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I am trying to model the cooling of an object (for example, a sheet of glass) placed outside at night. At the moment I am only considering heat loss by radiation.
I know that the net radiation from the object will be:
Rnet = Robj - Rsky
where:
Rnet = the net radiation from the object
Robj = the total thermal radiation from the object
Rsky = the thermal downwelling radiation from the sky
I have come across a formula which does the above, but also takes into consideration the absorptivity of the sheet of glass at the 8-14μm wavelength (I have only considered emissivity of the glass in this wavelength as I'm only concerned with thermal radiation heat loss to the sky).
The formula is:
Rnet = A((εobj2/αobj2)σTobj4 - εskyσTamb4)
where:
εobj = the emissivity of the object at 8-14μm
αobj = the absorptivity of the object at 8-14μm
εsky = the emissivity of the sky
Tobj = the temperature of the object
Tamb4 = the ambient air temperature
A = the area of the object
What I would like to know is where does the εobj2/αobj2 bit come from? I know if I wasn't considering absorptivity then it would just be εobj, but why are εobj and αobj now squared? I have since lost where I saw it, and I'm pretty sure there wasn't an explanation there anyway. I have searched all over for a derivation of it but have had no luck.
Can anyone help?
I know that the net radiation from the object will be:
Rnet = Robj - Rsky
where:
Rnet = the net radiation from the object
Robj = the total thermal radiation from the object
Rsky = the thermal downwelling radiation from the sky
I have come across a formula which does the above, but also takes into consideration the absorptivity of the sheet of glass at the 8-14μm wavelength (I have only considered emissivity of the glass in this wavelength as I'm only concerned with thermal radiation heat loss to the sky).
The formula is:
Rnet = A((εobj2/αobj2)σTobj4 - εskyσTamb4)
where:
εobj = the emissivity of the object at 8-14μm
αobj = the absorptivity of the object at 8-14μm
εsky = the emissivity of the sky
Tobj = the temperature of the object
Tamb4 = the ambient air temperature
A = the area of the object
What I would like to know is where does the εobj2/αobj2 bit come from? I know if I wasn't considering absorptivity then it would just be εobj, but why are εobj and αobj now squared? I have since lost where I saw it, and I'm pretty sure there wasn't an explanation there anyway. I have searched all over for a derivation of it but have had no luck.
Can anyone help?