Campbell Scientific SP-LITE Solar Radiation Sensor User Manual

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SP-LITE Silicon Pyranomete
Revision: 7/04
Copyright © 1998-2004
Campbell Scientific, Inc.

Warranty and Assistance

Products may not be returned without prior authorization. The following contact information is for US and International customers residing in countries served by Campbell Scientific, Inc. directly. Affiliate companies handle repairs for customers within their territories. Please visit www.campbellsci.com to determine which Campbell Scientific company serves your country. To obtain a Returned Materials Authorization (RMA), contact CAMPBELL SCIENTIFIC, INC., phone (435) 753-2342. After an applications engineer determines the nature of the problem, an RMA number will be issued. Please write this number clearly on the outside of the shipping container. CAMPBELL SCIENTIFIC's shipping address is:
CAMPBELL SCIENTIFIC, INC.
RMA#_____ 815 West 1800 North Logan, Utah 84321-1784
CAMPBELL SCIENTIFIC, INC. does not accept collect calls.
SP-LITE Table of Contents
PDF viewers note: These page numbers refer to the printed version of this document. Use the Adobe Acrobat® bookmarks tab for links to specific sections.
1. General Description.....................................................1
1.1 Electrical Properties..................................................................................1
1.2 Spectral Properties....................................................................................2
1.3 Directional/Cosine Response....................................................................3
2. Sensor Specifications.................................................4
3. Installing the SP-LITE..................................................5
4. Wiring............................................................................7
5. Datalogger Programming............................................7
5.1 Datalogger Input Range Codes.................................................................8
5.2 Calibration Factor and Multiplier.............................................................8
5.3 Program Example 1, Average Solar Radiation.........................................8
5.4 Program Example 2, Total Solar Radiation............................................10
5.4.1 Output Format Considerations......................................................10
5.5 Program Example 3, Average and Total Solar Radiation.......................12
6. Maintenance...............................................................13
6.1 Calibration.............................................................................................. 13
7. Troubleshooting ........................................................13
7.1 Pyranometer produces no apparent output..............................................13
7.2 Readings are not as expected..................................................................13
Figures
1. SP-LITE Sensor without Leveling Fixture.................................................1
2. SP-LITE Electrical Circuit..........................................................................2
3. Spectral Sensitivity of Pyranometers Compared with Solar Radiation ......2
4. Cosine Response of a Typical SP-LITE Pyranometer................................3
5. Dimensions of SP-LITE with Leveling Device..........................................4
6. 015ARM Mounting Arm............................................................................5
7. 025STAND and 019ALU Crossarm...........................................................6
8. SP-LITE to Datalogger Connections..........................................................7
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SP-LITE Table of Contents
Tables
1. Datalogger Connections for Differential Measurement............................. 7
2. Datalogger Connections for Single-Ended Measurement.......................... 7
3. Multipliers Required for Flux Density and Total Fluxes........................... 8
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SP-LITE Silicon Pyranometer

The SP-LITE measures incoming solar radiation (sun plus sky radiation) with a photodiode detector. Output from the photodiode is a current, which is converted to voltage by an internal shunt resistor. The SP-LITE can be used in solar energy applications such as plant growth, thermal convection and evapotranspiration.

1. General Description

FIGURE 1. SP-LITE Sensor without Leveling Fixture
The SP-LITE is used for measuring solar radiation. It measures the solar energy received from the entire hemisphere – i.e. 18field of view. The output is expressed in Watts per square meter (W m
The SP-LITE is designed for continuous outside use, and its calibration is valid only for unshaded natural daylight – not for artificial light. It is most usually used to measure solar radiation being received on the horizontal plane. However, the SP-LITE can, if required, be used in an inverted or tilted position.

1.1 Electrical Properties

The SP-LITE consists of a photodiode complete with housing and cable. The circuit includes a shunt resistor for the photodiode in order to generate a voltage output. The electrical specification of the sensor is determined by the characteristics of the photodiode and resistor. The electrical circuit of the pyranometer is shown in Figure 2, below.
The electrical sensitivity of the photodiode changes with temperature. A nominal value for this change is 0.2% change per °C. Calibration is carried out at 20 °C.
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SP-LITE Silicon Pyr an ome ter

1.2 Spectral Properties

FIGURE 2. SP-LITE Electrical Circuit
The spectral properties of the SP-LITE are mainly determined by the spectral response of the photodiode, which is shown in Figure 3, below.
FIGURE 3. Spectral Sensitivity of Pyranometers Compared with Solar
Radiation
The SP-LITE is calibrated for solar radiation under clear sky conditions. The spectrum for these conditions, at sea level, is also shown in Figure 3.
Unfortunately, however, the actual solar spectrum varies as a function of cloud cover, season and solar elevation. Since the pyranometer does not have a flat sensitivity across the whole solar spectrum, the accuracy of its response will vary. However, the error range across the whole spectrum has been proven to be small. The maximum total estimated error will only be in the region of ±5 percent when compared to the calibration conditions.
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