TimeStep Daylighting Calculation[LINK]
A daylighting calculation is performed each time step that the sun is up for each zone that has one or more daylighting reference points specified. The exterior horizontal illuminance from the sun and sky is determined from solar irradiance data from the weather file. The interior illuminance at each reference point is found for each window by interpolating the daylight illuminance factors for the current sun position, then, for skyrelated interior illuminance, multiplying by the exterior horizontal illuminance from the appropriate sky types that time step, and, for sunrelated interior illuminance, multiplying by the exterior horizontal solar illuminance that time step. By summation, the net illuminance and glare due to all of the windows in a zone are found. If glare control has been specified window shading (by movable shading devices or switchable glazing) is deployed to reduce glare. Finally the illuminance at each reference point for the final window and shade configuration is used by the lighting control system simulation to determine the electric lighting power required to meet the illuminance setpoint at each reference point.
Variables in TimeStep Calculations
Snorm,dir

Direct normal solar irradiance 
W/m2

BeamSolarRad 
Sh,dif

Exterior diffuse horizontal solar irradiance 
W/m2

SDIFH, DifSolarRad 
Sh,dir

Exterior direct horizontal solar irradiance 
W/m2

SDIRH 
Z 
Solar zenith angle 
radians 
Zeta 
m 
Relative optical air mass 
 
AirMass 
Δ 
Sky brightness 
 
SkyBrightness 
ε 
Sky clearness 
 
SkyClearness 
k, k’ 
Sky type index 
 
ISky 
sk,k′

Interpolation factor for skies k and k’ 
 
SkyWeight 
ψk,k′

Sky luminance distribution formed from linear interpolation of skies k and k’ 
cd/m2

 
fk

Fraction of sky that is type k 
 
 
Eh,k

Horizontal illuminance from sky type k 
cd/m2

HorIllSky 
Eh,sky

Exterior horizontal illuminance from sky 
lux 
HISKF 
Eh,sun

Exterior horizontal illuminance from sun 
lux 
HISUNF 
ηdif, ηdir

Luminous efficacy of diffuse and direct solar radiation 
lm/W 
DiffLumEff, DirLumEff 
Iwin

Interior illuminance from a window 
lux 
DaylIllum 
Swin

Window luminance 
cd/m2

SourceLumFromWinAtRefPt 
Bwin

Window background luminance 
cd/m2

BACLUM 
dsun, dsky,k

Interior illuminance factor for sun, for sky of type k 
 
DaylIllFacSun, DFSUHR, DaylIllFacSky, DFSUHR 
wsun, wsky,k

Window luminance factor for sun, for sky of type k 
 
DaylSourceFacSun, SFSUHR, DaylSourceFacSky, SFSKHR 
bsun, bsky,k

Window background luminance factor for sun, for sky of type k 
 
DaylBackFacSun, BFSUHR, DaylBackFacSky, BFSKHR 
wj

Weighting factor for time step interpolation 
 
WeightNow 
iL

Reference point index 
 
IL 
iS

Window shade index 
 
IS 
Itot

Total daylight illuminance at reference point 
lux 
DaylIllum 
Btot, B 
Total window background luminance 
cd/m2

