StoffStoff
Civil/Environmental
- Dec 18, 2014
- 1
Hello Everyone,
I am currently working on a design project that deals with solar updraft concepts and I would urgently need some feedback and advice on two Problems i am encountering.
Problem 1) - I need to calculate the daily (preferably hourly) global solar insolation in W/m2 for Ciudad Real in Spain. I am using the following equations and data to do so:
Extraterrestrial Solar Radiation Calculation
Ho = (1/p) * Isc *Eo *[cos (λ)*cos(δ)*sin(ωs) +(p/180)*sin(λ)* sin(δ)* ωs]
where
Eo = 1.00011 + 0.034221*cos(Γ) + 0.00128*sin(Γ) + 0.000719*cos(2Γ) + 0.000077*sin(2Γ)
δ = (180/p) *(0.006918 - 0.399912*cos(Γ) + 0.07025*sin(Γ) - 0.006758*cos(2Γ) + 0.000907*sin(2Γ) - 0.002697*cos(3Γ)+0.00148*sin(3Γ))
Γ = 2*p *(nday - 1)/365
ωs = cos-1 [-sin(λ)* sin(δ)/cos(λ)* cos(δ)] or ωs = cos-1 [-tan(λ)* tan(δ)]
Ho = Daily Solar Radiation above the Atmosphere [MJ/m2d]
Eo = Eccentricity correction factor of Earth's orbit [-]
δ = Solar Declination [degrees]
Γ = Day Angle [radians]
ωs = Hour Angle of the Sun [degrees]
pi = 3.14159
nday = Day of the year ,e.g. January 1 = nday = 1 , February 1 = nday = 32, etc.
λ = Latitude of the site [degrees]
Isc = Solar constant = 118.11 [MJ/m2d]
Global Solar Radiation Calculation using the Hargreaves and Samani Model
H = Ho [AModel1(Tmax - Tmin)1/2] (H is also known as G)
where
H = Daily Global Solar Radiation [MJ/m2d]
Ho = Daily Solar Radiation above the Atmosphere [MJ/m2d]
Tmax = Daily Maximum Temperature [oC]
Tmin = Daily Minimum Temperature [oC]
AModel1 = Empirical Coefficient equal to 0.16 for interior regions [oC -0.5]
Conversion from MJ/m2[/sup]d to W/m2
1 MJ/m2d = 1E6 J/ m2[/sup]d = (1.000.000 J / m2d )*(d/60*60*24 s) = 11.57 J/ s m2 = 11.57 W/m2
1 MJ/m2d = 11.57 W/m2
Questions:
1)
Are the equations for Global Solar Radiation, H (or G) and Extraterrestrial Solar Radiation, Ho correct ?
2)
Do the equations for H and Ho calculate the daily average values for Global Solar Radiation (Gaverage) and Extraterrestrial Solar Radiation (Ho,average)?
3)
Is the conversion from MJ/m2d to W/m2 correct ?
4)
Are there more efficient or simpler yet accurate ways to calculate Global Solar Radiation for a given location ?
5)
Are my calculations of Ho and H correct ?
6)
Are there freely available data sets for the daily global horizontal solar radiation, (H or G) available for different Spanish towns and cities (Ciudad Real and Madrid in particular ? If so , where can I find them ?
