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HAL Id: jpa-00205750

https://hal.archives-ouvertes.fr/jpa-00205750

Submitted on 1 Jan 1964

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Improved dielectric films for multilayer coatings and mirror protection

J.T. Cox, H. Hass, J.B. Ramsey

To cite this version:

J.T. Cox, H. Hass, J.B. Ramsey. Improved dielectric films for multilayer coatings and mirror protec- tion. Journal de Physique, 1964, 25 (1-2), pp.250-254. �10.1051/jphys:01964002501-2025000�. �jpa- 00205750�

(2)

IMPROVED DIELECTRIC FILMS FOR MULTILAYER COATINGS AND MIRROR PROTECTION

By

J. T.

COX,

H. HASS and J. B.

RAMSEY,

U. S. Engineer Army Research and Development Laboratories, Fort Belvoir, Virginia, U. S. A.

Résumé. 2014 Ce mémoire contient des données sur les propriétés optiques de couches d’oxydes

de silicium, d’aluminium, de thorium et de zirconium préparées par evaporation. Le domaine de longueur d’onde s’étend de 0,2 03BC à 1,6 03BC. Les couches étaient préparées, soit par chauffage direct

dans l’oxygène à faible pression, soit par bombardement électronique. On décrit quelques appli-

cations : protection des miroirs, surfaces antiréfléchissantes, filtres par réflexion, et surfaces,

servant au contrôle de la température des satellites.

Abstract. 2014 This paper presents data on the

optical

properties of evaporated films of silicon oxide, aluminium oxide, thorium oxide, and zirconium oxide in the wavelength region from 0.2 03BC.

to 1. 6 03BC. The films were prepared by direct heating both in vacuum and in the presence of oxygen, and by electron bombardment. Some of their more important applications such as:

protected front surface mirrors, antireflection coatings, reflection filters, and coatings for controlling

the temperature of satellites in outer space, are described.

JOURNAL DE PHYSIQUE TOME 25, JANVIER-FÉVRIER 1964,

1. Introduction. - For a

long time,

the

designer

of

multilayer

antireflection

coatings

and

protected

front surface mirrors was

seriously hampered by

the fact that the number of dielectric materials suitable for

producing

durable and

nonabsorbing

films

by

direct

evaporation

in

high

vacuum was

quite

restricted.

Only recently,

new

deposition techniques

and treatments, such as

evaporation by

electron

bombardment, deposition

in the presence of oxygen, and exposure to ultraviolet

radiation,

have

greatly

increased the number of oxides that

can now be

deposited

in the form of

nonabsorbing coatings.

These new

techniques

have been espe-

cially

suitable for

producing

durable

optical

coa-

tings

of

Si203, Si02, A1203, Th02,

and

Zr02’

It is the purpose of this paper to present data on

the

preparation

and

optical properties

of these

oxide films and to discuss some of their

appli- cations,

such as the

preparation

of well

protected

front surface mirrors with

high

reflectance in the

ultraviolet, multilayer

antireflection

coatings,

and

surface films for

controlling

the temperature of satellites in outer space.

II.

Experimental techniques.

- The evapora- tions were

performed

in a 60 cm vacuum system in

which film

depositions

could be monitored

by

reflectance measurements with monochromatic

light.

Polished

plates

of

glass,

fused quartz and

sapphire

were used as substrates.

They

were

mounted about 45 cm above the

evaporation

sources, and could be cleaned

by

a

high-voltage

dc

glow discharge using

up to 5 kV and 100 ma, and could be heated up to 350°C. A removable shutter was

placed

close to the substrate

plates

to

avoid their contamination

during

the

outgasing

of

the

evaporation

sources and

charges.

Silicon

monoxide was

evaporated

from a tantalum con-

tainer

by

direct

heating.

A

high-powered

electron

gun

capable

of

applying

up to 20 kV and 250 ma was used for

evaporating Si02, A1203, Th02,

and

Zr02.

The oxides to be

evaporated by

electron

bombardment

were

placed

into a

dimple

of a

heavy

copper

block.

To assure

high

and rather cons-

tant

evaporation

rates, and to avoid

overheating

and

decomposing

the

oxides,

an electron beam’of at least 1.5 cm diameter was used. With this

technique,

films of

Si02

and

Al 03 produced

at

deposition

rates of about

400 Å/min

and at a

distance 45 cm from the

evaporation

source, showed no

absorptance

in the visible and ultra- violet. This is not true for films

produced

with a

highly

focussed electron beam.

