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TERRA Validation:Saudi Arabian Solar Radiation FluxGround Measurements |
NETWORK INSTRUMENTATION
The following table lists network instrumentation common to all sites:
| PARAMETER | UNITS | SENSOR | MANF. | MODEL | UNCERTAINTY | COMMENTS |
|---|---|---|---|---|---|---|
| Ambient Temperature | Deg C | 1000 Ohm Plat. Resistance Thermometer |
Vaisala | 50 Y | +/- 0.5 Deg C | Combined Temp. and RH sensor |
| Relative Humidity | % RH | Capacitive | Vaisala | 50Y | +/- 2.5% | 0%-100% range |
| Global horizontal solar Irradiance |
W/m2 | Type -T Thermopile |
Eppley Laboratory |
PSP | +/- 3.0% @ 1 kW/m2 |
Using single calibration factor |
| Direct Beam Solar Irradiance |
W/m2 | Type -T Thermopile |
Eppley Laboratory |
NIP | +/- 2.0% @ 1 kW/m2 |
5.7° field of view |
| Diffuse Horizontal Solar Irradiance |
W/m2 | Type -T Thermopile |
Eppley Laboratory |
PSP | +/- 3.0% @ 1 kW/m2 |
Under tracking shading disk subtending 5.7° |
| Solar Tracker: Direct Beam |
n/a | Synchronous motor drive |
Eppley Laboratory |
ST-1 | +/- 3.0° per day | manual alignment daily |
| Solar Tracker: Shade Disk |
n/a | Synchronous motor drive |
Eppley Laboratory |
RSD-2 | +/- 3.0° per day | manual alignment daily |
| Data Logger | volts | Analog to digital sample and hold |
Campbell Scientific, Inc. |
CR-10 | 0.2% Full Scale | Full scale: 25 mV Resolution 3.33 mV Time +/- 4 ms noise<0.8 uV RMS |
All but Solar Village instrumentation is mounted on 0.5 m tall instrumentation
platform at station ground level. At sandy soil sites, platform mounted on concrete pads.
Solar Village Installation on 0.5 m tall instrumentation platform at 10 m above ground on
building rooftop. Site layout to be incorporated into metadata.
Sample rate: 10 seconds (0.1 Hz)
Data rate: 5 minute (0.0033 Hz)
Clock accuracy +/- 2.0 Sec/ Day (set nightly with respect to national time standards)
Network Instrumentation Calibration History
ADDITIONAL INSTRUMENTATION
The Solar Village station is instrumented with addition sensors designed to operate in conformance with WMO/WCRP BSRN specifications. BSRN instrumentation deployed at the Solar Village is described in table 2.
| PARAMETER | UNITS | SENSOR | MANF. | MODEL | UNCERTAINTY | COMMENTS |
|---|---|---|---|---|---|---|
| Direct Beam Absolute Cavity Pyrheliometer |
W/m2 | Wire wound Type T Cu-Ct Thermopile solid silver inverted cone cavity |
Eppley Laboratory |
AHF Auto- matic Hickey- Frieden |
+/- 0.45% | @ 1kW/m2 Corning 7940 fused silica window correction factor additional 0.8% uncertainty. Tracking by BRUSAG tracker |
| Downwelling longwave (sky irradiance) under Shading Disk |
W/m2 | Pyrgeometer Type T Thermopiles |
Eppley Laboratory |
PIR | +/- 10 W/m2 | Silicon dome with thin film interference filter passing longwave (wavelength >8 micron ) infrared Shade disk mounted on BRUSAG tracker |
| Upwelling Longwave (ground emission) |
W/m2 | Pyrgeometer Type T Thermopiles |
Eppley Laboratory |
PIR | +/- 10 W/m2 | As above, mounted at 100 ft (33 m) level at 3 ft (1 m) from 1 ft (0.3 m) diameter tower; body shaded from direct sun, downward looking |
| Upwelling shortwave radiation |
W/m2 | Type T Thermopiles |
Eppley Laboratory |
PSP | +/- 3.0% @ 1 kW/m2 |
100 ft (33 m) level at 3 ft (1 m) from 1 ft (0.3 m) diameter tower; body shaded from direct sun, downward looking |
| Solar Tracker: Cavity radiometer Direct Beam and downwelling longwave shade disk |
n/a | Stepping motor drive |
BRUSAG | INTRA | +/- 0.2° per day | autonomous, self correcting based on quad Silicon solar sensor input on clear days |
| Aerosol Optical Depth | n/a | filtered silicon cell sunphoto- meter(*) |
CIMEL Electronique |
CE-318 | +/- 0.01 OD | Wavelengths at 340, 380,440,500,670,870, 1020 nm. Autonomous collection at 0.5 air mass intervals. Real time collection via METEOSAT at NASA Langley |
| Total Column Water Vapor |
cm | as above | as above | as above |
+/- 10% | Range 0.1-5 cm ( 1 mm to 50 mm) |
| Cloud Properties (height, layers) |
km | Nd:YF diode laser source & EGG SPCM- AQ-121 avalanche diode detector |
Science and Engineering Services, Inc. |
MPL(**) | +/- 0.3 km | 523 nm Wavelength, 18 bins up to 60 km 300 m resolution. Layer and boundary information from backscatter analysis |
(*) Deployed by 24 Feb 1999
(**) deployment to be determined with respect to availability of instrumentation and logistics
with Saudi participants.
