Heat Flashcards
temperature
a measure of how hot or cold something is
unit: kelvin (K)
thermometric property
any physical property that changes measurably with temperature. e.g. length of a column of liquid, electrical resistance, emf of a thermocouple, colour, volume of gas at constant pressure, pressure of gas at constant volume
heat capacity
heat energy needed to change the temperature of an object by 1K
Q= CΔθ
unit for heat capacity
joule per kelvin (JK^-1)
specific heat capacity
heat energy needed to change the temperature of 1kg of that substance by IK
unit = Jkg^-1K^-1
Q=mcΔθ
latent heat
heat energy needed to change the state of a substance without a change in temperature
unit = joule (J)
specific latent heat
heat energy needed to change the state of 1kg of a substance without a change in temperature
unit = joule per kilogram (Jkg^-1)
specific latent heat of fusion
heat needed to change 1kg of a substance from a solid to a liquid
specific latent heat of vaporisation
heat needed to change 1kg of a substance from a liquid to a gas
conduction
transfer of heat through a substance by molecules vibrating without overall motion of the substance e.g. metals
convection
transfer of heat through a liquid/gas by means of circulating currents (convection currents) e.g. sea breezes/radiators
radiation
transfer of heat from one place to another in the form of electromagnetic waves e.g. hot objects, sun, human body
U-value
amount of heat energy conducted per second through 1m^2 of that structure when a temperature difference of 1 deg. celsius is maintained between its ends
Tog value
The tog is a measure of thermal insulance of a unit area, also known as thermal resistance. It is commonly used in the textile industry and often seen quoted on, for example, duvets and carpet underlay. A tog is 0.1⋅m2⋅K/W. In other words, the thermal resistance in togs is equal to ten times the temperature difference (in °C) between the two surfaces of a material, when the flow of heat is equal to one watt per square metre.
solar constant/ solar irradiance
average amount of the suns energy falling per second perpendicularly on 1m^2 of the earth’s atmosphere
about 1.35kWm^-2
= power/area
or energy per sec/ area