Coating and Cleaning Large - ESO · chamber of 2.6 m in diameter located at the 2.2 m telescope...
Transcript of Coating and Cleaning Large - ESO · chamber of 2.6 m in diameter located at the 2.2 m telescope...
ESO Workshop: Coating and Cleaning Large
Mirrors
ESO Headquarters Karl-SchwarzschiidstraBe 2
8046 Garching Germany
7 and 8 October 1991
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List of Participants at ESO Workshop: Cleaning and Coating Large Mirrors, 7 and 8 October 1991
Participant
A. Abraham P. Alvarez B. Atwood K. Birkle D. Cowley C. Del Vecchio A. Gilliotte T. Gregory N. Itoh M. lye D. Jackson K. Kissel B. Mack M. Maars L. Miglietta J. Montesinos M. Nakagiri H. Nicklas F. Perez H. Petrie K. Raybould P. Salinari V. Sanchez A. Schier J. Sovka R. Thicksten J. Williams R. Wolf S. Worswick
Affiliation/Project
Gemini 8m Telescope, USA Instituto de Astrofisica de Canarias, E Columbus Project, USA Max-Planck-Institut fur Astronomie, D Canada-France-Hawaii Telescope Arcetri Obs., Florence, I ESO La Silla Canada-France-Hawaii Telescope Japanese National Large Telescope Japanese National Large Telescope Royal Greenwich Observatory, UK AMOS/MOTIF Observatory, USA Royal Greenwich Observatory, UK Magellan Project, USA Arcetri Obs., Florence, I Instituto de Astrofisica de Canarias, E Japanese National Large Telescope Uni-Sternwarte Gottingen, D Carnegie Obs., Pasadena USA Palomar Obs., Caltech USA Gemini 8m Telescope, USA Arcetri Obs., Florence, I Instituto de Astrofisica de Canarias, E Carnegie Obs., Pasadena USA Canada-France-Hawaii Telescope Palomar Obs., Caltech USA MMT/University of Arizona USA Max-Planck-Institut fur Astronomie, D Royal Greenwich Observatory, UK
Summary and Presentation of Current Practice and Experience in Washing and Coating (Primary) Mirrors at existing Observatories
Contents:
1. Calar Alto 2. Kitt Peak 3. CFHT 4. La Silla 5. Mt. Palomar 6. Roque de Los Muchachos
K. Birkle A. Abraham J. Sovka A. Gilliotte R. Thicksten B. Mack
Calor Alto
Presentation by K. Birkle
Calar Alto Observatory
ESO Workshop: Coating and Cleaning Large Mirrors
Standard Procedures of Mirror Coating at Calar Alto Observatory K. Birkle, R. Wolf, G. Lingenfelder
Max-Planck-Institut fUr Astronomie, Heidelberg
Telescopes of the MPI fUr Astronomie at Calar Alto Observatory: 1.2 m RC, 2.2 m RC/Coude, 3.5 m Prime/RC/Coude, 0.8/1.2 m Schmidt. In addition, a 1.5 m RC/Coude is operated by the Instituto de Astrofisica de
Andalucia, Granada.
The MPI fUr Astronomie has installed two aluminization plants: (1) vacuum chamber of 2.6 m in diameter located at the 2.2 m telescope building (Fig. 1);
(2) since 1983 with completion of the 3.5 m telescope a 4 m vacuum tank at the 3.5 m building (Figs. 2 - 4).
Mirror Handling for Re-coating
In a series of illustrations (Figs. 5 - 12) the mirror handling is demonstrated. The whole procedure, in particular aluminizing is carried out with the (primary) mirrors in horizontal position.
For dismounting the mirror cell and lateron attaching it to the telescope again
a cart on a hydraulic platform is lifted underneath the cell (Fig. 5), Beside the
telescope, after protecting the mirror with a cover, the mirror is removed from its cell with the dome crane (Fig. 6) and lowered through the building to the ground floor.
In the metallization plant, with separate crane properly screened to prevent
grease or oil to drop from the crane onto the mirror, the mirror is lifted for washing into a tub made up of glass fibre reinforced plastic and from there after cleaning into the lower part of the vacuum chamber (Figs. 8, 9), At the 3.5 m telescope, instead of a washing tub a three-legged bench of
stainless steel is used (Fig. 10), By this, cleaning liquids freely flow to the drain in the floor.
The central support for lifting the mirror, which remains inside the vacuum tank during aluminization, is made up of stainless steel. It is different from
the radial definition support of the mirror inside the mirror cell and has to be interchanged with the latter before washing and before re-assembling the mirror in its cell, respectively.
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Fig. 1.
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Caler Alto Observatory
N-S sectional drawing of the 2.2 m telescope bUilding.