BLUM 
Iset

Illuminance setpoint 
lux 
ZoneDaylight(ZoneNum).IllumSetPoint 
fL

Fractional electric lighting output 
 
FL 
fp

Fractional electric lighting input power 
 
FP 
NL

Number of steps in a stepped control system 
 
LightControlSteps 
MP

Lighting power multiplier 
 
ZonePowerReductionFactor 
TimeStep Sky Luminance[LINK]
The sky luminance distribution, ψ, for a particular time step is expressed as a linear interpolation of two of the four standard skies — ψcs, ψts , ψis and ψos — described above under “Sky Luminance Distributions.” The two sky types that are interpolated depend on the value of the sky clearness. The interpolation factors are a function of sky clearness and sky brightness (Perez et al., 1990). Sky clearness is given by:
ε=Sh,dif+Snorm,dirSh,dif+κZ31+κZ3
where Sh,dif is the diffuse horizontal solar irradiance, Snorm,dir is the direct normal solar irradiance, Z is the solar zenith angle and κ is a constant equal to 1.041 for Z in radians.
Sky brightness is given by:
Δ=Sh,difm/Sextnorm,dir
where m is the relative optical air mass and Sextnorm,dir is the extraterrestrial direct normal solar irradiance.
The relative optional air mass is calculated as follows:
m=1−1e−4⋅hsin(b)+0.15(b+3.885)1.253
where b is the Solar Altitude Angle, that is the angle of the sun above the horizontal (in degrees), and h is the building altitude (elevation, in meters).
b=Π2−ZDegToRadians
If ε ≤ 1.2,
ψis,os=sis,osψis+(1−sis,os)ψos
where ψis is the intermediate sky luminance distribution, ψos is the overcast sky luminance distribution, and
sis,os=min{1,max[0,(ε−1)/0.2,(Δ−0.05)/0.4]}
If 1.2 <ε ≤ 3
ψts,is=sts,isψts+(1−sts,is)ψis
where ψts is the clear turbid sky luminance distribution and
sts,is=(ε−1.2)/1.8
If ε > 3,
ψcs,ts=scs,tsψcs+(1−scs,ts)ψts
where ψcs is the clear sky luminance distribution and
scs,ts=min[1,(ε−3)/3]
Interior Illuminance[LINK]
For each time step the interior illuminance, Iwin, from a window is calculated as follows by multiplying daylight factors and exterior illuminance.
First, the sun and skyrelated daylight illuminance factors for the time step are determined by interpolation of the hourly factors:
¯dsun(iL,iS)=wjdsun(iL,iS,ih)+(1−wj)dsun(iL,iS,ih+1)
¯dsky,k(iL,iS)=wjdsky,k(iL,iS,ih)+(1−wj)dsky,k(iL,iS,ih+1)
where iL is the reference point index (1 or 2), iS is the window shade index (1 for unshaded window, 2 for shaded window), ih is the hour number, and k is the sky type index. For the jth time step in an hour, the timestep interpolation weight is given by:
wj=1−min[1,j/Nt]
where Nt is the number of time steps per hour.
The interior illuminance from a window is calculated as:
Iwin(iL,iS)=¯dsunEh,sun+[¯dsky,k(iL,iS)fk+¯dsky,k′(iL,iS)fk′]Eh,sky
where Eh,sun and Eh,sky are the exterior horizontal illuminance from the sun and sky, respectively, and fk and fk′ are the fraction of the exterior horizontal illuminance from the sky that is due to sky type k and k’, respectively.
The horizontal illuminance from sun and sky are given by:
