Save Money and Energy by Detecting Heat Losses
Transcript of Save Money and Energy by Detecting Heat Losses
Quantitative ThermographyTemperature and Tantrums
Infrared – What is it?
How is it emitted?
E = hvFrequency of radiation, sometimes written as f giving expression E=hf.
Quantum energyof a photon.
H – Planck’s constant = 6.626 x 10 Joule-sec = 4.136 x 10 eV-s-34 -15
The Weird World of Infrared
What is this?
Emitted (Tg)
Reflected (Tr)
Transmitted (Tt)
The Weird World of Infrared – Part 2
AbsorbedBackground (Tb)
Gas “Cloud”
Radiation Laws
Planck’s Law The formula describing the spectral radiation of a perfect blackbody as a function of its
temperature and the wavelength of the emitted radiationWλb = 2π h c2 x 10-6 [ W/m2(µm)]
λ5 (ehc/λkT – 1)h-=Planck’s constantk=Boltzman’s contstant
Stefan-Boltzmann’s Law The formula indicates the total radiation at ALL wavelengths from a perfect blackbody
W[TOTAL] = 5.67 x 10-8 T4 [W/m2]
Convection
For horizontal pipes
WConvection = 1.35 x (Ts – Ta)0.25 / dop [ W/m2]
Ts = Absolute temperature of heat emitting surfaceTa = Absolute temperature of airdop = Outside diameter of pipe/insulation
Camera Selection
Total loss in horizontal pipework
Q = length π dop (WConvection + WRadiation)
= length x π dop x (1.35 x (Ts – Ta)0.25 / dop + 5.67 x 10-8 T4)
Examples
Examples
Examples
Quiz – How much per year?
£10,811 £33,000pa for 25mph wind
Quiz – How much
£21,500 £73,000pa for 25mph wind
Thank you for ListeningAny Questions?