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HAL Id: jpa-00229493

https://hal.archives-ouvertes.fr/jpa-00229493

Submitted on 1 Jan 1989

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THERMAL TRANSPORT IN MONOLITHIC SILICA AEROGEL

R. Caps, G. Döll, J. Fricke, U. Heinemann, J. Hetfleisch

To cite this version:

R. Caps, G. Döll, J. Fricke, U. Heinemann, J. Hetfleisch. THERMAL TRANSPORT IN MONO- LITHIC SILICA AEROGEL. Journal de Physique Colloques, 1989, 50 (C4), pp.C4-113-C4-118.

�10.1051/jphyscol:1989417�. �jpa-00229493�

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R E W E DE PHYSIQUE APPLIQUEE

Colloque C4, Suppl6ment au n04, Tome 24, a v r i l 1989

THERMAL TRANSPORT IN MONOLITHIC SILICA AEROGEL

R. CAPS, G. DOLL, J. FRICKE, U. HEINEMANN and J. HETFLEISCH

Physikalisches Institut der Universitdt, Am Hubland, D-8700 ~iirzburg, F.R.G.

Resume : Des rnesures sur le transport therrnique dans des briques d'a6rogels de sillce (Bpaisseur volslne de 8 mm) ont QB rBalis6es pour deux densites (p = 110 et 270 Kg.m-3) et pour des 6missivk6~ = 0.04 et 0,77 dans I'alr et sous vide. Canalyse est rBalisBe dans un intervalle de temperature cornpris entre 100 et 650°K. De plus pour une .densit6 de 70 Kg.rn-' les pertes therrniques ont Bt6 d6terminbes pour deux bpaisseurs (I'une &ant le double de I'autre). Pour bien interprbter les rbsultats nous avons r6aIisB des mesures de transmission IR radiative en fonction de la longueur d'onde. L'Bvaluation des donnBes suit les rnQhodes dBveloppBes pour les materiaux optiques de faible Bpaisseur et transparents.

Abstract

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Measurements on t h e thermal t r a n s p o r t i n SiO, a e r o g e l t i l e s ( t h i c k n e s s about 8 mm) were performed f o r two d e n s i t i e s ( p = 110 kg-m-' and 270 kgom-'), f o r e m i s s i v i t i e s & = 0.04 and 0.77, i n a i r and evacuated. The covered temperature range was 100 K t o 650 K. I n a d d i t i o n f o r d e n s i t y p = 70 kg.m-' t h e thermal l o s s e s were determined f o r two t h i c k n e s s e s ( d i f f e r i n g by a f a c t o r of two). For proper i n t e r p r e - t a t i o n wavelength dependent IR r a d i a t i v e transmission measurements were peqfomed.

Data e v a l u a t i o n proceeded along t h e methods developed f o r o p t i c a l l y t h i n , non-grey m a t e r i a l s .

1

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INTRODUCTION

I n h i g h l y porous a e r o g e l s h e a t is t r a n s f e r r e d v i a i n f r a r e d (IR) r a d i a t i o n and s o l i d conduction along t h e f r a g i l e Si0,-skeleton. For non-evacuated specimens i n a d d i t i o n gaseous thermal conduction occurs. A s a l r e a d y K i s t l e r 111 knew, t h e l a t t e r c o n t r i b u t i o n is conside- r a b l y s m a l l e r than would be expected f o r a f r e e non-convecting gas. I n e a r l i e r papers / 2 , 3 / we have pointed out t h a t a e r o g e l s a r e o p t i c a l l y t h i n m a t e r i a l s i n l a y e r s of 10

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20 mm which

a r e t y p i c a l t h i c k n e s s e s f o r window a p p l i c a t i o n s . An important consequence is t h a t t h e thermal c o n d u c t i v i t y depends on t h i c k n e s s and boundary e m i s s i v i t y , and t h u s is not a m a t e r i a l property. I n a e r o g e l s t h e I R r a d i a t i v e e x t i n c t i o n , is provided by a b s o r p t i o n

hot side rel. position x cold side

Fig.1. Temperature p r o f i l e s for, a grey medium with o p t i c a l t h i c k n e s s r, = 4 and boundary e m i s s i v i t y & = 0.05 f o r d i f f e r e n t r a t i o s N I of s o l i d conduction t o r a d i a t i v e h e a t t r a n s f e r 141.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:1989417

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(scattering only occurs in the visible spectral region). The absorption coefficient strongly depends on wavelength. Therefore an extremely complex interaction between solid conduction and IR heat transport occurs. In general under these conditions one expects a temperature gradient which is steep close to the low emissivity boundaries and rather flat within the bulk (fig.1).

