Civil Engineering Reference
In-Depth Information
monoclinic VO
2
(B) (Théobald
et al.
, 1976), paramontroseite VO
2
(Wu
et al.
,
2008) and body centred cubic VO
2
(Wang
et al.
, 2008). The interesting ther-
mochromic properties ensue from VO
2
(R) and VO
2
(M) which exhibit a
reversible structural transformation and associated metal-insulator transi-
tion at a 'critical' temperature
τ
c
in the neighbourhood of a comfort tem-
perature; VO
2
(M) is semiconducting and reasonably infrared transparent
at a temperature
τ
, so that
τ
<
τ
c
, whereas VO
2
(R) is metallic and infrared
refl ecting for
τ
c
.
The pioneering work on the thermochromism of VO
2
by Morin (1959)
was performed on bulk specimens. However, it was soon realized that reac-
tively sputter deposited and reactively evaporated thin fi lms could exhibit
a similar metal-insulator transition. Subsequently it has been found that
virtually any thin fi lm technology is capable of providing thermochromic
VO
2
. The reversibility of the metal-insulator transition can be excellent in
fi lms (Ko and Ramanathan, 2008), whereas bulk samples tend to deteriorate
upon repeated thermal cycling around
τ
>
τ
c
. The possibilities to create energy-
effi cient fenestration by letting solar energy into a building when there is a
heating demand and rejecting solar energy when there is a cooling demand
were pointed out already in the 1980s (Greenberg, 1983; Jorgenson and Lee,
1986; Babulanam
et al.
, 1987), and various aspects of this technology have
been reviewed several times more recently (Granqvist, 2007; Parkin
et al.
,
2008; Saeli
et al.
, 2010a,b; Smith and Granqvist, 2010).
Figure 11.6 introduces the characteristic features of the thermochromism
that can be seen in a thin VO
2
fi lm. Spectral normal transmittance
T
(
λ
) and
spectral near-normal refl ectance
R
(
λ
) were recorded at 22 and 100°C, i.e.,
at
m-thick fi lm pro-
duced by reactive dc magnetron sputtering as reported elsewhere by Mlyuka
et al.
(2009a). Similar optical data - usually of spectral transmittance - have
been reported many times in the scientifi c literature and are hence very
well established (see the paper by Li
et al.
(2012) for references). It is clear
from Fig. 11.6 that the short-wavelength optical properties are similar irre-
spective of the temperature, while the infrared refl ectance for wavelengths
beyond
τ
<
τ
c
and at
τ
>
τ
c
. The data were obtained for a 0.05-
μ
τ
c
, thus giving proof for
the metal-insulator transition. The infrared transmittance at
∼
1
μ
m is higher for
τ
>
τ
c
than it is for
τ
<
λ
>
1
μ
m shows
an analogous change.
Figure 11.6 also shows the spectral sensitivity of the light-adapted human
eye, denoted
m wavelength range
(Wyszecki and Stiles, 2000) and the solar irradiance spectrum for air mass
1.5 (corresponding to the sun standing 37° above the horizon), denoted
ϕ
lum
and lying in the 0.4
<
λ
<
0.7
μ
ϕ
sol
and extending across the 0.3
<
λ
<
3
μ
m interval (ASTM, 2003). One
observes in particular that
ϕ
sol
drops sharply towards long wavelengths.
Wavelength-integrated luminous and solar transmittance values are now
introduced by
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