The reflectance and transmittance of films

depo-

sited under various conditions onto transparent

substrates and onto

evaporated

aluminum were

measured from 2 000 A to 15 pL with Perkin Elmer and Beckman instruments. The refractive indices of

nonabsorbing

films were

computed

from the

measured reflectance values at the quarter-wave-

length positions.

Additional values for the film indices were determined from the true interfero-

metrically

determined film thicknesses and the

wavelength positions

of reflectance maxima and minima..

III. Results. - 1. FILMS PRODUCED BY EVAPO- RATION OF SiO. - Thin films

produced by high

vacuum

evaporation

of silicon monoxide are,

today,

the most

frequently

used

protective layers

for

evaporated

aluminum mirrors. However the com-

position

and

optical properties

of such

protective

films and the reflectance characteristics of pro- tected aluminum mirrors

depend strongly

upon the conditions under which SiO is

evaporated [1-3].

High deposition

rate at low pressure results in films of true SiO which show rather strong

absorp-

tance in the ultraviolet and shorter

wavelength

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01964002501-2025000

(3)

251

region

of the visible.

Coatings prepared

at a low

deposition

rate and rather

high

pressure of oxygen

are

strongly

oxidized and show a

large

shift of the

absorption edge

toward shorter

wavelength, negli- gible absorptance

in the visible and near ultra-

violet,

and lower index of retraction. Aluminum mirrors that are to be used in the visible and near

ultraviolet should therefore be

protected

with a

strongly

oxidized film rather than with one of true SiO. Below x = 300 mu,

strongly

oxidized

silicon oxide films still show rather strong

absorp-

tance which increases with

decreasing wavelength.

This has for a

long period

of time limited their usefulness as

protective layers

for aluminum mir-

rors.

Recently

it has been shown that exposure to the ultraviolet radiation of a

quartz

mercury burner

completely

eliminates the undesired ultra- violet

absorptance

of

strongly

oxidized silicon oxide films and thus makes it

possible

to

produce

well-

protected

aluminum mirrors with

high

reflectance

throughout

the far ultraviolet

[7]. Figure

1 shows

the effect of SiO

evaporation

conditions and ultra-

FIG. 1. - Effect of SiO evaporation conditions and ultra- violet irradiation on the visible and ultraviolet reflec- tance of silicon oxide protected aluminum mirrors. Pro- tective coatings effectively X/2 thick at 550 my. Irra- diation performed with 435 watt quartz mercury burner at a distance of 20 cm.

violet irradiation on the visible and ultraviolet reflectance of silicon oxide

protected

aluminum

mirrors. Both

protective coatings

are

effectively xJ2

thick at x = 550 mu. The true SiO

coating deposited

at a very low pressure shows strong

absorptance

in the shorter

wavelength region

of

the

visible,

which

gives

the mirror a

yellow

appea-

rance. The

strongly

oxidized film material pre-

pared by evaporation

at 9 X 10’5 torr of oxygen shows almost no

absorptance

in the visible and

near ultraviolet. It can be seen that five hours of ultraviolet irradiation eliminates the far ultra-

violet

absorptance

of the

strongly

oxidized film

completely

but has very little effect on the true SiO

coating produced

without oxygen. Additional

experiments

made with

coatings

more than

1 u

thick gave the same results. Ultraviolet treatment of aluminum coated with

strongly

oxidized silicon

oxide

represents, therefore,

a new

technique

for

producing well-protected

aluminum mirrors with

high

ultraviolet reflectance.

Strongly

oxidized films of silicon oxide have also been

deposited

on ultraviolet

transparent

fused quartz and

sapphire

and measured in transmit- tance and reflectance before and after ultraviolet irradiation. Their

initially

rather

high

ultraviolet

absorptance

could be

completely

eliminated and their refractive indices were

greatly

decreased

by

the ultraviolet treatment.

Figure

2 shows the refractive index of a silicon oxide

film, produced by

FIG. 2. - Refractive index of a silicon oxide film produced by evaporating SiO slowly in the presence of 02, before and after ultraviolet irradiation, from X : 0.2 to 1.6 y.

