- Page 1 and 2: NEWRAD PROCEEDINGS OF THE 9 TH INTE
- Page 3 and 4: NEWRAD 2005 Scientific Program Day
- Page 5 and 6: 14:50 Hiroshi Shitomi, AIST 5-3 Pho
- Page 7 and 8: NEWRAD 2005 Scientific Program-Post
- 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 19: Reflecting Cavity Blackbodies for R
- Page 22 and 23: whole CCD in the range (460 nm - 70
- Page 24 and 25: off the back end of the cavity. The
- Page 26 and 27: Transimpedance amplifier Digital-vo
- Page 29: PULSED UV SPECTRORADIOMETRY WITH TH
- Page 32 and 33: Detector stage Figure 1. Schematic
- Page 35: Experimental study of application o
- Page 38 and 39: UV-VUV branch The design is not yet
- Page 41 and 42: Energy Calorimeter for Pulsed Laser
- Page 43 and 44: Characterization of new trap detect
- Page 45 and 46: Measurement of Small Aperture Areas
- Page 47 and 48: Low-Background Temperature Calibrat
- Page 49: Cryogenic Radiometers and Absolute
- Page 52 and 53: terms of the illuminance responsivi
- Page 55: WRR to SI intercomparisons 1991 - 2
- 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
- Page 98 and 99:
el. spectral distribution 1 0,8 0,6
- Page 100 and 101:
3.5 Radiometric spectra 780-3000nm
- Page 102 and 103:
Results The corrections required fo
- Page 104 and 105:
the second term, containing the sec
- Page 106 and 107:
OTDR but also a commercial spectral
- Page 108 and 109:
temperature and the spectral emissi
- Page 110 and 111:
110
- Page 112 and 113:
Although the optical quality, unifo
- Page 114 and 115:
we have proven that field uniformit
- Page 116 and 117:
116
- Page 118 and 119:
Daily Avg / Weekly Mean Figure 1. T
- Page 120 and 121:
1.2 Spectral irradiance (W/cm 3 ) 1
- Page 122 and 123:
coupling photometric and radiometri
- Page 124 and 125:
the Broadband Calibration Chamber (
- Page 126 and 127:
FTIR Mode Further spectral capabili
- Page 128 and 129:
128
- Page 130 and 131:
Results The procedure described bef
- Page 132 and 133:
lackbody, with the aim of investiga
- Page 134 and 135:
The top design is the traditional o
- Page 136 and 137:
Figure 2. The ratio of the irradian
- Page 138 and 139:
138
- Page 140 and 141:
however, recently demonstrated that
- Page 142 and 143:
142
- Page 144 and 145:
144
- Page 146 and 147:
146
- Page 148 and 149:
et al. 3 References 1. G. Xu and X.
- Page 150 and 151:
150
- Page 152 and 153:
(XPS): Overview and Calibrations,
- Page 154 and 155:
and Aqua MODIS have been consistent
- Page 156 and 157:
performance. We plan to measure the
- Page 158 and 159:
the purpose of creating highly stab
- Page 160 and 161:
over all bands. ROLO Lunar Calibrat
- Page 162 and 163:
To characterize the spectral depend
- Page 164 and 165:
erties of detectors (with different
- Page 166 and 167:
166
- Page 168 and 169:
168
- Page 170 and 171:
than 0.25%. Also addressed in this
- Page 172 and 173:
directed to the Sun give reference
- Page 174 and 175:
version. The noise N (expressed in
- Page 176 and 177:
176
- Page 178 and 179:
178
- Page 180 and 181:
180
- Page 182 and 183:
are seen in Figure 2. We note that
- Page 184 and 185:
184
- Page 186 and 187:
3. Integrating sphere The determina
- Page 188 and 189:
These standards match in an ideal w
- Page 190 and 191:
tiles, a matte opal glass and a spr
- Page 192 and 193:
Relative Signal 1.0E+01 1.0E+00 1.0
- Page 194 and 195:
The uncertainty budget for calibrat
- Page 196 and 197:
For all of the analysed reflection
- Page 198 and 199:
198
- Page 200 and 201:
200
- Page 202 and 203:
of the lamp housing (halogen lamp)
