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Lec 31

This document summarizes the daily energy incident on a horizontal flat plate from solar radiation. It provides the equation to calculate the daily incident energy (H naught) in kilowatt hours per meter squared per day based on the solar constant, latitude, day number, and sunrise/sunset hour angles. The key inputs are the latitude (φ) and day number, which are used to determine the declination (δ) and insulation constant (K). The sunrise/sunset hour angles depend only on the latitude and declination. This model calculates the horizontal flat plate energy without considering atmospheric effects.
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0% found this document useful (0 votes)
30 views4 pages

Lec 31

This document summarizes the daily energy incident on a horizontal flat plate from solar radiation. It provides the equation to calculate the daily incident energy (H naught) in kilowatt hours per meter squared per day based on the solar constant, latitude, day number, and sunrise/sunset hour angles. The key inputs are the latitude (φ) and day number, which are used to determine the declination (δ) and insulation constant (K). The sunrise/sunset hour angles depend only on the latitude and declination. This model calculates the horizontal flat plate energy without considering atmospheric effects.
Copyright
© © All Rights Reserved
We take content rights seriously. If you suspect this is your content, claim it here.
Available Formats
Download as PDF, TXT or read online on Scribd
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Indian Institute of Science

Design of Photovoltaic Systems

Prof. L Umanand

Department of Electronic Systems Engineering

Indian Institute of Science, Bangalore

NPTEL Online Certification Course

(Refer Slide Time: 00:18)

Let us now obtain the sunrise and sunset angles I have here the local cetera coordinate system
and the eccentric coordinate system, and I have also written down the insulation equation LCosθ Z
the normal incidence insulation at a horizontal flat plate located at a point on this latitude fight at
sunset and sunrise this θZ said will be 900C what it basically means is that the insulation line will
be just along the horizon plane at Sun far at sunset it will be just along the horizon plane it will
start to rise above the horizon plane and at sunset it will be along the horizon plane and start to
go below the horizon plane.

Therefore at sunset or sunrise we have θZ at the angle equal to π / 2 900C this will be 900C
because the insulation line is along the horizon plane and ω the our angle is the angle of interest
to us the our angle, we will call it as ωsr s our angle at sunrise and modulus of the our angle at
sunset, so you see that when ω = 0 the projection of the insulation line will be along the
meridional plane that would be considered as noon for that particular Meridian our angle on to
the east of the Meridian will be positive our angle to the west of the meridian is considered
negative.

So sunrise is on this quadrant on to the east side of the original axis and therefore sunrise angle is
considered positive and the sunset is to the west of the meridional axis and ωSS is considered as
negative but modulus of the sunset angle and our angle at sunrise will be the same applying
CosθZ = 0 at sunrise and sunset, so you say Cos Δ Cosωsr there is sunrise angle and Cosπ+ Sin �
Sinπ = 0 because CosθZ is 0 θZ that being π / 2 and from here you can get Cosω at sunrise which
is Cos inverse of – Tan of Tanϕ, so this is obtainable just directly from this step so you take Sin.
Sin � into this side and then Cosω is rs - Tans � Tan / ωsr will be Cos inverse of - Tan � Tan π
and the sunset angle is nothing but minus sunrise angle.

Because it is on the west side of the original axis so these two angles our angles our angle sunrise
our angle sunset are given by this relationship, entirely dependent on the declination and the
latitude of the place.

(Refer Slide Time: 04:24)


So now let us summarize the daily energy incident on a horizontal flat plate, so we know now H
naught is the daily incident energy and this is given by this relationship 24K L SCD solar constant
by ϕ into Cosϕ Cos � Sin ωsr + ω such Sinϕ Sin � and this is expressed in the unit kilowatt hour
per meter square per day where K is 1 + 0.03 3 + Cos360 N / 365 and n is the day number1 for
January 1st 365 for December 31st, so now this K is an expression which is obtained empirically
to obtain the insulation value at on a given day and LSC is the solar constant mean solar constant.

Which is 1.3k kilo watt per meter square ωsr is the sunrise hour angle which we saw just now
and this is given by Cos inverse of- Tanϕ Tan � again in terms of latitude and declination only
expressed in radians ϕ is the latitude and � is the declination both of these can be in radians or
degrees, now this can be considered as the model for obtaining the energy incident on a
horizontal flat plate without having considered the effects of atmosphere till, now we have not
considered atmospheric effects.

We will shortly discuss that also but right now this value is without any atmosphere by coming
into the picture to put it in a block algorithmic form let us say we need two important inputs one
is latitude ϕ another one is day number n that is we need the Dana Marion and the latitude ϕ
remaining.

Everything else is determinable can be calculated using the equations that we just now discussed
so the day from the day number we can get � declination and this constant K using this
relationship, so knowing ϕ as one of the inputs these 3 will be given to the model for estimating
the energy and you will get H0 in kilowatt hours per meter square per day and this whole block
algorithmically can be considered as the energy determining module for a horizontal flat plate.

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