Solar Pro 2.1, December/ January 2009

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Q&A
Technical Questions & Answers
Calculating Inter-Row Spacing
C
omputer software that permits
shadow studies is an excellent
design tool for large scale, ground
mounted PV arrays. These programs
model complex geometries with great
accuracy and speed. Assuming that
the CAD data entry is correct, these
inter-row spacing results are correct. In
all likelihood, your manual calculations
are correct as well—just incomplete.
Historically many photovoltaic systems arranged in rows were designed
using only an altitude angle calculation. This is the approach detailed, for
example, in the American Technical
Publishers’ textbook, Photovoltaic
Systems. The formula given there for
calculating minimum inter-row
shading is:
d = h ÷ tan α
According to the editors, d is the
minimum distance between rows; h is
the height differential between the top
of one row and the bottom of the row
to the north; and α is the solar altitude
angle.
It is more accurate to say that
this formula determines the shadow
distance between rows. But because
this shadow falls perpendicular to a
south-facing array only when the sun
is located at true south in the sky,
solar noon is the only time when the
length of the shadow cast between
rows would be equal to the minimum
inter-row distance. If your design
calculations call for a shade-free solar
window of 9am to 3pm on December
16
S o l a r pr o | December/January 2009
21, for example, then an azimuth angle
correction is required.
The first step for doing manual
inter-row spacing calculations is to
generate a sun path chart for the site, as
shown in Illustration 1. The University
of Oregon’s Solar Radiation Monitoring
Laboratory (SRML) provides an online
program for this purpose (solardat.
uoregon.edu/SoftwareTools.html). For
70º
11am
12pm
er Solstice
Summ
May/ Jul 21
10am
60º
50º
1pm
2pm
Apr/ Aug 21
9am
40º
and west longitude as negative numbers. Following these steps for Ogden,
Utah, results in a 41.21° latitude and a
-111.97° longitude.
Use the sun path chart in Illustration 1 to determine the sun’s altitude
angle at 9am and 3pm solar time on
December 21, the shortest day of the
year. Referring to the chart for Ogden,
Utah, the sun’s altitude angle for
3pm
Equinox
8am
4pm
Feb/ Oct 21
30º
Jan/ Nov 21
Winter
Solstice
7am
20º
= 13º
5pm
6am
6pm
10º
altitude angle
5am
7pm
azimuth correction
0º
120º
90º
East
60º
30º
= 42º
0º
South
-30º
-60º
-90º
West
-120º
Azimuth Angle
Illustration 1 When the latitude and longitude for Ogden, UT, are specified, the
SRML sun path chart program plots the path of the sun across the sky at that
location.
best results, enter the site’s specific latitude and longitude. These are easy to
obtain using the free version of Google
Earth (earth.google.com). Simply point
to the specific site, and latitude and
longitude are provided to the nearest
100th of a second in the lower left hand
corner of the program screen. Convert
the latitude and longitude provided
in Google Earth to decimal degrees.
Also, make sure to enter south latitude
design purposes is about 13°. Illustration 2 (p. 18) indicates that h equals
10 feet. We can now solve for the
shadow length (d_shadow) using the
referenced formula:
d_shadow = h ÷ tan α°
d_shadow = 10 ft. ÷ tan 13°
d_shadow = 10 ft. ÷ 0.231
d_shadow = 43.3 ft.
c o n ti n u e d o n pa g e 1 8
Da t a c o ur t e sy sola rda t.u ore gon .e du
he inter-row spacing calculations that
I am doing manually do not match
the results of our shadow studies in
AutoCAD. Which results are accurate?
What is the correct way to manually
calculate inter-row spacing for a ground
mounted PV array layout?
Altitude Angle
T
Q&A
d_shadow = 43.3'
h=10'
ttop
op
p of Ro
Row 1
35º
= 13º
bottom of Row 2
South
Illustration 2 Side view of inter-row shadow length at 9am
and 3pm on the winter solstice.
d_min = d_shadow x cos Ψ
d_min = 43.3 ft. x cos 42°
d_min = 43.3 ft. x 0.743
d_min = 32.2 ft.
m ollyoh a llor a n .c om (2)
South
sh
d_
ow
ad
=
'
.3
43
d_min = 32.2'
top of Row 1
= 42º
Illustration 3 Plan view at 9am.
18
Once shadow length is determined, it is time to apply
the azimuth angle correction. Referring again to the sun
path chart for Ogden, Utah, the sun’s azimuth is approximately 42° east of true south at 9am and 42° west at 3pm
on the winter solstice. As Illustration 3 indicates, knowing
both the shadow length and the azimuth (Ψ) correction
angle allows us to solve for minimum inter-row spacing
(d_min):
S o l a r pr o | December/January 2009
bottom of Row 2
The azimuth angle correction detailed here is very
significant for PV system designers, integrators and their
customers. Inter-row spacing is reduced by 25% in this
example. This could mean 25% less site grading or a 25%
larger array for the client. Improving power density in this
manner can increase PV plant size, energy harvest, revenue,
profit or all of the above.
—Ken Gardner / Gardner Engineering Alternative Energy Services /
Ogden, UT / gardnerengineering.net
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