Eh,sun=ηdirSnorm,dircosZEh,sky=ηdifSh,dif
where Z is the solar zenith angle, ηdif is the luminous efficacy (in lumens/Watt) of diffuse solar radiation from the sky and ηdir is the luminous efficacy of direct radiation from the sun. The efficacies are calculated from direct and global solar irradiance using a method described in (Perez et al, 1990), inside the DayltgLuminousEfficacy routine of the WeatherManager module.
The fractions fk and fk′ are given by:
fk=sk,k′Eh,ksk,k′Eh,k+(1−sk,k′)Eh,k′fk′=(1−sk,k′)Eh,k′sk,k′Eh,k+(1−sk,k′)Eh,k′
where Eh,k and Eh,k′ are the horizontal illuminances from skies k and k’, respectively (see “Exterior Horizontal Luminance,” above), and sk,k′ is the interpolation factor for skies kand k’(see “TimeStep Sky Luminance," above). For example, if ε > 3, k = cs (clear sky), k’ = ts (clear turbid sky) and
sk,k′=scs,ts=min[1,(ε−3)/3]
Similarly, the window source luminance, Swin, and window background luminance, Bwin, for a window are calculated from
Swin(iL,iS)=¯wsunEh,sun+[¯wsky,k(iL,iS)fk+¯wsky,k′(iL,iS)fk′]Eh,sky
Bwin(iL,iS)=¯bsunEh,sun+[¯bsky,k(iL,iS)fk+¯bsky,k′(iL,iS)fk′]Eh,sky
The total illuminance at a reference point from all of the exterior windows in a zone is
Itot(iL)=∑windowsin zoneIwin(is,iL)
where iS = 1 if the window is unshaded and iS = 2 if the window is shaded that time step. (Before the illuminance calculation is done the window shading control will have been simulated to determine whether or not the window is shaded.)
Similarly, the total background luminance is calculated:
Btot(iL)=∑windowsin zoneBwin(is,iL)
The net glare index at each reference point is calculated as:
GI(iL)=10log10∑windowsin zoneSwin(iL,iS)1.6Ω(iL)0.8B(iL)+0.07ω(iL)0.5Swin(iL,iS)
where
B(iL)=max(Bwin(iL),ρbIset(iL))
In the last relationship, the background luminance is approximated as the larger of the background luminance from daylight and the average background luminance that would be produced by the electric lighting at full power if the illuminance on the room surfaces were equal to the setpoint illuminance. In a more detailed calculation, where the luminance of each room surface is separately determined, B(iL) would be better approximated as an areaweighted luminance of the surfaces surrounding a window, taking into account the luminance contribution from the electric lights.
Glare Control Logic[LINK]
If glare control has been specified and the glare index at either reference point exceeds a userspecified maximum value, GI,max, then the windows in the zone are shaded one by one in attempt to bring the glare at both points below GI,max. (Each time a window is shaded the glare and illuminance at each reference point is recalculated.) The following logic is used:
If there is only one reference point, shade a window if it is unshaded and shading it decreases the glare, even if it does not decrease the glare below GI,max. Note that if a window has already been shaded, say to control solar gain, it will be left in the shaded state.

