6. Radiation Flashcards
What is the equation for the amount of heat emitted from a black body?
q = sigma T^4 sigma = 5.67x10^-8
What is a black body?
A body which absorbs all incident light and emits the most given its temperature
What is irradiation (G)
G = total rate at which radiation arrives per unit area G = ( α + tau +ρ) G α = absorbed, tau = transmitted ρ= reflected
What is radiosity (J)
Total rate at which radiation leaves per unit area
J = εσT^4 + ρG
J = emitted + reflected
What is the effective resistance to emission/absorption?
1-ε/(εA)
What is the effective resistance to heat travelling from the surface of 1 to the surface of 2?
1/(A1 * F_12)
How do you calculate the proportion of heat leaving one body which reaches another? (F12)
F12 = A2/A1
What is a view factor (F_12)
Fraction of energy leaving surface 1 that reaches surface 2
What is the view factor for a flat surface
0
What is the view factor for a concave inner shell
1
What is the reciprosity relationship
If T1 = T2, then F_12A1 = F_21A2
What is Kirchoff’s Law
If T1 = T2, then epsilon = alpha (emitted = absorbed)
What are the two types of scattering
Rayleigh and Mei scattering
What molecules absorb infrared radiation from the earth best (greenhouse effect)
CO2, H2O, CH4 (methane), Chlorofluorocarbons (CFCs)
How does the Greenhouse effect work
Short wavelength (high energy) radiation from the sun, penetrates the atmosphere and is absorbed on the surface
Earth warms and transmits long wavelength infrared radiation back
This infrared radiation is absorbed by certain molecules instead of leaving the atmosphere