Chapter 16 Heat Transfer Flashcards
Conduction
The transfer of heat energy by molecular and electron collisions within a substance (especially in a solid).
Convection
The transfer of heat energy in a gas or liquid by means of currents in the heated fluid. The fluid moves, carrying energy with it.
Radiation
The transfer of energy by means of electromagnetic waves.
Terrestrial radiation
The radiation emitted by the Earth to outer space.
Newton’s law of cooling
The rate of loss of heat from an object is proportional to the temperature difference between the object and its surrounds.
Greenhouse effect
Warming of the lower atmosphere by short-wavelength radiation from the Sun that penetrates the atmosphere, is absorbed by the Earth, and is reradiated at longer wavelengths that cannot easily escape Earth’s atmosphere.
Solar constant
1400 J/m^2 received from the Sun each second at the top of Earth’s atmosphere on an area perpendicular to the Sun’s rays; expressed in terms of power, 1.4 kW/m^2
Solar power
Energy per unit time derived from the Sun.