Linked from

The 54 pages that link to Thermal radiation, each with the reason it gives.

• Greenhouse effectNarrower topic: Earth’s surface and atmosphere exchange energy through this radiation.

• Black-body radiationNarrower topic: Black-body radiation is the ideal limiting case of thermal radiation.

• Thermal insulationNarrower topic: Reflective insulation reduces radiative heat exchange across gaps.

• Planck's lawNarrower topic: Planck's law quantitatively describes the ideal equilibrium case of thermal radiation.

• Interstellar dustNarrower topic: Absorbed starlight heats grains, which then radiate energy primarily in the infrared.

• Stefan–Boltzmann lawNarrower topic: The law describes the total power carried by this radiation from a black body.

• EmissivityNarrower topic: Emissivity quantifies how strongly a surface emits this radiation relative to an ideal reference.

• Incandescent light bulbNarrower topic: Visible glow and waste heat are parts of the bulb’s broader thermal-radiation output.

• Kirchhoff's law of thermal radiationNarrower topic: The law concerns the emission and absorption of this radiation.

• Radiative coolingNarrower topic: Radiative cooling is heat loss through this broader form of energy transfer.

• Radiative equilibriumNarrower topic: The emission side of radiative equilibrium is thermal radiation for many physical systems.

• LuminescenceNarrower topic: It is the broader thermal process against which nonthermal luminescence is distinguished.

• Gas mantleNarrower topic: The mantle’s temperature determines the spectrum and intensity of its emitted light.