If there are two reference points, then:
If glare is too high at both points, shade the window if it decreases glare at both points.
If glare is too high only at the first point, shade the window if the glare at the first point decreases, and the glare at the second point stays below GI,max.
If glare is too high only at the second point, shade the window if the glare at the second point decreases, and the glare at the first point stays below GI,max.
Shades are closed in the order specified by the fenestration objects listed in the WindowShadingControl object until glare at both points is below GI,max, or until there are no more windows left to shade.
Lighting Control System Simulation[LINK]
Once the final daylight illuminance value at each reference point has been determined, the electric lighting control is simulated. The fractional electric lighting output, fL, required to meet the setpoint at reference point iL is given by
fL(iL)=max[0,Iset(iL)−Itot(iL)Iset(iL)]
Here, Iset is the illuminance setpoint and Itot is the daylight illuminance at the reference point. This relationship assumes that the electric lights at full power produce an illuminance equal to Iset at the reference point.
The fractional electric lighting input power, fP, corresponding to fL is then calculated. The relationship between fP and fL depends on the lighting control type.
Continuous Dimming Control[LINK]
For a continuouslydimmable control system, it is assumed that fP is constant and equal to fP,minfor fL<fL,min and that fP increases linearly from fP,min to 1.0 as fL increases from fL,min to 1.0 (Figure 1). This gives:
fP=⎧⎨⎩fP,minfor fL<fL,minfL+(1−fL)fP,min−fL,min1−fL,minfor fL,min≤fL≤1
Continuous/Off Dimming Control[LINK]
A “continuous/off” dimming system has the same behavior as a continuous dimming system except that the lights switch off for fL < fL,min rather than staying at fP,min.
Stepped Control[LINK]
For a stepped control system, fP takes on discrete values depending on the range of fL and the number of steps, NL (Figure 2). This gives:
fP=⎧⎪
⎪
⎪⎨⎪
⎪
⎪⎩0for fL=0int(NLfL)+1NLfor 0<fL<11for fL=1
If a lighting control probability, PL, is specified, f(P) is set one level higher a fraction of the time equal to 1−p(L). Specifically, if fP<1, fP=fP+1/NL if a random number between 0 and 1 exceeds pL. This can be used to simulate the uncertainty associated with manual switching of lights.
Lighting Power Reduction[LINK]
Using the value of fP at each reference point and the fraction fZ of the zone controlled by the reference point, the net lighting power multiplier, MP, for the entire zone is calculated; this value multiplies the lighting power output without daylighting.
MP=2∑iL=1fP(iL)fZ(iL)+⎛⎝1−2∑iL=1fZ(iL)⎞⎠
In this expression, the term to the right in the parentheses corresponds to the fraction of the zone not controlled by either reference point. For this fraction the electric lighting is unaffected and the power multiplier is 1.0.
CIE Technical Committee 4.2. 1973. Standardization of the Luminance Distribution on Clear Skies. CIE Pub. No. 22, Commission Internationale d’Eclairage, Paris.
Hopkinson, R.G., J. Longmore and P. Petherbridge. 1954. An Empirical Formula for the Computation of the Indirect Component of Daylight Factors. Trans. Illum. Eng. Soc. (London) 19, 201.
Hopkinson, R.G., P. Petherbridge and J. Longmore. 1966. Daylighting. Heinnemann, London, p. 322.
Hopkinson, R.G. 1970. Glare from Windows. Construction Research and Development Journal 2, 98.
Hopkinson, R.G. 1972. Glare from Daylighting in Buildings. Applied Ergonomics 3, 206.
Kittler, R. 1965. Standardization of Outdoor Conditions for the Calculation of the Daylight Factor with Clear Skies. Proc. CIE InterSession Meeting on Sunlight, NewcastleUponTyne.
Lynes, J.A. 1968. Principles of Natural Lighting. Applied Science Publishers, Ltd., London, p. 129.
Matsuura, K. 1987. Luminance Distributions of Various Reference Skies. CIE Technical Report of TC 309.
Moon, P. and D. Spencer. 1942. Illumination from a Nonuniform Sky. Illuminating Engineering 37, 707726.
Perez, R., P. Ineichen, R. Seals, J. Michalsky and R. Stewart. 1990. Modeling Daylight Availability and Irradiance Components from Direct and Global Irradiance. Solar Energy 44, 271289.