Aluminization chamber (2.6 m diameter) on the ground floor. Vertical coude spectrograph at left (northern side of building>.
Calar Alto Observatory
Fig. 2. N-S sectional drawing of the 3.5 m telescope building.
Below the telescope a 35 ton hydraulic platform for mounting cas
segrain focus instruments and for disassembly of the mirror cell. The
aluminization chamber (4 m diameter) is located on ground floor.
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Caler Alto Observatory
Fig. 3. The 4 m vacuum chamber; at the right the electronic rack for comple
te control of pumping, cooling, glow discharge and filament firing.
In the foreground at right and left of the vessel 2 of the 4- mechanical supports for lifting the upper part of the chamber, so that the lower part can be moved horizontally.
In the vaccum chamber, it is important for mirrors of different thickness to
keep their optical surfaces at the same level to an accuracy of about ± 5 cm
for reasons of homogeneity of the aluminium film depositing on the mirror surface during evaporation ( Fig. 11).
There is only one step in mirror handling which needs special care because of
increased risk of mirror damage (only in case of the 2.2 m mirror): Connecting
the mirror baffle with the central radial definition support (Fig. 12) shortly
before the newly coated mirror in its cell is attached again to the telescope,
4-
v f' r ~ , ~ ,-
Calar Alto Observatory
,
Fig. 4. Side view of the 4 m aluminization chamber with the twin oil diffusion
pumping station; in the foreground the rotary vane pump, the roots pump is not visible.
as this can only be done after removal of the mirror protecting cover. The same holds for the reverse procedure after dismounting the mirror cell. The construction of another cover to avoid this problem was not possible because
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Calar Alto Observatory
r Fig. S. Disassembly of the 2.2 m mirror cell using a transfer cart on a hydrau
lic platform.
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Calar Alto Observatory
Fig. 6. Before the mirror is taken out of its cell, the mirror surface is protected by a cover.
of the special geometry of the baffle. To avoid this risk at the 3.5 m telesco
pe the construction of the corresponding parts is completely different there.
All other steps of mirror handling are considered to be of no special risk
when carried out with normal care. For example, crane operations with the mirror are of no risk even in the case of the 14 ton 3.5 m primary, as accele
rations are kept small « 0.1 g) when starting and ending crane motion at
slow-speed; due to elastic stretching of the twisted wire cables acceleration forces are also damped.
Normally, re-coating the primary means that the telescope is out of operation
for one night. When dismounting the mirror cell begins in the morning of the
first day, the telescope is operational again in the evening of the second day.
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Calar Alto Observatory
About 5 persons are needed for mechanical work. Mirror cleaning, preparation of the vacuum chamber is done by 1 person, at times with 1 - 2 helpers.
cart weight ----\---1.5 Mp
mirror + cell total weight 30 Mp
dome floor
~ E
r-;-..-154 0
Fig. 7. In case of the 3.5 m mirror we use two identical carts, one on the do
me floor which bears mirror and cell, the other on the ground floor
for transportation of the mirror only.
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Calar Alto Observatory
Fig. 8. A view in the aluminization hall of the 2.2 m telescope bUilding.
In the middle the glass fibre reinforced PVC tub for mirror washing. In the foreground the lower part of the vacuum vessel.
Mirror Cleaning
First step washing is done with tap water at slightly increased temperature (350 C) with detergent added.
In case that some grease or oil (from lubrication of dome shutter elements) is visible on the mirror, these stains are removed first with acetone before washing starts in order not to distribute further the grease on the surface. The old aluminium film is removed using NaOH (8% solution) within about 15 minutes. If the removal of Al is not uniform or rather slow at some parts of the surface, NaOH solution at increased temperature (up to 40° C) is applied,
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Calar Alto Observatory
Fig. 9. The 2.2 m primary (Zerodur) is lifted from the washing tub into the lower part of the vacuum chamber. The upper part of the chamber and the control electronics for evacuation, glow discharge, and firing are to the right.
and cotton wool soaked with NaOH solution is placed on the mirror surface
for about 10 minutes. In most cases, however, these additional steps are not necessary.
We do not use HCl. Even with special ventilation installations HCI gas cannot removed with sufficient efficiency. Use of breathing masks is not ideal. The main concern, however, is contamination and corrosion of electronics and other
sensitive devices present in the plant. No problems of bad adhesion of the Al coating could ever be observed by not applying any acid medium.
After complete removal of the old Al film the surface is cleaned further with tap water and detergent. Normally, no mechanical treatment is applied. If it is
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Calar Alto Observatory
Fig. to. Part of 3.5 m aluminization plant showing cleaning facilities. The ion exchanger producing de-ionized water which we use instead of distilled water is to be seen in the background (box-type device with hose on the wall).
inevitable, wet cotton wool is used WlpIng in radial direction towards the cen
tral hole in a single use mode, that is, for each radial strip on the polished surface new cotton wool is used. When the surface seems to be clean, further flushing with distilled or de-ionized water in case of the 3.5 m plant is carried out (no disadvantages to distilled water used at the 2.2 m plant can be noticed).
