- The radiance temperature of the gold-point transfer
standard (GPTS) is determined by comparison to the gold
point blackbody. A high stability vacuum lamp operated at
approximately 1337.33 K is the gold-point transfer
standard.
- The radiance temperature of the working standard (WS) is
determined by comparison to the gold-point transfer
standard. A high stability vacuum lamp operated at
approximately 1528 K is the working standard.
- The FASCAL spectroradiometer is the transfer device used
to compare the sources.
- The transfer device is a CARY 14 spectroradiometer
which uses a prism/grating double monochromator to select
the bandpass. A photomultiplier tube with a quartz window
and a S-20 spectral response is used in the DC mode for
measurements from 200 nm to 900 nm. A lead
sulfide photodiode is used the AC mode for measurements
from 800 nm to 2400 nm. The spectral radiance
spot size is a 0.6 mm by 0.8 mm rectangle.
- The radiance temperature of the variable-temperature
blackbody (VTBB), transfer standard, is determined by
comparison to the working standard. The spectral radiance
of the VTBB is calculated using Eq. (1). The
blackbody operates between 900 K and 2700 K
with a 2-mm diameter opening and an estimated emissivity
of 0.999.
- The spectral radiance of the test source from 225 nm
to 2400 nm is determined by comparison to the
variable-temperature blackbody.
Spectral Irradiance Scale
Realization
To realize the spectral irradiance scale, the spectral
radiance of an integrating sphere source (ISS) is determined by
comparison to the variable-temperature blackbody.
- An integrating sphere is used as the spectroradiometer
input optics for spectral irradiance measurements. A
barium sulfate (BaSO4) coated sphere is used
for the deuterium arc lamp measurements and a
polytetrafluoroethylene (PTFE) coated sphere is used for
the tungsten lamp measurements.
- The spectral irradiance of the ISS is calculated by
multiplying the spectral radiance of the ISS by a
geometrical factor.
- The spectral irradiance of the primary working standards
(PWS) is determined by comparison to the ISS. A group of
1000-watt quartz-halogen lamps are the primary working
standards.
- For the spectral range from 250 nm to 2400 nm,
the spectral irradiance of the test source is compared to
the PWS.
- The relative spectral irradiance of the deuterium working
standards (D2WS) is determined by comparison to an argon
mini-arc. A group of 30-watt deuterium arc lamps are the
deuterium working standards.
- For the spectral range from 200 nm to 240 nm,
the spectral irradiance of the test source is compared to
the D2WS.
Spectroradiometric Source
Calibration Services
- NIST calibrates and issues a
type 30A/T24/13 ribbon filament lamp with a mogul bi-post
base.
Test No. |
Measurement Description |
39010C |
Spectral Radiance Standard, Ribbon
Filament Lamp (225 nm to 2400 nm) |
39020C |
Spectral Radiance Standard, Ribbon
Filament Lamp (225 nm to 800 nm) |
39030C |
Spectral Radiance Standard, Ribbon
Filament Lamp (650 nm to 2400 nm) |
-
Spectral irradiance
calibrations are performed at 50 cm.
NIST calibrates and issues
an 1000-watt, quartz halogen lamp mounted in a medium
bi-post base.
-
Test No. |
Measurement Description |
39040C |
Spectral Irradiance Standard, 1000-watt
Quartz Halogen Lamp (250 to 1600 nm) |
39045C |
Spectral Irradiance Standard, 1000-watt
Quartz Halogen Lamp (250 to 2400 nm) |
-
NIST calibrates and issues a
30-watt, deuterium arc lamp mounted in a medium bi-post
base.
-
Test No. |
Measurement Description |
39050C |
Spectral Irradiance Standard, 30-watt
Deuterium Arc Lamp (200 nm to 400 nm) |
39060S |
Special Tests of Radiometric Sources |
Calibration Uncertainties
- The expanded uncertainty (coverage factor k = 2) is a
two standard deviation estimate.
Standard |
Wavelength
(nm) |
Typical
values |
Relative
Expanded Uncertainty |
Ribbon filament lamp |
225
250
350
655
900
1600
2400 |
5.5 W cm-3
sr-1
1.3 x 105
4.0 x 104
|
1.5
1.3
1.0
0.6
0.6
0.5
0.4 |
Quartz halogen lamp |
250
350
655
900
1600
2400 |
0.2 W cm-3
170
40
|
1.8
1.1
0.9
1.1
1.4
4.4 |
Deuterium arc lamp |
200
250
400 |
0.5 W cm-3
0.3
0.05 |
5.0
3.2
3.2 |
This laboratory's quality system is based on the ANSI/NCSL
Z540-1-1994 standard and the ISO/IEC Guide 25.