Deposition rate 3 Å/sec at 8 X 10-5 torr.

evaporating

SiO

slowly

in the presence of oxygen, before and after ultraviolet irradiation from

0. 2 p,

to 1.6 u. A film

prepared

under the described conditions consists

predominately of Si2O3 [4-6,8]

and shows an initial refractive index of 1.57 at A == 600 m,. After 5 hours of ultraviolet irradia-

tion,

its refractive index is decreased to 1.48 at the same

wavelength,

which

brings

it near to that

of fused quartz.

However,

measurements of the infrared

absorption spectra

of such films have led to the conclusion that 5 hours of ultraviolet treat- ment does not convert

Si203

into

Si02.

2.

S’02

FILMS PRODUCED BY ELECTRON BOM- BARDMENT. -

Undecomposed

films of

Si02

can be

FIG. 3. - Refractive index of evaporated Si02 produced by electron bombardment, in the wavelength region from 0.2 to 1.6 V..

(4)

obtained

by evaporating

quartz

glass

with an elec-

tron gun. If

properly evaporated,

such films show

no

absorptance

in the ultraviolet and

visible,

and

have a refractive index which is identical to that of fused

quartz. Figure

3 shows the

dispersion

curve of

S’02

films

produced by

electron bombard-

ment in the

wavelength region

from

0. 2 V.

to 1.6 y.

The measurements were made on films of various thicknesses

deposited

at rates of 400 to

800 A/min

at a distance of about 45 cm.

They

show no

interference effects when

evaporated

onto

quartz glass

since

they

have the same index of refraction.

Such films are

especially

suitable for

producing chemically

and

mechanically,

durable

protective

ayers for front surface mirrors. The ultraviolet and visible reflectance of aluminum with and without a 7 800

Å thick protective

film of

S’02

is

shown in

figure

4.

y

Even in the far ultraviolet the

FIG. 4. - Reflectance of aluminum coated with an evapo- rated S’02 film (t = 7 800

A),

as a function of wave-

length from 200 to 700 my.

protected

mirror

shows,

at the interference maxi- ma,

slightly higher

reflectance values than the

unprotected

one, which proves that

theS’02

film

is free of

absorptance

in the

wavelength region

shown. Much thinner

protective layers

of

Si0 2

should be used of course for

producing

the most

efficient front surface mirrors for the visible and ultraviolet.

3. ALUMINUM OXIDE FILMS PRODUCED BY ELEC- TRON BOMBARDMENT. - Another material which should

be

useful for

producing optical coatings

is aluminum oxide because it is both

extremely

hard

and

transparent

in the far ultraviolet. Aluminum oxide

(A’203)

can be

evaporated

from

tungsten

heaters but the

resulting

films are

slightly

decom-

posed,

due to reduction

by

tungsten, and show

some

absorptance. Decomposition,

and therefore

absorption,

can be avoided

by using

electron bom- bardment for the

evaporation

of aluminum oxide.

With this

technique extremely

hard and durable

A1203 films,

up to several, micron in

thickness,

can

easily

be

prepared

which show no

absorptance

in

the visible and ultraviolet. The refractive indices

of aluminum oxide films

evaporated by

electron

bombardment onto substrates at 40 OC and 300 OC

are shown in

figure

5 for the

wavelength region

from

0. 2 p.

to 1.6 y. The refractive indices of the

FIG. 5. - Refractive index of evaporated A1203 produced by electron bombardment, in the wavelength region

from 0.2 to 1.6 u. Substrate temperature during depo-

sition : 40 OC and 300 OC.

films

produced

at 300 °C are

slightly higher

than

those of the films

prepared

at 40 °C. In the

visible at x = 500 my an increase of the substrate temperature from 40 °C to 300 °C causes a rise in

the refractive index from 1.60 to 1.63. These values are

considerably

smaller than those of crys- talline y -

Al2O3

films

produced by

reactive

sput- tering

onto

glass

at

higher

substrate tempera-

tures

[9].

This is due to the fact that the evapo- rated films condensed on substrates of 40 °C and 300 °C are

amorphous.

Their indices agree well therefore with those of

amorphous Al2O3

films pre-

pared by

anodic oxidation

[10],

and

deposition

from

organic

solutions

[11].

Because of their hardness and excellent adhe- rence,

evaporated A’203

films are very suitable as

protective layers

for aluminum front surface

mirrors.