I used Excel to process the following data and attached the file to the thread/post
Input Data:
Set 1
nday = 1 (January 1st)
Tmax = 12 C
Tmin = 6 C
λ = 39 degrees
Set 2
nday = 200 (July19th)
Tmax = 30 C
Tmin = 12 C
λ = 39 degrees
Results:
Set 1
Eo = 1,04 [-]
δ = -22.72 degrees / -0.40 radians
Γ = 0 degrees /radians
ωs = 70.18 degrees / 1.22 radians
Ho = 26.04 MJ/m2d
H = 10.21 MJ/m2d = 118.10 W/m2
Set 2
Eo = 0,97 [-]
δ = 21.30 degrees / 0,37 radians
Γ = 3.43 degrees / 0.06 radians
ωs = 108.40 degrees / 1.89 radians
Ho = 25.25 MJ/m2d
H = 17.14 MJ/m2d = 198.31 W/m2
Problem 2) The calculation of the power output Pturbine of the turbine a solar updraft tower
I am using the following equations to calculate Pturbine:
Equation 1 [(a*t*G - β*ΔT) *p*d2]/4 = Q*ρ*cp* ΔT
Equation 2 Q = K*A*[2*g*h*(ΔT)/ T1]0.5
Equation 3 Pturbine = cp*ρ*Q*(ΔT)
where
G = global solar radiation [W/m2]
a = soil absorptance of solar irradiation (= 0.89) [-]
t = glass transmittance for solar irradiation (=0. 88) [-]
β = equivalent heat losses [W/K]
ρ = density of air [kg/m3]
ΔT = T2 -T1 [K]
T1 = Temperature at the collector entrance [K]
T2 = Temperature at the collector exit at the turbine [K]
d = diameter of the solar collector [m]
cp = specific heat of air [J/Kg*K]
g = acceleration due to gravity [m/s2]
h = height of the solar tower stack [m]
K = discharge coefficient (= 0.65)
A = cross-sectional area of the solar updraft tower stack [m2]
Q = air mass moving speed [Kg/s]
Questions:
1)
Are equations 1, 2 and 3 correct?
2)
Can equation 1, 2 and 3 be used to calculate the daily power produced by the turbine ?
3)
Equations 1 and 2 are supposed to be solved simultaneously to calculate ΔT. How can this be done properly ?
I attempted to solve for ΔT and ended up with the following equations:
for equation 1, ΔT = (a*t*G*p*d2) / (4*Q*ρ*cp + β*p*d2)
for equation 2, ΔT = (Q2*T1) / [(K*A)2*2*g*h]
I set T1 equal to the average environmental temperature that exists outside the collector
Since Q is unknown, I attempt to solve for Q and got the following results:
(4 * ρ* cp* T1) *Q3 + ( β*pi*d2*T1) *Q2 - (K*A)2 * (2*g*h) * (a*t*G*p*d2) = 0
The equation above is of the following form:
a*x3 + b*x2 + c*x +d = 0
where
a = 4 * ρ* cp* T1
b = β*pi*d2* T1
c = 0
d = - (K*A)2 * (2*g*h) * (a*t*G*p*d2)
This cubic equation will yield 3 solutions/roots.
Sources:
1)
2)
3)
4)
I am currently working on a design project that deals with solar updraft concepts and I would urgently need some feedback and advice on two Problems i am encountering.
Problem 1) - I need to calculate the daily (preferably hourly) global solar insolation in W/m2 for Ciudad Real in Spain. I am using the following equations and data to do so:
Extraterrestrial Solar Radiation Calculation
Ho = (1/p) * Isc *Eo *[cos (λ)*cos(δ)*sin(ωs) +(p/180)*sin(λ)* sin(δ)* ωs]
where
Eo = 1.00011 + 0.034221*cos(Γ) + 0.00128*sin(Γ) + 0.000719*cos(2Γ) + 0.000077*sin(2Γ)
δ = (180/p) *(0.006918 - 0.399912*cos(Γ) + 0.07025*sin(Γ) - 0.006758*cos(2Γ) + 0.000907*sin(2Γ) - 0.002697*cos(3Γ)+0.00148*sin(3Γ))
Γ = 2*p *(nday - 1)/365
ωs = cos-1 [-sin(λ)* sin(δ)/cos(λ)* cos(δ)] or ωs = cos-1 [-tan(λ)* tan(δ)]
Ho = Daily Solar Radiation above the Atmosphere [MJ/m2d]
Eo = Eccentricity correction factor of Earth's orbit [-]
δ = Solar Declination [degrees]
Γ = Day Angle [radians]
ωs = Hour Angle of the Sun [degrees]
pi = 3.14159
nday = Day of the year ,e.g. January 1 = nday = 1 , February 1 = nday = 32, etc.
λ = Latitude of the site [degrees]
Isc = Solar constant = 118.11 [MJ/m2d]
Global Solar Radiation Calculation using the Hargreaves and Samani Model
H = Ho [AModel1(Tmax - Tmin)1/2] (H is also known as G)
where
H = Daily Global Solar Radiation [MJ/m2d]
Ho = Daily Solar Radiation above the Atmosphere [MJ/m2d]
Tmax = Daily Maximum Temperature [oC]
Tmin = Daily Minimum Temperature [oC]
AModel1 = Empirical Coefficient equal to 0.16 for interior regions [oC -0.5]
Conversion from MJ/m2[/sup]d to W/m2
1 MJ/m2d = 1E6 J/ m2[/sup]d = (1.000.000 J / m2d )*(d/60*60*24 s) = 11.57 J/ s m2 = 11.57 W/m2
1 MJ/m2d = 11.57 W/m2
Questions:
1)
Are the equations for Global Solar Radiation, H (or G) and Extraterrestrial Solar Radiation, Ho correct ?
