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Modeling the Heat Gain of a Window With an Interior Shade ... - inive

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Proceedings <strong>of</strong> Clima 2007 WellBeing Indoors<br />

The incident radiation on <strong>the</strong> inside <strong>of</strong> <strong>the</strong> glass is diffuse radiation reflected from <strong>the</strong> shade.<br />

Optical properties for diffuse radiation for <strong>the</strong> glass c<strong>an</strong> be determined for isotropic radiation by<br />

integration over all <strong>an</strong>gles <strong>of</strong> incidence. This was done using glass properties from a<br />

m<strong>an</strong>ufacturer <strong>an</strong>d shown in <strong>the</strong> next section <strong>of</strong> this report.<br />

Similarly, <strong>the</strong> short wave beam radiation fraction absorbed by <strong>the</strong> glass, Abs bg , is:<br />

Abs bg<br />

∞<br />

n 1 n<br />

τ gb α gd ρss<br />

= α gb + τ gb α gd ∑ [ ρ<br />

+<br />

ss ρ gd ] = α gb +<br />

Eq[5]<br />

n = 0<br />

1 − ρ ss ρ gd<br />

where variables are as defined before <strong>an</strong>d α gb = beam absorpt<strong>an</strong>ce <strong>of</strong> <strong>the</strong> glass (a function <strong>of</strong><br />

incidence <strong>an</strong>gle, θ), α gd = diffuse absorpt<strong>an</strong>ce <strong>of</strong> glass. Equations 4 <strong>an</strong>d 5 also apply for diffuse<br />

radiation Abs dss <strong>an</strong>d Abs dg , but τ gb is replaced with τ gd <strong>an</strong>d α gb is replaced with α gd (see footnote<br />

7).<br />

Glass<br />

<strong>Shade</strong><br />

P τ gb ρ ss 2 ρ gd<br />

2<br />

Abs=ρ ss 2 τ gs ρ gd 2 α ss<br />

τ gb ρ ss<br />

2<br />

ρ gd τ gd ρ ss<br />

2<br />

τ gb ρ gd<br />

2<br />

Abs= ρ ss 2 τ gb ρ g60 α g60<br />

ρ ss<br />

2<br />

τ gb ρ gd<br />

P τ sb ρ ss ρ gd<br />

Abs=ρ ss τ gb ρ gδ α ss<br />

τ gb ρ ss τ gd<br />

ρ ss τ gb ρ gd<br />

Abs= ρ ss τ gb α gd<br />

ρ ss τ gb<br />

P τ gb<br />

Abs=τ gb α ss<br />

ρ gb<br />

τ gb<br />

Abs=α gb<br />

Figure 1. Short wave energy flows.<br />

We c<strong>an</strong> now do a short wave energy bal<strong>an</strong>ce:<br />

[ cos θAbs<br />

G cd Abs ]<br />

& 3<br />

Q gs = G cnb bg +<br />

dg<br />

Eq[6]<br />

& = [ cos θ Abs<br />

Abs ] Eq[7]<br />

Q ss G cnb<br />

bss + G cd<br />

3 We assume a uniform diffuse short wave field. This is accurate except for <strong>the</strong> lower floors where <strong>the</strong> diffuse<br />

radiation is a mix <strong>of</strong> diffuse sky radiation <strong>an</strong>d ground reflected radiation. We have ignored ground reflected<br />

radiation in this <strong>an</strong>alysis but its inclusion would be straight forward.<br />

dss

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