Figure

6 shows the visible and ultra- violet reflectance of

evaporated

aluminum with and without

AlgO3 protective

films of two diffe-

rent thicknesses. To obtain

highest

reflectance

FIG. 6. - Reflectance of aluminum protected with evapo- rated A1203 films of two different thicknesses, as a func-

tion of wavelength from 200 to 700 mu.

(5)

253

in the

ultraviolet,

an oxide thickness of 740

A

was

used,

and to

produce highest

reflectance in the visible the thickness of the oxide film

applied

was 1740

A.

This makes the

A120s

films effec-

tively

one half

wavelength

thick at X = 250 mu at X = 550 mu,

respectively.

It can be seen that

the

A’20.,

films do not exhibit any noticeable

.absorptance

in the

wavelength region

shown.

A1203-protected

aluminum mirrors show very

good

abrasion and scratch resistance.

They

cannot be

damaged by rubbing

with

rough

linen

and can be

repeatedly

cleaned withwater and deter- gent without

changing

their reflectance.

They

are,

however,

more sensitive to salt spray and

boiling

water than silicon oxide

protected

mirrors.

Figure

7 demonstrates the use of

A1203

films in

multilayer

anti-reflection

coatings

for

glass.

It

FIG. 7. - Reflectance of glass (ng = 1.51) coated with a

triple layer antireflection coating (X/4 - À/2 - X/4)

of Al20s + Zr02 + MgF2, from X : 400 to 700 my.

shows the visible reflectance of

glass

(ng =

1.51)

with and without a

three-layer

antireflection coa-

ting

which uses

A12O3

as the inside

layer.

This

coating provides

a very broad

region

of low reflec- tance and is

extremely

durable when

deposited

on

a

glass

substrate at about 300°C. The middle

layer

of

ZrO2 used

in this film combination was also

evaporated by

electron bombardment and has an

index of about 2.1 at X = 550 my.

Evapor.ated A’20.3

can also be used in combi-

nation with films of rhodium for

producing

mirror

coatings

with low visible and

high

infrared reflec-

tance similar to the ones described

by

Hass et

al.

[12].

This new

type

of " dark mirror " consis-

ting

of Rh.

(opaque)

-

A’2 0.3

- Rh

(semi-trans- parent)

-

A’20.3

is very

temperature

resistant and

is, therefore, especially

suitable for use in solar

energy converters. The Rh films used in this combination should also be

evaporated by

electron

bombardment.

4. THORIUM DIOXIDE FILMS PRODUCED BY ELEC- TRON BOMBARDMENT. - Films of thorium dioxide

(Th02)

are of

special

interest since

they

are trans- parent

throughout

most of the ultraviolet

region

and have a rather

high

index of refraction.

Th02

films

have, therefore,

been used in combination with low-index films of

Si02

for

producing

multi-

layer

interference

filters, [13]

and

multilayer pola-

rizers

[14]

for the ultraviolet

region.

The films for these

applications

were

prepared by deposition

from

organic

solutions.

Using

electron bombard-

ment, stable and

nonabsorbing coatings

of

Th02

can also be

prepared by high

vacuum

evaporation.

Figure

8 shows the

dispersion

curve of

Th02

films

evaporated

onto fused quartz at close to room

FIG. 8. - Refractive index of evaporated Th02 produced by electron bombardment, in the wavelength region

from 0.2 to 1.6 u.

temperature in the

wavelength region from 0.2 V.

to 1.6 (1.. The refractive indices of

evaporated Th02

are

considerably

lower than those

prepared

from

organic

solutions

by

Schroeder

[11].

Their

index in the ultraviolet is

high enough

however to

use them in combination with

evaporated

low-

index films of

Si02

for

enhancing

the reflectance of aluminum in this

spectral region.

The ultra-

violet reflectance of aluminum coated with a reflec-

tance-increasing

film

pair

of

S’02

+

Tho2’S

shown

in

figure

9. Both dielectric films are

effectively

FIG. 9. - Reflectance of aluminum coated with a reflec- tance increasing film pair of Si02 + Th02, as a function

of wavelength from 200 to 400 mu.

one

quarter wavelength

thick at À = 290 mu, and

result in a maximum reflectance of more than 95

%.

The

region

of

high

reflectance can be shifted to shorter and

longer wavelengths

and its maximum

can be increased

by adding

additional film

pairs

of

Si02

and

Th02.