Finally the surface is treated with pure alcohol (ethanol p.a. or isopropanol p.
a.>. In this final stage of cleaning with distilled water and alcohol a vacuum
cleaner is used at the inner rim of the mirror to remove any remaining partic-
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Calar Alto Observatory
- -I':
Fig. 11. A 1.S m primary (Chinese 1.5 m telescope with 2 Nasmyth foci for the observatory of the Instituto de Astrofisica de Andalucia, Sierra Nevada, ' Spain) is brought into the 4 m vacuum chamber ready for aluminizing. It is placed on 6 supports of such a height to compensate for the difference in thickness of the 3.5 m primary of the MPIA (one of the 6 supports for the 3.5 m mirror is to be seen at right [arrow]; the vacuum sufficient rubber disks used to avoid direct contact between mirror and the metallic support are removed>. For thin mirrors or tests with thin glass probes other supports of aluminium or stainless steel
are used, see e.g. the support leant against the wall in the background in Fig. 1Q
les or dirt floating in the liquid at the flattest part of the mirror surface.
Moreover, this speeds up the drying process. Before putting the mirror into the vacuum chamber, the remaining not polished surfaces including the rear side are cleaned with alcohol.
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, .-.,;---" , --j
-.'
Caler Alto Observatory
Fig. 12. Connecting the mirror baffle with the central radial definition support of the newly coated 2.2 m primary in its cell. This baffle serves also
as base for the mounting of the first coude flat mirror. Here, instead the compensation weight for this flat is mounted.
What are criteria for a clean optical surface, that is, clean at least for aluminization purposes? When the polished surface is drying, one can observe Newtonian interference fringes formed by a thin wedge of remaining distilled water and alcohol (Fig. 13), with the fringes slowly moving towards the mirror centre
(a few mm/sed as evaporation of the liquid is going on, leaving behind a dry surface which seems to be perfectly clean (right parts of Fig. 13), However, as
long as one can see nonuniformities in the illuminated layer of cleaning liquid (left parts of Fig. 13) the polished surface cannot be considered clean.
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Calar Alto Observatory
Fig. 13. Final stage of cleaning of the optical surface (Chinese 1.S m primary of the lAA, Sierra Nevada) with Newtonian interference fringes formed by a thin wedge of cleaning liquid (see text). The best visible fringes have a distance of about S mm from each other.
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Calar AI to Observatory
Most of these nonuniformities seen in Fig. 13 are not impurities (particles) in the liquid layer but small craters formed by breaking up the thin liquid film due to some kind of (chemical ?) inhomogeneities in the polished surface affecting the surface tension of the liquid film in a different way than further away from the craters. This (non-) v isibility of the nonuniformities is a qualitative criterion only but a rather rigorous one, which means that cleaning and flushing has to be repeated until these craters are reduced to a minimum in size and quantity.
Mirror Coating
The vacuum chambers at the 3.5 m and 2.2 m domes are equipped with 96 and 64 tungsten filaments, respectively, arranged in one circle along the chamber wall with radius of 1.8 m (1.15 m) and height = radius above the mirror surface (Figs. 14, 15). There are four electrical circuits, each of them connected with every fourth filament. All 96 (64) filaments can be fired simultaneously (normal mode of aluminization), or separately one after the other of the four circuits with 24 (16) filaments each. Each of the filaments is normally loaded with a 2 mm Al wire (99.999% purity)
58 mm long (0.5 gL A load of up to three times this normal load can be used. Above this maximum load aluminium droplets are found.
The tungsten filaments are fixed outside the mirror radius. Two rings of horizontal shields with a gap between them are mounted below the filaments to protect the mirror from aluminium droplets. The glow discharge ring electrode and its surroundings as well as the regions around the tungsten filaments, baffles and shields are cleaned before each evaporation.
Using pure aluminium, the filaments have to be renewed after two to four times of firing. The aluminium foil cover of the glow discharge electrode is renewed after about 10 discharge processes.
After closing the tank pumping, glow discharge, aluminization, and flooding in total takes about 4 hours.
The glow discharge process starts if the pressure is 10-3 mbar. The glowing time is 15 minutes at 3 kV, 1.5 Aj The pressure is 0.1 mbar controlled by a needle valve.
We begin with the evaporation at a gas pressure of 0.5 - 2 * 10-6 mbar sup
ported by the additional pumping of a LN2 cooled Meissner trap. Firing takes 30 - 40 sec with 6000 A at maximum for the 3.5 m plant, falling down to 3500 A if all aluminium is evaporated.
