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Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must...

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Solar Site Assessment
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Page 2: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

Why the variation in solar radiation?

• Amount of atmosphere sun’s energy must travel through to reach earth– Time of day, Time of year, tilt of earth

• Cloudiness• Shading

Page 3: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 4: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

NC SOLAR RESOURCE

Other Cities for Comparison

Miami, FL 5.2

Albany, NY 4.3

Phoenix, AZ 6.5

Tokyo 4.5

Berlin 3.0

Page 5: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 6: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 7: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

SUMMER SOLSTICE NORTHERN HEMISPHERE

Page 8: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

Solar Trajectory

2-3Solar Resources - Solar Radiation

Page 9: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 10: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 11: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 12: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 13: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

General Siting Guidelines

• Face Collectors towards the south

• Year round performance will be greatest if collectors tilted at angle of latitude (36 degrees)

• Summer Lat – 15• Winter Lat + 15• Clear of shading from

9 – 3

Page 14: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

Roof Pitch     Tilt Angle (°)  

4/12 18.4

5/12 22.6

6/12 26.6

7/12 30.3

8/12 33.7

9/12 36.9

10/12 39.8

11/12 42.5

12/12 45.0

Tilt Angles & Roof Pitch

Page 15: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

100% 95.5%

81.5%

61.4%

49.0%

0%10%20%30%40%50%60%70%80%90%

100%

South Southeast East Northeast North

Perc

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t o

f M

axim

um

Do We Have to Face Exactly South?

Raleigh NC 35.9º Latitude

Page 16: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

84%

95%97%

98% 99% 100% 100% 99% 98%

51%

0%

10%

20%

30%

40%

50%

60%

70%

80%

90%

100%

Horizontal (0º) 3/12 (14º) 4/12 (18.4º) 5/12 (22.6º) 6/12 (26.6º) 7/12 (30.3º) 8/12 (33.7º) 10/12 (39.8º) 12/12 (45º) Vertical (90º)

Perc

en

t o

f M

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So What About Slope?

Raleigh, NC 35.9 deg Latitude 14 deg => 95% of

Maximum

Page 17: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

01

53

04

56

07

59

0-90 -60 -30 0 30 60 90

Slo

pe

Azimuth Angle

Annual Angle Modifier vs. Orientation Raleigh, NC

95%-100%90%-95%

85%-90%

80%-85%

Fraction of

East WestSouth

Orientation Effect on Annual Output

Page 18: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

Shading can reduce performance significantly

Page 19: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

Types of Solar Site Assessments

1. Compass, Protractor with Weighted String and Sun Chart Method

• All you need is a pencil, sun chart, compass, and a protractor with a weighted string.

http://solardat.uoregon.edu/SunChartProgram.html

Page 20: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 21: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 22: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 23: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 24: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 25: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 26: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

Compass and Protractor Method1. Stand at the proposed site.2. Face south, adjusting for magnetic declination3. Point the flat end of the protractor at the horizon or any

other obstructions (trees, buildings, etc.)4. Measure the number of degrees the string is off from 90

degrees.5. Record findings on Sun chart.6. Repeat process in 15 degree increments for both East and

West.7. Connect horizon dots and see if any hours are obstructed

for any months between the hours of 9a – 3p.

Page 27: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 28: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 29: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

Magnetic Declination

• Magnetic declination is the deviation of magnetic north from true north or how much and in what direction the compass needle is off of true north.

• True south in western NC is approximately 7 degrees west of magnetic south

Page 30: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

Magnetic Declination in the U.S.

Page 31: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

Using the Solar Pathfinder

Page 32: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

Pathfinder on Roof

Page 33: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

Solar Pathfinder

http://www.solarpathfinder.com/video

Page 34: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 35: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 36: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Page 38: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

Extension Kit

Page 39: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

Solmetric PV Designer

http://www.solmetric.com/buy210.htmlhttp://www.solmetric.com/

Page 40: Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.

Solmetric PV Designer


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