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VTBB, BB29Ga, and BB156In with 100 K to 1000K<br />

working temperature range, designed for calibration of<br />

spaceborne IR sensors and high-precision radiometry at<br />

such research organizations as German Aerospace Center<br />

(DLR) and Physikalisch-Technische Bundesanstalt<br />

(Germany), National Physical Laboratory (UK), Space<br />

Dynamics Lab (USA), NIM and IAO (China).<br />

Cavity-type BB100-V1 as a source of thermal radiation<br />

features a series of advantages over any other thermal<br />

sources – such as high reproducibility, low sensitivity of its<br />

effective emissivity to variations and degradation of optical<br />

properties of its cavity inner surface.<br />

Low-temperature and cryogenic BB100-V1 is build up<br />

on the principles of the usage of external liquid-based<br />

thermostat LAUDA Proline PR1845-LCK1891 with<br />

circulating coolant KRYO-51 in a closed loop.<br />

As a material of radiating cavity for low-temperature<br />

and cryogenic BB one can use copper and aluminum alloys.<br />

The necessary value of emissivity was obtained with the<br />

usage of black cover paints, e.g. Chemglaze Z-302 for<br />

BB29gl blackbody or Nextel Velvet 811-21 for BB100 /<br />

BB100-V1 radiation sources. While identifying<br />

appropriate coating for BB-100V1 bottom possessing<br />

emissivity better 0.9 in the spectral range of interest (see<br />

Fig. 1), the Nextel Velvet Coating 811-21 was chosen by<br />

ourselves after comparative analysis of several<br />

comprehensive reviews [e.g., 4] on application and optical<br />

properties of black paints and various coatings to stray<br />

light suppressing, solar energy absorbing, for thermal<br />

detectors of optical radiation, radiation losses control, etc.<br />

Emissivity<br />

0.990<br />

0.985<br />

0.980<br />

0.975<br />

0.970<br />

0.965<br />

0.960<br />

0.955<br />

0.950<br />

0.945<br />

0.940<br />

[10]<br />

[11]<br />

[12]<br />

0.935<br />

0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15<br />

Wavelength (ì m)<br />

Figure 1.<br />

Spectral emissivity of Nextel Velvet Coating 811-21<br />

It is enough to assume that the spectral hemispherical<br />

emissivity of Nextel 811-21 is within 0.935…0.990<br />

interval for wavelength range from 1.5 to 15 μm. The<br />

measurements of reflectance performed for the predecessor<br />

of Nextel 811-21, the 3M Velvet Black, show the presence<br />

of a small specular component, less than 10% from overall<br />

hemispherical reflectance; the diffuse component of<br />

reflectance has the near-Lambertian BRDF.<br />

The drawing of BB100-V1 design performed with the<br />

account of above-mentioned studies is depicted in Fig. 2.<br />

The computations of the normal effective emissivities<br />

of an isothermal cavity depicted in Fig.2 using STEEP3 [5]<br />

software. We have used the limiting values of wall<br />

emissivity (0.935 and 0.990) and 4 values of wall diffusity.<br />

The results of computations are presented in Table 2.<br />

Figure 2. BB100-V1 cross-section.<br />

Cavity dimensions: 200 mm length x 120 mm diameter.<br />

Table 2.<br />

Normal Effective Emissivity of BB100-V1 Isothermal Cavity<br />

Cavity<br />

Cavity Wall Diffusity<br />

Wall<br />

Emissivity<br />

0.7 0.8 0.9 1.0<br />

0.935 0.9972 0.9976 0.9980 0.9983<br />

0.990 0.9996 0.9996 0.9997 0.9997<br />

The BB100-V1 is currently under testing in<br />

cryo-vacuum chamber. The uncertainty of thermodynamic<br />

temperature reproducibility of BB100-V1 within working<br />

temperature ranges did not exceed 0,5K (1). The<br />

temperature non-uniformity and long-term stability<br />

account for less than 0.1K and 0.1% for 1.5 μm to 15 μm<br />

wavelength region under cryo-vacuum conditions of<br />

medium background environment. The results of these<br />

measurements will be presented in the paper.<br />

References<br />

[1] V.I.Sapritsky, S.P.Morozova, B.E.Lisiansky, S.A.Ogarev,<br />

M.K.Sakharov, M.L.Samoylov, A.S.Panfilov, B.B.Khlevnoy,<br />

V.E.Privalsky The Global Earth Observation System of<br />

Systems (GEOSS) and problems of measuring the radiant<br />

properties of objects of observations . Proceedings of<br />

NEWRAD’2005 (in print).<br />

[2] V.I.Sapritsky, S.A.Ogarev, B.B. Khlevnoy, M.L.Samoylov,<br />

V.B.Khromchenko “Blackbody sources for the range 100 K to<br />

3500K for precision measurements in radiometry and<br />

thermometry“ – in Proceedings of the 8th Symposium on<br />

temperature: its measurement and control in science and<br />

industry. Chicago, IL, U.S.A. October 21-24, 2002.<br />

[3] V.I.Sapritsky, V.B.Khromchenko, S.N.Mekhontsev,<br />

M.L.Samoilov, A.V.Prokhorov, S.A.Ogarev, A.Shumway<br />

“Medium Background Blackbody BB1000”. Conference CD<br />

of CALCON’2000. SDL, Utah, USA, 2000.<br />

[4] Hameury J, Hay B, Filtz J R 2003 Measurement of Infrared<br />

Spectral Directional Hemispherical Reflectance and<br />

Emissivity at BNM-LNE – Paper presented at the Fifteen<br />

Symposium on Thermopysical Properties, June 22-27, 2003,<br />

Boulder, CO, USA<br />

[5] STEEP3, version 1.3. User’s Guide. Virial, Inc., NY, 2000<br />

270

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