Before flushing the tank it is important to heat the Meissner trap to ambient temperature. The heating is simply done by blowing out the nitrogen in it with compressed air. Quality control of the adhesion of the new aluminium film is carried out by
pressing a piece of scotch tape onto the aluminium surface and removing it suddenly.
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glow discharge rin electrode
evaporation
--- -= -i -.: - ~
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Calar Alto Observatory
.,.. ,..
-f-
..;.
·1
o o o l..()
Fig. 14. Drawing of the 4 m aluminization chamber with indicated mirror posi
tion in the lower horizontally movable part.
Cleaning Mirrors in situ the Telescopes
The 3.5 m mirror cell is constructed in such a way allowing mirror washing
inside the cell. However, experience has shown that the results of washing in
most cases are not very satisfactory. Therefore, the primaries and also auxilia
ry mirrors wi th their refl ecting surfaces looking upwards are periodically recoated about once a year (1: about 4 months) without washing in the meantime.
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Calar Alto Observatory
Fig. 15. Inside view of the 2.6 m aluminization chamber. The tungsten filaments
are just loaded with aluminium wires. Annular shielding screens below the filaments and the Meissner trap are clearly visible. Part of the
glow discharge ring electrode covered with aluminium foil is visible above the head of the operator.
17
Kitt Peak
Presentation by A. Abraham
Canada France Hawaii Telescope
Presentation by J. Sovka
CF\1T
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3.6 METER PRIMARY MIRROR
ALUMINIZATION
SOP 51 1 October 1991
Page 1
3.6 METER PRIMARY MIRROR ALUMINIZATION
(Procedures followed since May, 1986)
A. Initial Inspection
The primary mirror is removed from the telescope and delivered to the aluminizing room and placed atop the mirror washing stand. Next day the mirror sides are cleaned and the radial support pads wrapped in polythene plastic for protection. The mirror surface is rinsed with tap water to remove loose dirt and then it is washed with a detergent solution of 100 parts water to 1 part Liqui-Nox concentrate. Sponges are used in a dabbing, up-down motion only so as not to scratch the aluminum surface. oily spots are carefully dobbed-up with xylene soaked Kaydry towels. Also, bubble holes in the surface are cleaned.
The surface of the cleaned aluminum is inspected for pinholes, abrasion and scattering due to environmental corrosion. The surface is examined by viewing a high intensity lamp in reflection from the surface. There was a significant amount, perhaps a few percent, of scattering of the specular reflection into a halo of diffuse light. At this point a decision must be made to keep the old coating or remove it and deposit a new one.
B. Removal of Old coating
The coating is stripped from the glass surface by flooding it with a solution of hydrochloric acid and cupric sulfate1 . After rinsing the mirror with tap water and drying it with Kaydry towels a solution of sodium hydroxide is used. This has little effect on the more stubborn residual aluminized areas. Finally the mirror surface is flooded with de-ionized water and then sprinkled with reagent calcium carbonate powder and rubbed with cotton pads. The calcium carbonate is sufficient to remove the last residue of aluminum from the optical surface. The mirror is rinsed with deionized water and then rubbed dry with Kaydry towels. Care must be taken not to allow the mirror to dry on its own by evaporation as water spots would be a likely result. After the entire mirror surface is gradually dried there still remains a large amount of Kaydry towel lint sticking to the glass surface as a result of the static electricity produced by the rubbing of the clean glass with the paper towels. This lint is removed with static-master antistatic brushes before placing the mirror in the vacuum chamber.
lSee procedure for stripping aluminum coating.
C. Aluminization
SOP 51 Page 2
Once the mirror placed within the vacuum chamber, the roughing pump and roots rotary lobe blower evacuated the chamber to a pressure of 5 microns in about 1 hr. After the cold trap LN2 chevrons are filled, the diffusion pumps is used to lower the pressure to below 5 x 10-5 torr. A glow discharge is performed to insure cleanliness of the mirror surface2 . After the glow discharge, the high vacuum diffusion pumps are used to bring vacuum to the 10-6 range. The meissner coil is filled to aid in the further reduction of pressure. Ultimately a pressure of 3 x 10-6 torr is reached in about 3 hours from the time of initial pump-down.