How to Request Spectroradiometric Source Calibration
Services
- Prepare a purchase order with the following:
- Company name and address
- Contact person's name and phone number.
- Billing address
- Service ID number requested (include range and
points)
- Test fee
- Address to ship test item
- Return shipping instructions (prepay and add,
COD, charge to account with shipper)
- the test fee does not include shipping
costs
- customers are responsible for all
shipping costs
- If no instructions are given, NIST will
return the test item by common carrier,
collect, and uninsured.
- Send the purchase order to:
- National Institute of Standards and
Technology
- Calibration Program
- Building 820, Room 232
- Gaithersburg, MD 20899-0001
-
- Tel.: (301) 975-2002
- FAX: (301) 869-3548
- E-mail: calibrations@enh.nist.gov.
- Send the test item(s) to:
- Charles Gibson
- NIST
- Building 221 / Room B208
- Gaithersburg, MD 20899-0001
-
- Tel.: (301) 975-2329
- FAX: (301) 869-5700
- E-mail: cgibson@nist.gov.
Spectroradiometric source calibrations are performed in March,
June, September, and December. Requests for calibration services
are scheduled after the receipt of a purchase order.
NIST policy requires prepayment of all calibration services
performed for non-U.S. organizations. Please contact the
Calibration Program Office to arrange payment.
Groups supported by this calibration service
- Aerospace industry
- Lighting manufacturers
- Measurement equipment and other instrumentation
manufacturers
- NASA
- National standards laboratories
- Photographic equipment manufacturers
- Research universities
- Solar UV monitoring community
- US military service calibration laboratories
Radiometric Measurements References
Spectroradiometric Determination of the Freezing Temperature of Gold,
K. D. Mielenz, R. D. Saunders and J. Shumaker, J. Res. Natl. Inst. Stand.
Technol., Vol. 95 (Jan-Feb. 1990).
The International Temperature Scale of 1990 (ITS-90), H. Preston-Thomas,
Metrologia 27, 2-310 (1990).
NBS Measurement Services: The NBS Photodetector Spectral Response Calibration
Transfer Program,E. F. Zalewski, Natl. Bur. Stand. (U.S.), Spec. Publ. 250-17
(1988).
NBS Measurement Services: Spectral Irradiance Calibrations, J. H. Walker,
R. D. Saunders, J. K. Jackson, and D. A. McSparron, Natl. Bur. Stand. (U.S.),
Spec. Publ. 250-20 (Sept. 1987).
NBS Measurement Services: Spectral Radiance Calibrations, J. H. Walker,
R. D. Saunders, and A. T. Hattenburg, Natl. Bur. Stand. (U.S.), Spec. Publ.
250-1 (Jan. 1987).
Spectral Response Self-Calibration and Interpolation of Silicon Photodiodes,
J. Geist, E. F. Zalewski, and A. R. Schaefer, Appl. Opt. 20, 3795 (1980).
Spectral Irradiance Standard for the Ultraviolet: The Deuterium Lamp,
R. D. Saunders, W. R. Ott, and J. M. Bridges, Appl. Opt. 17, 593 (1978).
The 1973 NBS Scale of Spectral Irradiance, R. D. Saunders and J. B. Shumaker,
Natl. Bur. Stand. (U.S.), Tech. Note 594-13 (1977).
Spectral Radiometry: A New Approach Based on Electro-Optics, J. Geist,
M. A. Lind, A. R. Schaefer, and E. F. Zalewski, Natl. Bur. Stand. (U.S.),
Tech. Note 954 (1977).
Fundamental Principles of Absolute Radiometry and the Philosophy of This NBS
Program (1968 to 1971), J. Geist, Natl. Bur. Stand. (U.S.), Tech. Note 594-1
(1972).
High-Accuracy Spectral Radiance Calibration of Tungsten-Strip Lamps,
H. J. Kostkowski, D. E. Erminy, and A. T. Hattenburg, Adv. Geophys. 14,
111 (1970).
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