(6)

5. COATINGS FOR CONTROLLING THE TEMPERA- TURE OF SATELLITES. -

Evaporated

films of alumi-

num

plus

silicon oxide have

played

an

important

role as surface

coatings

for

controlling

the

tempe-

rature of satellites in outer space

[15].

The

tempe-

rature control of an

orbiting

satellite with small internal power

dissipation

is established

by

arran-

ging

for the solar energy absorbed to be balanced

by

the thermal radiant energy emitted

by

the sur-

face at the

temperature

desired for the

payload.

For a

given orbit, therefore,

the crucial parameter

is the ratio of the effective. solar

absorptance,

a, of

the surface to its

hemispherical emittance,

e. For

spherical

satellites this ratio of a/e should be about

1. 2 for

maintaining

the satellite at close to room

temperature. Highly polished

metal surfaces have

a/e

values of 4 to 10 which would result in very hot satellites and failure of their instruments.

By using

aluminum in combination with surface films that are

nonabsorbing

in the solar

region

but

strongly absorbing

in the far

infrared,

surfaces

with a wide range of

a/e

values can

easily prepared.

If

evaporated

aluminum is coated with a non-

absorbing

surface film with an index of 1. 5 to

1.6,

and a thickness greater than

0 .3 u,

its solar

absorp-

tance becomes almost

independent

of the surface film thickness and assumes a value of 11.5

%

to

12.5

%.

If the surface film

has

strong infrared

absorption

bands the thermal

emittance

of the overcoated aluminum increases

greatly

with increa-

sing

thickness of the surface film.

By using evapo-

rated silicon oxide or aluminum oxide

coatings

of

various thicknesses on top of opaque

aluminum,

surfaces with any desired a/e ratio from about 5 to

0.25 can be

prepared. Figure

10 shows the infra- red reflectance of aluminum coated

0. 5, 1.0,

and

FIG. 10. - Infrared reflectance of aluminum coated with 0.5,1.0, and 1 .5 (J. thick films of A1203, from 5 to 15 y.

1.5 u

thick films of

A1203-

It can be seen that

increasing

the

A’203

thickness decreases

greatly

the infrared reflectance of

Al 203

coated aluminum and thus increases its thermal emittance without

changing

its solar

absorptance. Up

to now, more

than

thirty

satellites of different

shapes

and sizes

have been coated with aluminum and silicon

oxide,

and the

coatings

have been

completely

successtul

in

stabilizing

their

temperature

to the desired range ot 150 to 35 °C. The same results can be obtained with

coatings of

Al +

A12Û3.

REFERENCES [1] HASS (G.), J. Am. Ceramic Soc., 1950, 33, 353.

[2] HASS (G.) and SALZBERG (C. D.), J. Opt. Soc. Am., 1953, 44, 181.

[3] HASS (G.), J. Opt. Soc. Am., 1955, 45, 945.

[4] RITTER (E.), Dissertation Innsbruck, Austria, 1958.

[5] CREMER (E.), KRAUS (Th.) and RITTER (E.), Z. Elek- trochem., 1958, 62, 939.

[6] RITTER (E.), Optica Acta, 1962, 9,197.

[7] BRADFORD (A. P.) and HASS (G.), J. Opt. Soc. Am., 1963, 53, 1096.

[8] CREMER (E.) and PULKER (H.), Monatshef te f. Chem., 1962, 93, 491.

[9] HIESINGER (L.) and KOENIG (H.), Festchrift 100 Jahre Heraeus Platinschmelze, Hanau,1951, p. 376.

[10] HASS (G.), J. Opt. Soc. Am., 1949, 39, 532.

[11] SCHROEDER (H.), Optica Acta, 1962, 9, 249.

[12] HASS (G.), SCHROEDER (H. H.) and TURNER (A. F.),

J. Opt. Soc. Am., 1956, 46, 31.

[13] SOKOLOVA (R. S.) and KRYLOVA (T. N.), Opt. i Spek- troskopiya, 1959, 6, 788.

[14] SOKOLOVA (R. S.) and KRYLOVA (T. N.), Opt. i Spek- troskopiya, 1963,14, 401.

[15] HASS (G.), DRUMMETER (L. F., Jr.) and SCHACH (M.),

J. Opt. Soc. Am., 1959, 49, 918.

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