The individual tungsten filaments, each laden with aluminum clips are pre-heated together in a series/parallel circuit for 4 minutes to bring them all to approximately 10000C. When the Inficon crystal thickness monitor indicates 50A of deposited aluminum, the power to the filaments is increased to the maximum level. Within 30 seconds the Inficon monitor is reading 637A. This thickness, according to previous tests, corresponds to an actual coating thickness of 900-950A on the mirror surface. A deposition rate of 27A per second is indicated upon the Inficon monitor. Interferometric tests were performed upon test plates placed at the central hole and outside the circumference of the mirror. These tests, and others performed earlier at zones simulating the mirror surface showed the coating to be radialy symmetric and even in deposited thickness to within 150A. The probable wavefront error induced by the coating process is estimated to be less than or equal to A/15 at visible wavelengths. During the filament firing, no drops of molten aluminum fall upon the mirror surface. The resultant coating looked brilliant and very free of scatter over its entire area and showed no signs of bloom or diffusion pump backstreaming. No wipe marks or haze due to incomplete cleaning should be observed upon the mirror surface.
D. Adhesion Test
A scotch tape test is performed on the outer bevel and upon the actual mirror surface one inch inside the outer circumference. No aluminum should be removed by the tape at either site.
2See glow discharge procedure.
THICKNESS OF EVAPORATED ALUMINUM FILM
SOP 51 Page 3
During the month of April 1986 tests of the CFHT Summit Aluminizing chamber were carried out to measure the actual thickness and uniformity of Aluminum coatings produced by the 112 filament array of evaporation sources. A set of ten test plates were used to simulate the mirror surface. For the initial test all filaments were loaded with 10 loops with a weight of .065 grams each. (Loops are from Jori Resources and are of 99.99% purity).
The loaded filaments were heated for approximately 5 minutes while monitoring the amperage at Inner Ring #2 = 330 amps. The Inficon crystal thickness/Rate of deposition monitor at the end of the 5 minute preheat period was reading o-lA /second. The total accumulated thickness after the preheat was 40A.
At this time the array voltage was increased and monitored at the Inner Ring #2 = 25 volts. This voltage was maintained for approximately 80 seconds during which time the evaporation rate reached a peak value of 28 A/sec. After an elapsed time of 80 seconds the evaporation rate dropped to zero and all power to the array of filaments was stopped. A total indicated thickness of 652 A was obtained. When· the test plates were measured with the Angstrom-scope interferometer, the following thicknesses were obtained.
1. Test plates approximating the outer 1 meter annular surface = 884 to 913A .
2. Test plates approximating the inner 1 meter circular surface = 1148 k to 1207A .
It was concluded from these results that a superior coating uniformity could be obtained by loading outer ring filaments with 10 loops and inner ring filaments with only 8 loops each. Also, the Inficon crystal monitor readings are about 30% low presumably due to the proximity of the crystal sensor to the chamber wall (-150mm) .
During the primary mirror aluminization in May 1986, test plates were positioned around the circumference of the mirror and within the central hole. After evaporation the following thicknesses were obtained upon the test plates as measured with the interferometer:
a. Circumferential Test Plates = 842, 795, 795, 845, 825, 913, 913, 854, 756A .
b. Central Test Plate = 962 A+.
c. Inficon Measurement = 639A .
d. Maximum Deposition Rate = 27A /second.
SOP 51 Page 4
It is estimated that local mirror surface wavefront distortions caused by the coating process itself are less than A/15 at visible wavelengths. Another test is planned for the future as it is felt that the 3.6 meter mirror surface coating is not accurately depicted with only 10 test plates and that perhaps 30 plates are necessary. This is particularly important near the chamber walls.
CFHT Vacuum Chamber T. Gregory
22 April 1986
ffi Test Plate Height = 24 inches (.6096m)
o P #1 o P #2
e884A
652A 913A ffi
el178A
ffil178A
ffi 1207A + center
ffi1148A
81178A
ffi 884A
61178A ffi884A
Filament Loading: All loaded with 10 loops of .065 grams AI.
SUMMIT VACUUM CHAMBER PREPARATORY CHECKLIST
1. Inficon monitor operation.
2. Cold cathode gauge operation.
3. Chamber lift-jack operation.
4. Integrity of roughing manifold rubber connection.
5. Pre-aluminized test plates, 10 required.
6. 10 single edge razor blades required.
7. Test plate stands.
8. Static-master brushes, 6 required.
9. Check air pressure and control panel functions.
10. Glycol coolant, chiller fan and pump operation.
11. Back-up diesel generator checklist.
12. 3x160 liter dewars of LN2 required.
13. Viewpoint windows cleaned.
14. Torque wrench (15 in-lbs.) for filament installation.
SOP 51 Page 5
CFHT SUMMIT VACUUM CHAMBER CHECKLIST
Pump-down operation:
SOP 51 Page 6
1. Check Inficon Thickness Monitor for proper crystal oscillation.
2. Close tank after inspecting bottom plate "0" rings for smooth and very light lubrication with Dow Corning High Vacuum Grease.
