TERRA Validation:Saudi Arabian Solar Radiation FluxGround Measurements



NETWORK INSTRUMENTATION


The following table lists network instrumentation common to all sites:

TABLE 1. INSTRUMENTATION COMMON TO ALL NETWORK 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


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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.

TABLE 2: SOLAR VILLAGE BSRN RADIOMETRIC INSTRUMENTATION
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

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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:

TABLE 3: SOLAR VILLAGE RADIOMETRIC CALIBRATION INSTRUMENTATION
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.


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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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