Petherbridge, P. and J. Longmore. 1954. Solid Angles Applied to Visual Comfort Problems. Light and Lighting 47,173.
Winkelmann, F.C. 1983. Daylighting Calculation in DOE2. Lawrence Berkeley Laboratory report no. LBL11353, January 1983.
Winkelmann, F.C. and S. Selkowitz. 1985. Daylighting Simulation in the DOE2 Building Energy Analysis Program. Energy and Buildings 8, 271286.
TimeStep Daylighting Calculation[LINK]
Overview[LINK]
A daylighting calculation is performed each time step that the sun is up for each zone that has one or more daylighting reference points specified. The exterior horizontal illuminance from the sun and sky is determined from solar irradiance data from the weather file. The interior illuminance at each reference point is found for each window by interpolating the daylight illuminance factors for the current sun position, then, for skyrelated interior illuminance, multiplying by the exterior horizontal illuminance from the appropriate sky types that time step, and, for sunrelated interior illuminance, multiplying by the exterior horizontal solar illuminance that time step. By summation, the net illuminance and glare due to all of the windows in a zone are found. If glare control has been specified window shading (by movable shading devices or switchable glazing) is deployed to reduce glare. Finally the illuminance at each reference point for the final window and shade configuration is used by the lighting control system simulation to determine the electric lighting power required to meet the illuminance setpoint at each reference point.
TimeStep Sky Luminance[LINK]
The sky luminance distribution, ψ, for a particular time step is expressed as a linear interpolation of two of the four standard skies — ψcs, ψts , ψis and ψos — described above under “Sky Luminance Distributions.” The two sky types that are interpolated depend on the value of the sky clearness. The interpolation factors are a function of sky clearness and sky brightness (Perez et al., 1990). Sky clearness is given by:
ε=Sh,dif+Snorm,dirSh,dif+κZ31+κZ3
where Sh,dif is the diffuse horizontal solar irradiance, Snorm,dir is the direct normal solar irradiance, Z is the solar zenith angle and κ is a constant equal to 1.041 for Z in radians.
Sky brightness is given by:
Δ=Sh,difm/Sextnorm,dir
where m is the relative optical air mass and Sextnorm,dir is the extraterrestrial direct normal solar irradiance.
The relative optional air mass is calculated as follows:
m=1−1e−4⋅hsin(b)+0.15(b+3.885)1.253
where b is the Solar Altitude Angle, that is the angle of the sun above the horizontal (in degrees), and h is the building altitude (elevation, in meters).
b=Π2−ZDegToRadians
If ε ≤ 1.2,
ψis,os=sis,osψis+(1−sis,os)ψos
where ψis is the intermediate sky luminance distribution, ψos is the overcast sky luminance distribution, and
sis,os=min{1,max[0,(ε−1)/0.2,(Δ−0.05)/0.4]}
If 1.2 <ε ≤ 3
ψts,is=sts,isψts+(1−sts,is)ψis
where ψts is the clear turbid sky luminance distribution and
sts,is=(ε−1.2)/1.8
If ε > 3,
ψcs,ts=scs,tsψcs+(1−scs,ts)ψts
where ψcs is the clear sky luminance distribution and
scs,ts=min[1,(ε−3)/3]
Interior Illuminance[LINK]
For each time step the interior illuminance, Iwin, from a window is calculated as follows by multiplying daylight factors and exterior illuminance.
First, the sun and skyrelated daylight illuminance factors for the time step are determined by interpolation of the hourly factors:
¯dsun(iL,iS)=wjdsun(iL,iS,ih)+(1−wj)dsun(iL,iS,ih+1)
¯dsky,k(iL,iS)=wjdsky,k(iL,iS,ih)+(1−wj)dsky,k(iL,iS,ih+1)
where iL is the reference point index (1 or 2), iS is the window shade index (1 for unshaded window, 2 for shaded window), ih is the hour number, and k is the sky type index. For the jth time step in an hour, the timestep interpolation weight is given by:
wj=1−min[1,j/Nt]
where Nt is the number of time steps per hour.
The interior illuminance from a window is calculated as:
Iwin(iL,iS)=¯dsunEh,sun+[¯dsky,k(iL,iS)fk+¯dsky,k′(iL,iS)fk′]Eh,sky
where Eh,sun and Eh,sky are the exterior horizontal illuminance from the sun and sky, respectively, and fk and fk′ are the fraction of the exterior horizontal illuminance from the sky that is due to sky type k and k’, respectively.