3. Close Air-leak and vent valves. 4. Turn cycle selector switch to manual position (key switch). 5. Connect chamber foreline manifold to roughing pump. 6. Turn chiller condenser fan "ON" in equipment room with
chillers. 7. Turn on 2 glycol supply taps and adjust flow with glycol
return tap to flow gauge valve of 2 1/4 gpm. (The safety flow switch enables the D.P. heating circuit at flow rates in excess of 2 gpm).
8. Start stokes roughing pump. (10 minute warmup period) 9. Check rough pump flow and oil level sight glasses. 10. The Rootes Blower will start automatically after a few
seconds when p ~ 15mm Hg. (see gauge near holding pump) 11. Turn on air supply valve and air dryer. (plug in!) 12. Start the holding pump. 13. Open fore line valves #1 and #2 to evacuate the diffusion
pumps. Wait for valve to open, takes 30 seconds. 14. Turn on thermocouple gauges number 1 through 4. 15. The roughing pump will quickly evacuate the DP's to p ~ 10
microns at T.C. #2 and T.C. #4. 16. Open holding pump valves to D.P. 's 17. Close foreline valves #1 and #2. 18. Turn on DP' s #1 and #2. (These will heat up only if the
glycol safety flow switch senses greater than 2 gpm glycol coolant flow).
19. Turn on seal pump. 20. Open chamber roughing valve. (It will take approximately 30
minutes for the rootes blower to turn on at p=15 mm Hg. It will take an additional 30 minutes for the chamber to reach the range of p ~ 20 microns).
21. Turn on Varian Cold Cathode gauge (pressure should be low enough to be on scale wi thin 1 hr. after opening roughing valve. (p ~ 10 microns)
22. Connect LN2 supply to DP Chevron traps via LN2 manifold. (The liquid level in the traps is automatically maintained. The consumption of LN2 is 10-20 liters/hr) . Open trap valves.
23. Connect LN2 supply to Meissner trap. 24. While the chamber is roughing down it will be necessary to
monitor the fore-pressure of the hot DP's as their pressure may exceed 100 microns with only the small capacity holding
SOP 51 Page 7
chamber rough pumping after the interruption. (There is a 10 second delay built into the control circuit which delays the opening of the foreline valves after closing the chamber roughing valve) .
25. When the chamber pressure is approximately 10 microns close the roughing valve and open the foreline valves to the DP's.
26. Close the holding pump valves. 27. To start high vacuum pumping on the chamber through the
diffusion pumps open the high vacuum valves #1 and #2 in succession while monitoring the foreline pressure in each to not exceed 100 microns. (As a precaution against backstreaming D.P. oil into the chamber allow about one minute between opening of the High Vacuum valve #2 after high vacuum valve #1 is opened).
28. Shortly after both high vacuum valves are opened the chamber pressure should be in the low 10-5 torr range. (SEE GLOW DISCHARGE PROCEDURE) .
29. with the chamber empty it takes about 1 hr. after the high vacuum valves are opened to reach a chamber pressure of approximately 5x10-6 torr.
30. During the high vacuum mode of pumping the Meissner trap should be filled as follows. Turn on the LN2 supply to the Meissner coil by gently opening the LN2 supply valve less than one full turn to avoid pressure vibrations from LN2 evaporation inside the coil. Pressure rises occur within chamber if the coil is filled too rapidly. Trap fills in approximately 30 minutes. Close valve and re-f ill in 10 minutes.
31. The chamber is ready for operation at a pressure less than or equal to 5 x 10-6 torr.
Procedure for stripping Mirrors of Aluminum coating
1. Change water filters.
2. Prepare a Solution of Hydrochloric Acid as follows: 4 liters of deionized water
SOP 51 Page 8
4 liters of Reagent grade (1 Normal) Hydrochloric Acid 100 grams of Cupric Sulfate crystal, Reagent grade. (When diluting, always add acid to water!)
3. Prepare a solution of Sodium Hydroxide: 4 liters of solution at a concentration of 100 grams of Sodium Hydroxide pellets (Reagent Grade) to 1 liter of deionized water.
4. Protect radial supports attached to sides of mirror by duct taping polyethylene film around them.
5. Flush mirror surface with copious amounts of filtered tap water to remove loose particles of dust.
6. Use Xylenes to clean. any oil from the mirror surface with soft Balzer's cotton wool pads.
7. Wash mirror with diluted (1:50) Liqui-Nox detergent using natural sponges and a dabbing action without heavy rubbing. Repeat this washing after a thorough rinse.
8. After mirror is clean, dry it's surface with natural chamois skins and inspect coating for condition, i.e. pinholes, stains, etc ...
9. During washing operations, pay careful attention to cleaning out bubble-holes in the optical surface as these can conceal dirt.
