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NEWRAD PROCEEDINGS OF THE 9 TH INTE
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NEWRAD 2005 Scientific Program Day
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- Page 9 and 10: 33. Drift in the absolute responsiv
- Page 11 and 12: Session 6 Novel Techniques 64. The
- Page 13: Session 9 Realisation of scales 94.
- Page 17: Absolute Accuracy of Total Solar Ir
- Page 21 and 22: Low-uncertainty absolute radiometri
- Page 23 and 24: NIST Reference Cryogenic Radiometer
- Page 25 and 26: Measurement of the absorptance of a
- Page 27: Grooves for Emissivity and Absorpti
- Page 31 and 32: New apparatus for the spectral radi
- Page 33: VUV and Soft X-ray metrology statio
- Page 37 and 38: The metrology line on the SOLEIL sy
- Page 39: Cryogenic radiometer developments a
- Page 42 and 43: measured with BiTe thermopiles. Exp
- Page 44 and 45: variations of the spectral sensitiv
- Page 46 and 47: aperture area by I = π·L·F·A, w
- Page 48 and 49: Table 1 Ratio of radiometric power
- Page 51 and 52: Consistency of radiometric temperat
- Page 53: Project of absolute measuring instr
- Page 59 and 60: QA/QC of Spectral Solar UV irradian
- Page 61 and 62: NEWRAD 2005 The Metrology Light Sou
- Page 63 and 64: NEWRAD 2005 Fractional self-calibra
- Page 65 and 66: Temperature effects of PTFE diffuse
- Page 67 and 68: Characterization of Photoconductive
- Page 69 and 70: The UV Spectral Responsivity Scale
- Page 71 and 72: Operational mode uncertainty for br
- Page 73 and 74: A method of characterizing narrow-b
- Page 75 and 76: Development of a Versatile Radiomet
- Page 77 and 78: Nonlinearity Measurement of UV Dete
- Page 79 and 80: Radiometric investigation of a comp
- Page 81 and 82: Accurate and independent spectral r
- Page 83 and 84: NEWRAD 2005: Characterization of de
- Page 85 and 86: NEWRAD 2005: Preparing Final Camera
- Page 87 and 88: NEWRAD 2005: Preparing Final Camera
- Page 89: Calibration of Space Instrumentatio
- Page 92 and 93: Vibrational Spectroscopy Vol. 1, J.
- Page 94 and 95: characteristic, both the correction
- Page 96 and 97: different wavelengths with that fro
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- Page 100 and 101: 3.5 Radiometric spectra 780-3000nm
- Page 102 and 103: Results The corrections required fo
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OTDR but also a commercial spectral
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temperature and the spectral emissi
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Although the optical quality, unifo
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we have proven that field uniformit
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Daily Avg / Weekly Mean Figure 1. T
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1.2 Spectral irradiance (W/cm 3 ) 1
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coupling photometric and radiometri
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the Broadband Calibration Chamber (
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FTIR Mode Further spectral capabili
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Results The procedure described bef
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lackbody, with the aim of investiga
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The top design is the traditional o
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Figure 2. The ratio of the irradian
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however, recently demonstrated that
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et al. 3 References 1. G. Xu and X.
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(XPS): Overview and Calibrations,
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and Aqua MODIS have been consistent
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performance. We plan to measure the
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the purpose of creating highly stab
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over all bands. ROLO Lunar Calibrat
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To characterize the spectral depend
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erties of detectors (with different
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than 0.25%. Also addressed in this
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directed to the Sun give reference
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version. The noise N (expressed in
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are seen in Figure 2. We note that
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3. Integrating sphere The determina
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These standards match in an ideal w
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tiles, a matte opal glass and a spr
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Relative Signal 1.0E+01 1.0E+00 1.0
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The uncertainty budget for calibrat
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For all of the analysed reflection
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of the lamp housing (halogen lamp)
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Current in Photometer / A 3,675E-07
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In radiometry absolute standards ar
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Spectral reflectance The reflectanc
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distances d were measured from the
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ÔÓØÓÒ ÔÖ× Ò ×ÐØÐÝ Ò
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visible measurements this is usuall
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some gold-black coatings. No measur
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in,max P mum available input power
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The time constant of the detector h
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correction factor for the current v
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The source radiance and power reach
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wavelengths can be tuned from 790 n
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The following represents a calculat
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232
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Discussion process The participants
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The measured spectra are kept anony
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Fig. 2), spatial uniformity of the
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98% was used for the measurements i
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were 45 mm diameter discs of approx
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Helm (Glasgow 2000) James & James (
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crucible material. Nominal purities
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248
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A new BB3500YY furnace (manufacture
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(9) were identical (T D = 3112.7 K)
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It uses two mirror arrays, opticall
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very similar temperature distributi
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aligned to the center of this apert
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presented, the ARS generates the sp
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Figure 2 shows (on a logarithmic sc
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uncertainty component was estimated
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Linearity factor 1 0.98 0.96 0.94 0
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268
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VTBB, BB29Ga, and BB156In with 100
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Figure 2. Layout of the measurement
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As the correction for atmospheric a
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principle achieve better accuracy,
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Comparing curves 5 and 6 shows that
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for smelting under vacuum are prese
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∂L L( λ, T ) = L( λ0, T ) + ∂
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Discussion 1 - ε (tot) x 10 -6 Fig
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20 lamps was below -2 %. Compared t
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Experiments The profile (full line,
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these materials. Repeatability of a
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temperature of the cell. The obtain
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1) Select the initial values of pow
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298
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Front Plate Field Stop Collimating
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Figure 1. Then new NPL cavity pyroe
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304
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ØØÓÖ Ó Ø ×ÔØÖÓÑØÖ Ò
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Table 1: Uncertainties in the calib
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310
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elies on the use of a pyroelectric
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filters with 4⋅ 10 -6 nm/K therma
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spectrometer BOMEM DA3 is not neces
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(nA/lx) (nA/lx) (%) (%) 9,568 9,590
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4 Unit transfer As a typical applic
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Results The gloss standard used in
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324
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if the measurement range of KRISS i
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The design of the graphite crucible
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Istanbul, 2001. 330
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esponsivity of trap detector with e
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Thornagel, R., Ulm, G., Metrologia,
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The commercial radiometers were sel
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where y test (λ) is the detector s
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incorporate a monochromator to allo