The horizontal illuminance from sun and sky are given by:
Eh,sun=ηdirSnorm,dircosZEh,sky=ηdifSh,dif
where Z is the solar zenith angle, ηdif is the luminous efficacy (in lumens/Watt) of diffuse solar radiation from the sky and ηdir is the luminous efficacy of direct radiation from the sun. The efficacies are calculated from direct and global solar irradiance using a method described in (Perez et al, 1990), inside the DayltgLuminousEfficacy routine of the WeatherManager module.
The fractions fk and fk′ are given by:
fk=sk,k′Eh,ksk,k′Eh,k+(1−sk,k′)Eh,k′fk′=(1−sk,k′)Eh,k′sk,k′Eh,k+(1−sk,k′)Eh,k′
where Eh,k and Eh,k′ are the horizontal illuminances from skies k and k’, respectively (see “Exterior Horizontal Luminance,” above), and sk,k′ is the interpolation factor for skies kand k’(see “TimeStep Sky Luminance," above). For example, if ε > 3, k = cs (clear sky), k’ = ts (clear turbid sky) and
sk,k′=scs,ts=min[1,(ε−3)/3]
Similarly, the window source luminance, Swin, and window background luminance, Bwin, for a window are calculated from
Swin(iL,iS)=¯wsunEh,sun+[¯wsky,k(iL,iS)fk+¯wsky,k′(iL,iS)fk′]Eh,sky
Bwin(iL,iS)=¯bsunEh,sun+[¯bsky,k(iL,iS)fk+¯bsky,k′(iL,iS)fk′]Eh,sky
The total illuminance at a reference point from all of the exterior windows in a zone is
Itot(iL)=∑windowsin zoneIwin(is,iL)
where iS = 1 if the window is unshaded and iS = 2 if the window is shaded that time step. (Before the illuminance calculation is done the window shading control will have been simulated to determine whether or not the window is shaded.)
Similarly, the total background luminance is calculated:
Btot(iL)=∑windowsin zoneBwin(is,iL)
Glare Index[LINK]
The net glare index at each reference point is calculated as:
GI(iL)=10log10∑windowsin zoneSwin(iL,iS)1.6Ω(iL)0.8B(iL)+0.07ω(iL)0.5Swin(iL,iS)
where
B(iL)=max(Bwin(iL),ρbIset(iL))
In the last relationship, the background luminance is approximated as the larger of the background luminance from daylight and the average background luminance that would be produced by the electric lighting at full power if the illuminance on the room surfaces were equal to the setpoint illuminance. In a more detailed calculation, where the luminance of each room surface is separately determined, B(iL) would be better approximated as an areaweighted luminance of the surfaces surrounding a window, taking into account the luminance contribution from the electric lights.
Glare Control Logic[LINK]
If glare control has been specified and the glare index at either reference point exceeds a userspecified maximum value, GI,max, then the windows in the zone are shaded one by one in attempt to bring the glare at both points below GI,max. (Each time a window is shaded the glare and illuminance at each reference point is recalculated.) The following logic is used:
If there is only one reference point, shade a window if it is unshaded and shading it decreases the glare, even if it does not decrease the glare below GI,max. Note that if a window has already been shaded, say to control solar gain, it will be left in the shaded state.
If there are two reference points, then:
If glare is too high at both points, shade the window if it decreases glare at both points.
If glare is too high only at the first point, shade the window if the glare at the first point decreases, and the glare at the second point stays below GI,max.
If glare is too high only at the second point, shade the window if the glare at the second point decreases, and the glare at the first point stays below GI,max.
Shades are closed in the order specified by the fenestration objects listed in the WindowShadingControl object until glare at both points is below GI,max, or until there are no more windows left to shade.
Lighting Control System Simulation[LINK]
Once the final daylight illuminance value at each reference point has been determined, the electric lighting control is simulated. The fractional electric lighting output, fL, required to meet the setpoint at reference point iL is given by
fL(iL)=max[0,Iset(iL)−Itot(iL)Iset(iL)]
