location. Whether it is light, sound, waves, rays, flower petals, wheel spokes or pain, if something radiates then it spreads outward from a starting point. You experience radiation personally whenever you get out of the shower, soaking wet, in the dead of winter and enjoy the warmth of the heat lamp in your bathroom. The heat lamp beams out heat to you and keeps you warm through radiation. With radiation, electromagnetic waves carry the energy. Electromagnetic radiation comes from accelerating electric charges. On a molecular level, that’s what happens as objects warm up — their molecules vibrate harder and harder, causing acceleration of electric charges. 2 Student Sheet 2 Heat energy transferred through radiation is as familiar as the light of day; in fact, it is the light of day. The Sun is a huge thermal reactor about 93 million miles away. In heat transfer by radiation, energy is carried by electromagnetic waves from a starting point to the space surrounding it and does not involve contact with matter. The other forms of heat transfer cannot produce any of the energy that arrives to Earth through the vacuum of space. The Sun’s energy gets to the Earth through radiation, which you can prove just by standing outside and letting the sun’s rays warm your face on a sunny day. Every object around you is continually radiating, unless its temperature is at absolute zero, at which point its molecules completely stop moving. A scoop of ice cream, for example, radiates heat, but that radiation isn’t visible as light because it’s in the infrared part of the spectrum. However, it is visible to infrared scopes, as you’ve probably seen in movies or on television. Objects emit radiation when high energy electrons in a high atomic level fall down to lower energy levels. The energy lost is emitted as light or electromagnetic radiation. Energy that is absorbed by an atom causes its electrons to "jump" up to higher energy levels. All objects absorb and emit radiation. When the absorption of energy balances the emission of energy, the temperature of an object stays constant. If the absorption of energy is greater than the emission of energy, the temperature of an object rises. If the absorption of energy is less than the emission of energy, the temperature of an object falls.
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