2)
Do the equations for H and Ho calculate the daily average values for Global Solar Radiation (Gaverage) and Extraterrestrial Solar Radiation (Ho,average)?
3)
Is the conversion from MJ/m2d to W/m2 correct ?
4)
Are there more efficient or simpler yet accurate ways to calculate Global Solar Radiation for a given location ?
5)
Are my calculations of Ho and H correct ?
6)
Are there freely available data sets for the daily global horizontal solar radiation, (H or G) available for different Spanish towns and cities (Ciudad Real and Madrid in particular ? If so , where can I find them ?
I used Excel to process the following data and attached the file to the thread/post
Input Data:
Set 1
nday = 1 (January 1st)
Tmax = 12 C
Tmin = 6 C
λ = 39 degrees
Set 2
nday = 200 (July19th)
Tmax = 30 C
Tmin = 12 C
λ = 39 degrees
Results:
Set 1
Eo = 1,04 [-]
δ = -22.72 degrees / -0.40 radians
Γ = 0 degrees /radians
ωs = 70.18 degrees / 1.22 radians
Ho = 26.04 MJ/m2d
H = 10.21 MJ/m2d = 118.10 W/m2
Set 2
Eo = 0,97 [-]
δ = 21.30 degrees / 0,37 radians
Γ = 3.43 degrees / 0.06 radians
ωs = 108.40 degrees / 1.89 radians
Ho = 25.25 MJ/m2d
H = 17.14 MJ/m2d = 198.31 W/m2
Problem 2) The calculation of the power output Pturbine of the turbine a solar updraft tower
I am using the following equations to calculate Pturbine:
Equation 1 [(a*t*G - β*ΔT) *p*d2]/4 = Q*ρ*cp* ΔT
Equation 2 Q = K*A*[2*g*h*(ΔT)/ T1]0.5
Equation 3 Pturbine = cp*ρ*Q*(ΔT)
where
G = global solar radiation [W/m2]
a = soil absorptance of solar irradiation (= 0.89) [-]
t = glass transmittance for solar irradiation (=0. 88) [-]
β = equivalent heat losses [W/K]
ρ = density of air [kg/m3]
ΔT = T2 -T1 [K]
T1 = Temperature at the collector entrance [K]
T2 = Temperature at the collector exit at the turbine [K]
d = diameter of the solar collector [m]
cp = specific heat of air [J/Kg*K]
g = acceleration due to gravity [m/s2]
h = height of the solar tower stack [m]
K = discharge coefficient (= 0.65)
A = cross-sectional area of the solar updraft tower stack [m2]
Q = air mass moving speed [Kg/s]
Questions:
1)
Are equations 1, 2 and 3 correct?
2)
Can equation 1, 2 and 3 be used to calculate the daily power produced by the turbine ?
3)
Equations 1 and 2 are supposed to be solved simultaneously to calculate ΔT. How can this be done properly ?
I attempted to solve for ΔT and ended up with the following equations:
for equation 1, ΔT = (a*t*G*p*d2) / (4*Q*ρ*cp + β*p*d2)
for equation 2, ΔT = (Q2*T1) / [(K*A)2*2*g*h]
I set T1 equal to the average environmental temperature that exists outside the collector
Since Q is unknown, I attempt to solve for Q and got the following results:
(4 * ρ* cp* T1) *Q3 + ( β*pi*d2*T1) *Q2 - (K*A)2 * (2*g*h) * (a*t*G*p*d2) = 0
The equation above is of the following form:
a*x3 + b*x2 + c*x +d = 0
where
a = 4 * ρ* cp* T1
b = β*pi*d2* T1
c = 0
d = - (K*A)2 * (2*g*h) * (a*t*G*p*d2)
This cubic equation will yield 3 solutions/roots.
Sources:
1)
2)
3)
4)