Here, Iset is the illuminance setpoint and Itot is the daylight illuminance at the reference point. This relationship assumes that the electric lights at full power produce an illuminance equal to Iset at the reference point.
The fractional electric lighting input power, fP, corresponding to fL is then calculated. The relationship between fP and fL depends on the lighting control type.
Continuous Dimming Control[LINK]
For a continuouslydimmable control system, it is assumed that fP is constant and equal to fP,minfor fL<fL,min and that fP increases linearly from fP,min to 1.0 as fL increases from fL,min to 1.0 (Figure 1). This gives:
fP=⎧⎨⎩fP,minfor fL<fL,minfL+(1−fL)fP,min−fL,min1−fL,minfor fL,min≤fL≤1
Control action for a continuous dimming system. [fig:controlactionforacontinuousdimming]
Continuous/Off Dimming Control[LINK]
A “continuous/off” dimming system has the same behavior as a continuous dimming system except that the lights switch off for fL < fL,min rather than staying at fP,min.
Stepped Control[LINK]
For a stepped control system, fP takes on discrete values depending on the range of fL and the number of steps, NL (Figure 2). This gives:
fP=⎧⎪ ⎪ ⎪⎨⎪ ⎪ ⎪⎩0for fL=0int(NLfL)+1NLfor 0<fL<11for fL=1
If a lighting control probability, PL, is specified, f(P) is set one level higher a fraction of the time equal to 1−p(L). Specifically, if fP<1, fP=fP+1/NL if a random number between 0 and 1 exceeds pL. This can be used to simulate the uncertainty associated with manual switching of lights.
Stepped lighting control with three steps. [fig:steppedlightingcontrolwiththreesteps.]
Lighting Power Reduction[LINK]
Using the value of fP at each reference point and the fraction fZ of the zone controlled by the reference point, the net lighting power multiplier, MP, for the entire zone is calculated; this value multiplies the lighting power output without daylighting.
MP=2∑iL=1fP(iL)fZ(iL)+⎛⎝1−2∑iL=1fZ(iL)⎞⎠
In this expression, the term to the right in the parentheses corresponds to the fraction of the zone not controlled by either reference point. For this fraction the electric lighting is unaffected and the power multiplier is 1.0.
References[LINK]
CIE Technical Committee 4.2. 1973. Standardization of the Luminance Distribution on Clear Skies. CIE Pub. No. 22, Commission Internationale d’Eclairage, Paris.
Hopkinson, R.G., J. Longmore and P. Petherbridge. 1954. An Empirical Formula for the Computation of the Indirect Component of Daylight Factors. Trans. Illum. Eng. Soc. (London) 19, 201.
Hopkinson, R.G., P. Petherbridge and J. Longmore. 1966. Daylighting. Heinnemann, London, p. 322.
Hopkinson, R.G. 1970. Glare from Windows. Construction Research and Development Journal 2, 98.
Hopkinson, R.G. 1972. Glare from Daylighting in Buildings. Applied Ergonomics 3, 206.
Kittler, R. 1965. Standardization of Outdoor Conditions for the Calculation of the Daylight Factor with Clear Skies. Proc. CIE InterSession Meeting on Sunlight, NewcastleUponTyne.
Lynes, J.A. 1968. Principles of Natural Lighting. Applied Science Publishers, Ltd., London, p. 129.
Matsuura, K. 1987. Luminance Distributions of Various Reference Skies. CIE Technical Report of TC 309.
Moon, P. and D. Spencer. 1942. Illumination from a Nonuniform Sky. Illuminating Engineering 37, 707726.
Perez, R., P. Ineichen, R. Seals, J. Michalsky and R. Stewart. 1990. Modeling Daylight Availability and Irradiance Components from Direct and Global Irradiance. Solar Energy 44, 271289.
Petherbridge, P. and J. Longmore. 1954. Solid Angles Applied to Visual Comfort Problems. Light and Lighting 47,173.
Winkelmann, F.C. 1983. Daylighting Calculation in DOE2. Lawrence Berkeley Laboratory report no. LBL11353, January 1983.
Winkelmann, F.C. and S. Selkowitz. 1985. Daylighting Simulation in the DOE2 Building Energy Analysis Program. Energy and Buildings 8, 271286.
Documentation content copyright © 19962020 The Board of Trustees of the University of Illinois and the Regents of the University of California through the Ernest Orlando Lawrence Berkeley National Laboratory. All rights reserved. EnergyPlus is a trademark of the US Department of Energy.
This documentation is made available under the EnergyPlus Open Source License v1.0.