10. If it is decided not to save the old aluminum coating and re-coating is necessary then apply the Hydrochloric/Cupric Sulfate solution to the mirror surface. Spread the solution by dragging soft cotton wool along the surface to even the flow of solution over the aluminum coating. (Always wear protective apparatus when working with acids & bases.)
11. After 5 to 10 minutes most of the Aluminum coating will have bee~ removed. Some rubbing action may be required.
12. Rinse with copious amounts of filtered tap water and then dry the surface with Kaydry Laboratory paper towels.
SOP 51 Page 9
13. Inspect the surface for residual aluminum or water marks and other hazy wipe marks which have stubbornly refused to be dissolved by the Hydrochloric/cupric Sulfate solution.
14. If the surface still does not appear to be perfectly clean of old deposits it is necessary to flood the surface with deionized water and to sprinkle a small quantity of Reagent grade Calcium Carbonate powder upon the surface of the water film. A light rubbing action should remove any residual stains or deposits. (Note: the CaC03 powder must never be applied dry or allowed to dry upon the mirror surface.
15. The mirror surface is once again flooded with copious amounts of filtered tap water. Finish the rinse with deionized water and dry with Kaydry towels. Repeat step #14 if needed.
16. Wash mirror surface thoroughly with diluted Liqui-Nox detergent using natural sponges.
17. Rinse well with plenty of filtered tap water and then deionized water.
18. Dry part of the mirror with Kaydry towels being careful not to allow the mirror surface to dry on its own as water marks will occur. Gradually, dry all the mirror keeping the portions not being dried at the moment wet with deionized water. Much rubbing is involved with this step and some residue of the paper toweling will remain on the mirror surface.
19. To remove the paper residue on the mirror it is necessary to brush the surface thoroughly with the set of six parallel anti-static brushes before placing the mirror inside the vacuum chamber.
20. As with all optical coatings, success depends upon obtaining an extremely clean substrate surface.
FILAMENT INSTALLATION
SOP 51 Page 10
Filament type: R.D. Mathis* (Order as 4 x .030 W RDM-F-16683A)
1. Install 112 new tungsten filaments onto the chamber electrodes using 10-32 x 3/4" stainless steel Allen Socket flat head screws. (1/8" Allen Socket opening)
2. Tighten all 224 screws using special torque wrench to insure equal contact resistance at joint.
Torque setting = 15 in-Ibs.
*The R.D. Mathis Company 2840 Gundry Avenue P. O. Box 6187 Long Beach, CA 90806 PH: (213) 426-7049
OUTGASSING OF FILAMENTS
SOP 51 Page 11
To perform high temperature (>2000 0 C), vacuum cycle of filaments.
1. a) b)
Pump chamber to 5xl0-6 range (see: Pump Down Operation). Perform a glow discharge as described in SOP 51 p. 13.
2. Turn Filament power switches to all 4 filament rings to "on" position.
3. Turn cycle selector switch to "manual" position.
4. Slowly raise power to all rings until current for inner ring #2 is about 330 amperes.
5. View all filaments or reflected light from filaments to insure they appear to heat equally and become incandescent together and with same apparent temperature.
6. After approximately 3 or 4 minutes rapidly increase the power to all filaments until there is 25 volts of potential across inner ring #2. Hold this power level for 10 seconds to degas all filaments of impurities (low melting point metal, etc.).
7. Lower power to all filaments until all ammeters read zero.
8. Turn off all 4 filaments ring power switches.
9. Turn cycle selector switch to "off" position.
10. End of Filament outgassing (See: Shutting down system).
(Note: Tungsten melts at 3,382°C)
Loading Aluminum Loops on Filaments
SOP 51 Page 12
1. Aluminum Loops: Jori Resources*-.065 gram loops-99.99% AI.
2. Loops are loaded only at the downward curves of the filaments near the ends where the electrodes connect to the filament. The central "pigtail" helix of the filament is left free of loops to discourage the possibility of a droplet of molten aluminum falling through the hole in the baffle plate and damaging the mirror surface. If a drop of molten aluminum does fall it will most likely falloff near the ends of the filament and will harmlessly cool and solidify on the baffle plate. Only a relatively thin layer of molten aluminum should be drawn by capillary action toward the central helix of the tungsten filament.
3. To deposit an even thickness of aluminum on the mirror substrate it is necessary to load 10 loops onto each of the outer ring filaments (those two concentric sets of filaments nearest the outer wall of the vacuum chamber) and 8 loops onto all the remaining inner rings of filaments.
*Jori Resources Corp. 2128 Knoll Drive Ventura, CA 93003 PH : ( 8 05 ) 64 2 - 2 2 66
GLOW DISCHARGE OPERATION
Theory-
SOP 51 Page 13
In order to condition the substrate surface to enhance the quality of the coated film, a glow discharge is caused to occur within the chamber which has been preevacuated to 5XIO-5 torr with the substrate inside the chamber. The glow discharge is ignited by a continuous AC high voltage arc across two insulated ring electrodes of aluminum after the pressure within the chamber has been increased by the introduction of air to a pressure of 25 to 30 microns.
