A thermal modeling term. The value of a radiation conductor is input
in units of energy per unit time per degree**4. It is be computed as:
G = A * e(eff) * F(i-j) * s
or
G = A * F(i-j) * s
where;
| G |
value of the conductor |
| A |
area of the surface i |
| e(eff) |
emittance (dimensionless) |
| s |
Stefan-Boltzmann Constant (energy/length2-time-deg4) |
| F(i-j) |
black body view factor from surface i to j (dimensionless) |
| F(i-j) |
gray body view factor from surface i to j (area) |
The emittance e, is a measure of how well a body can radiate energy
as compared with a black body. Emittance is the ratio of total emissive
power of a real surface at temperature T to the total emissive power
of a black surface at the same temperature. The emittance of surfaces
is a function of several things including the material, surface condition,
and temperature. The emittance may be altered by polishing, roughing,
painting, etc.<
The view factor F(i-j) is a function of the geometry of the system
only. Many computer programs have been developed to compute the view
factors between complex geometry's; however view factors between some
surfaces with simple geometry's can be hand calculated. The methods
and equations are found in several heat transfer texts.
The gray body view factor F(i-j) is the product of the geometric
shape factor F(i-j) and a factor which allows for departures from black
body conditions (i.e. reflections). For example, for two parallel flat
plates:
F(1-2) = F(2-1) = 1
F(1-2) = [ 1 / ( 1/e1 + 1/e2 -1) ] x F(1-2)
The effective emittance e* between two surfaces may be used to compute
the gray body view factor with the following equation;
F(i-j) = e* x F(i-j)
The error induced by the use of e* is the result of neglecting secondary
reflections from surfaces other than the two for which the effective
emittance was determined.