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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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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

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t o

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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