- Page 204 and 205:
Current in Photometer / A 3,675E-07
- Page 206 and 207:
In radiometry absolute standards ar
- Page 208 and 209:
208
- Page 210 and 211:
Spectral reflectance The reflectanc
- Page 212 and 213:
distances d were measured from the
- Page 214 and 215:
ÔÓØÓÒ ÔÖ× Ò ×ÐØÐÝ Ò
- Page 216 and 217:
visible measurements this is usuall
- Page 218 and 219:
some gold-black coatings. No measur
- Page 220 and 221:
in,max P mum available input power
- Page 222 and 223:
The time constant of the detector h
- Page 224 and 225:
correction factor for the current v
- Page 226 and 227:
The source radiance and power reach
- Page 228 and 229:
wavelengths can be tuned from 790 n
- Page 230 and 231:
The following represents a calculat
- Page 232 and 233:
232
- Page 234 and 235:
Discussion process The participants
- Page 236 and 237:
The measured spectra are kept anony
- Page 238 and 239:
Fig. 2), spatial uniformity of the
- Page 240 and 241:
98% was used for the measurements i
- Page 242 and 243:
were 45 mm diameter discs of approx
- Page 244 and 245:
Helm (Glasgow 2000) James & James (
- Page 246 and 247:
crucible material. Nominal purities
- Page 248 and 249:
248
- Page 250 and 251:
A new BB3500YY furnace (manufacture
- Page 252 and 253:
(9) were identical (T D = 3112.7 K)
- Page 254 and 255:
It uses two mirror arrays, opticall
- Page 256 and 257:
very similar temperature distributi
- Page 258 and 259:
aligned to the center of this apert
- Page 260 and 261:
presented, the ARS generates the sp
- Page 262 and 263:
Figure 2 shows (on a logarithmic sc
- Page 264 and 265:
uncertainty component was estimated
- Page 266 and 267:
Linearity factor 1 0.98 0.96 0.94 0
- Page 268 and 269:
268
- Page 270 and 271:
VTBB, BB29Ga, and BB156In with 100
- Page 272 and 273:
Figure 2. Layout of the measurement
- Page 274 and 275:
As the correction for atmospheric a
- Page 276 and 277:
principle achieve better accuracy,
- Page 278 and 279:
Comparing curves 5 and 6 shows that
- Page 280 and 281:
for smelting under vacuum are prese
- Page 282 and 283:
∂L L( λ, T ) = L( λ0, T ) + ∂
- Page 284 and 285:
Discussion 1 - ε (tot) x 10 -6 Fig
- Page 286 and 287:
20 lamps was below -2 %. Compared t
- Page 288 and 289:
Experiments The profile (full line,
- Page 290 and 291:
these materials. Repeatability of a
- Page 292 and 293:
temperature of the cell. The obtain
- Page 294 and 295:
294
- Page 296 and 297:
1) Select the initial values of pow
- Page 298 and 299:
298
- Page 300 and 301:
Front Plate Field Stop Collimating
- Page 302 and 303:
Figure 1. Then new NPL cavity pyroe
- Page 304 and 305:
304
- Page 306 and 307:
ØØÓÖ Ó Ø ×ÔØÖÓÑØÖ Ò
- Page 308 and 309:
Table 1: Uncertainties in the calib
- Page 310 and 311:
310
- Page 312 and 313:
elies on the use of a pyroelectric
- Page 314 and 315:
filters with 4⋅ 10 -6 nm/K therma
- Page 316 and 317:
spectrometer BOMEM DA3 is not neces
- Page 318 and 319:
(nA/lx) (nA/lx) (%) (%) 9,568 9,590
- Page 320 and 321:
4 Unit transfer As a typical applic
- Page 322 and 323:
Results The gloss standard used in
- Page 324 and 325:
324
- Page 326 and 327:
if the measurement range of KRISS i
- Page 328 and 329:
The design of the graphite crucible
- Page 330 and 331:
Istanbul, 2001. 330
- Page 332 and 333:
esponsivity of trap detector with e
- Page 334 and 335:
Thornagel, R., Ulm, G., Metrologia,
- Page 336 and 337:
The commercial radiometers were sel
- Page 338 and 339:
where y test (λ) is the detector s
- Page 340:
incorporate a monochromator to allo