2

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THEORETICAL REMARKS

In optically thin insulations the heat transfer for combined radiation and conduction is described by an integro-differential equation. This was performed recently by G. Doll 151.

It is very tedious to solve the exact equation numerically for a non-grey medium as aerogel, where the optical thickness T,(A) is a function of wavelength. Therefore the simplest way is to generalize an approximate three-flux solution for grey media to non-grey media 161.

Instead of the constant optical thickness TO one uses its spectral value rO(A) and integrates the heat flux over the thermal spectrum with the Rosseland distribution

&,(T)/ae,(T) as a weight factor (e,,(T) being the spectral and e,(T) = UT4 the total blackbody emissive power).

3

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EXPERIMENTAL SET-UP

The caloric data were derived with the evacuable, load-controlled guarded hot plate system LOLA I (fig.2). A special cylindric guard (temperature controlled) allows to cover an unusually large temperature range (T = 100 to 900 K3. The size of the specimens was 20 cm 0.

Infrared transmission between 2.5 and 45

urn

was measured with a fast FTIR spectrometer. A typical IR transmission spectrum is shown in fig.3. Clearly visible is the large extinction above 10

urn

and the very small extinction between 3 and 5 um.

LOLA 3

1 vacuum chamber a. upper part b. middle part c. lower part

2 hot plate with two guard-rings 3 upper cold plate

4 lower cold plate 5 tested specimen 6 heat sinks

7 cylindric guard (temperature controlled) 8 high-temperature insulation

9 ceramic support 10 pistons

11 ground pldte 12 flange fo'q pumps 13 small flanges 14 sensor for thickness 15 fluid pipes

Fig.2. Guarded hot plate apparatus LOLA P, which can be evacuated and externally pressure loaded. The metering section is 12 cm 0.

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10 wavelength

I I I

2 10 50

wavelength /pm

Fig.3. Specific extinction coefficient e versus wavelength a) for hydrophilic, b) for hydrophobic aerogel.

4

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RESULTS AND DISCUSSION

From the temperature difference AT = T,

-

T, = 30 K across the specimen and the power input per unit area P / A the thermal transfer coefficient A can be derived according to

P / A = 2.A.AT

.

The factor 2 takes care of the double-sided measurements. In all plots shown

A is depicted versus third power of mean temperature for radiation T,.

From fig.4a it is evident that optically thin specimens are investigated: A doubling of thickness d only reduces A marginally, while with optically thick insulations a reduction of A by a factor of 2 would be expected. This holds down to temperatures of about 150 K (fig.4b1, where the measured 14.2 mm-curve is about one half of the 7.4 mm curve. The extraordinary large influence of surface emissivity E on A (see fig.5) is another proof for the small optical thickness of the investigated aerogel tiles in the IR. This effect again shows down to about 150 K. One should point out, that above T, = 350 K the differences in A for low and high emissivities are clearly visible even for non-evacuated specimens.

Fig.4. Thermal transfer coefficient A versus T," for aerogel tiles ( p = 70kg.m-a) with thicknesses d = 7.4 (-) and 14.2 mm (---); a) temperature range I00 K

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670 K,

b) temperature range 100 K

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300 K.

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R E W E DE PHYSIQUE APPLIQUEE

Fig.5. Thermal transfer coefficient A versus Tr3 for an aerogel tile with p = 110 kg-m-', d = 7.6 mm; parameter is boundary emissivity E ; data for evacuated and non-evacuated specimens are shown.