BSRN radiometric fluxes recorded at 2 second (0.5 Hz) sample interval with 1 minute (0.0167 Hz) averages reported.
BSRN Instrumentation Calibration History
The Solar Village site serves as the Central Calibration Facility and Network Operations Center
for the Saudi Arabian Solar Network. Calibration instrumentation deployed at the site is listed in
the following table:
| PARAMETER | UNITS | SENSOR | MANF. | MODEL | UNCERTAINTY | COMMENTS |
|---|---|---|---|---|---|---|
| WRR Direct Beam Calibration Reference |
W/m2 | Wire wound Type T Cu-Ct Thermopile on solid silver inverted cone cavity |
Eppley Laboratory |
AHF (Auto- matic Hickey- Frieden) |
+/- 0.45% | @ 1kW/m2 Corning 7940 fused silica window correction factor additional 0.8% uncertainty. Participated in WMO WRR IPC VIII 1995 |
| TWO Shading Disk Diffuse Pyranometers |
W/m2 | Type T Thermopiles |
Eppley Laboratory |
PSP | +/- 3.0% @ 1 kW/m2 |
Average of two tracking shading diffuse readings used for diffuse reference |
| Atmospheric Stability Monitors |
W/m2 | Silicon cell pyranometer |
Li-Cor, Inc. |
SB-200 | n/a | Monitor global sky stability, flag all data where variation over last 3 data pts exceeds 1% |
| Solar Tracker: Cavity radiometer Direct Beam and downwelling longwave shade disk |
n/a | Stepping motor drive |
BRUSAG | INTRA-1 | +/- 0.2° per day | autonomous, self correcting based on quad Silicon solar sensor input on clear days |
| Calibration Data Logger |
volts | Analog to digital sample and hold |
John Fluke Company |
Helios | 0.05% Full Scale | Full scale: 25 mV Resolution 100 nV noise<50 nV RMS |
Data is recorded during Broadband Outdoor Calibration (BORCAL) events at 30 second intervals using the NREL Radiometer Calibration and Characterization (RCC) software. The software monitors atmospheric stability, total column water vapor, and broadband aerosol optical depth during the calibration event. Pyrheliometers are calibrated directly against the absolute cavity pyrheliometer. Pyranometers are calibrated against the reference irradiance derived from the absolute cavity pyrheliometer * cosine (zenith angle) + diffuse reference irradiance. Basic uncertainty "kernel" for each individual derived calibration factor (responsivity) is 1.3% (13 W/m2) of full scale reading (1 kW/m2) due to WRR uncertainty, temperature, data logger, solar geometry, and individual instrumental effects. Pyranometer calibration factors are binned according to 10 degree zenith angle increments for post-processing removal of cosine response effects for each individual radiometer. A "composite" cosine weighted average of the binned responsivities is used to derive the calibration factor used in recording the network 5 minute average data.
| BSRN and typical station instrument platform. | Panorama around base of 30 meter tower for upwelling radiation measurements. | Panorama around BSRN shortwave radiation site. |
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