Fig. 6. Thermal transfer coefficient versus TC3 for two tiles with different densities.

a) With E = 0.77 the expected curve crossing is clearly to be seen, b) with c = 0.04 non-linear coupling between radiation and conduction masks this effect.

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Another important quantity influencing the thermal transport is the aerogel density. It is plausible that at low temperatures, where solid conduction gives the major contribution, A is larger for higher densities. With rising temperature more and more IR radiation is emitted. For high emissivitiy boundaries heat transfer then is governed by the aerogel IR extinction properties, leading to lower A-values for higher densities (see fig.6a). For lower emissivities the situation is not as clear: Though an increasing density increases the IR extinction, non-linear coupling effects close to the low emissivity boundaries mask this effect, possibly leading to higher A-values for higher densities (fig.6b).

In order to study the influence of the gas (Nz) on the thermal transport, the transfer coefficients with air La,,, and for evacuated specimens A,,,,, are subtracted from each other. In a naiv consideration one would expect this difference to be determined by the free Nz conductivity (AN(300 K)

*

0.026 W-m-l.K-l), corresponding to a value ka, s 3.5 W.m-*.K-' for d = 7.6 mm. Firstly we recognize from fig.7 that we get A,,,,,

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,&, 2 1 W.m-2.K-1 for E = 0.77 over the whole temperature range investigated. This small contribution can be explained by the microporous aerogel structure, in which gas conduction is only partially developed even at ambient pressure 171. For & = 0.04 the difference

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&,&, is larger

and shows a strong temperature dependence. The reason again is the non-linear coupling between radiative transport and conduction (caused by the skeleton and the gas) within the radiative boundary layer in front of the ~ o w - E - S U ~ ~ ~ C ~ S .

Fig.7. Difference of thermal transfer coefficients for non-evacuated and evacuated tiles versus T.', The dramatic increase in Ae,t.r

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h,,, with temperature for low emissivity boundaries is caused by the non-linear coupling between radiation and conduction.

In order to evaluate the solid conductivity in aerogels as a function of density we tried to extend the measurements to as low temperatures as possible (fig.8). Below 150 K the influ- ence of E on A vanishes, indicating that the specimens become optically thick. If we neglect the radiative contributions we can derive upper values for the solid conductivities A,, for 150 K: For the 70 and 110 kg.md3 tiles a value A,, = 0.003 W*m-l.K-l and for the 270 kgarn-a tile h, a 0.01 W.m-l*K-' is estimated. These values have to be compared with A

,

, = 1 W*m-'.K-l for fully dense silica glass. These large discrepancies can be explained in terms of the density ratios (2200:70 and 2200:270) and the sound velocity ratios

(5000:120 and 5000:340).

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Fig.8. Low temperature behaviour of thermal transfer coefficient versus T', for 3 densities and 2 emissivities. At the lowest temperatures achieved, the dominant component ought to be solid conduction.

Acknowledgement:

This work was supported by the German Bundesminister fiir Forschung u. Technologie (BMFT). We would like to thank Dr. G. Poelz / DESY, Hamburg and DR. S. Henning / Airglass AB Staffanstorp, Sweden for generously providing aerogel tiles.

REFERENCES

/ I / Kistler S.S., Nature 127, 741 (1931)

/2/ Caps, R., Trunzer, A., Buttner, D. and Fricke, J., Int. J. Heat Mass Transfer 27, 1865 (1984)

/3/ Caps, R. and Fricke, J., Aerogels, Springer Proc. in Physics 5 , 104 (1986)

/4/ Scheuerpflug, P,, Caps, R., Buttner, D. and Fricke, J., Int. J. Heat Mass Transfer 2 8 , 2299 (1985)

/5/ Doll, G., Diplome Thesis, Report E12-0987-1 (19871, Physikalisches Institut der Universitat, D-8700 Wirzburg (unpublished)

/ 6 / Fricke, J., Caps, R., Hummer, E., Doll, G., Arduini, M.C. and De Ponte, F., ASTM C16 Meeting, Bal Harbour Florida (1987)

/7/ Biittner, D., Caps, R., Heinemann, U . , Hummer, E., Kadur, A. and Fricke, J., Solar Energy 40, 13 (1988)

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