The glow discharge has several beneficial effects which are:
1. The substrate surface is degassed through heating. 2. Conversion of organic substances on the substrate into their
volatile components through interaction with ionized residual gas.
3. Desorption of films on the substrate surface through electron impact.
Operation-
1. The chamber is evacuated to 5 x 10-5 torr •. 2. Close high vacuum valves. Shut off chamber ion gauge. 3. Open D.P. holding pump valves. 4. Close D.P. foreline valves. 5. Open air-leak pressure control valve. 6. When pressure reaches p= 25-30 microns open chamber roughing
valve. 7. Monitor chamber pressure at TC #1 while adjusting vernier
throttling valve until pressure is maintained between 25-30 microns (nominal setting = 10.2).
8. Monitor pressure at TC #1 throughout glow discharge cycle of approx. 10 minutes.
9. Turn powerstat located on glow discharge panel fully counter-clockwise until at the zero setting.
10. Turn on glow discharge. First turn on pressure control. 11. Turn powerstat clockwise slowly until .5 ampere is read on
the ammeter., Maintain this current setting throughout glow discharge cycle. (A powerstat setting of 40% should be sufficient to maintain the .5 ampere current at an electrode potential of 1,000 to 2,000 volts.
12. After 10 minutes return powerstat to zero position and turn off the power.
13. Close pressure control valve and vernier valve. 14. After chamber has roughed to a pressure of 10 microns close
the roughing valve and open the D.P. foreline valves. 15. Close holding pump valves. Turn off holding pump.
SOP 51 Page 14
16. Open high vacuum valves #1 & #2. After a few minutes the chamber pressure will again be at 5 x 10-5 torr.
To operate glow discharge without holding pump (not recommended but doable). Run glow discharge cycle before heating D.P. IS using this procedure.
run glow discharge cycle before heating D.P. IS
close rough valve open leak until TCl reads 25 millitorr open rough valve (now TCl will stay at 25 millitorr) turn on glow discharge turn on pressure control turn up glow discharge power to .5 amp (~40 on dial) (inspect visually the aurora) run ten minutes
MANUAL FIRING OF FILAMENTS
SOP 51 Page 15
To evaporate aluminum (M.P.=660 0 C) from outgassed tungsten filaments which are loaded with aluminum loops at each end.
Chamber pressure ~ 5xlO-6 torr.
1. Program the Inf icon thickness monitor with the following parameters: Aluminum Density = 2.70 g/cm3
z ratio = 1. 08 2. Turn cycle selector to "manual" position. 3. To fire all filaments simultaneously, turn all 4 filament ring
power switches to the "ON" position. 4. Slowly raise power to all rings until inner ring #2 ammeter
reads 330 amperes. 5. Within 5 minutes the aluminum loops will melt and the molten
aluminum will be drawn to the center of the filaments by the "wetting" action of the molten aluminum for the stranded Tungsten filament. As the molten aluminum reaches the hotter surface of the central region of the Tungsten filament it will begin to evaporate.
6. The Inficon crystal monitor will begin to read a rate of aluminum deposition of 1 to 2 Angstroms/second.
7. When the Inficon monitor reads a thickness of about 50 angstroms increase the power on all rings until the voltage on inner ring #2 reads 25 volts.
8. The Inficon monitor should now indicate a deposition rate of about 30/second.
9. When the Inficon reads a total thickness of approximately 600 to 650 the power on all rings should be returned to zero and all power switches turned off.
10. An Inficon reading of 650 Angstroms yields a coating thickness of 900 Angstroms measured with the Angstrom-scope, interferometer.
11. See: Shutting Down system.
SHUTTING DOWN ALUMINIZING SYSTEM
SOP Sl Page 16
After outgassing or aluminizing operations have been completed it will be necessary to follow these steps to discontinue vacuum chamber operation, prior to opening.
1. Start the holding pump. 2. Turn off LN~ supply and disconnect dewars from Meissner trap
and LN2 man1folds. 3. Close high vacuum valves #1 and #2. 4. Turn off chamber seal pump. S. Turn off chamber ion gauge and/or cold cathode gauges. 6. Turn off diffusion pumps. (Approximately 2 hr. cool down
required) . 7. Open holding pump valves to diffusion pumps. 8. Close foreline valves #1 & #2. 9. Turn off roughing pump. (Manually vent pump to atmospheric
pressure. Air venting of pump is accomplished via manual valve on roughing manifold).
10. Leave glycol cooling on for 2 hrs. (Do not use rapid cooling).*
If chamber is to be opened:
11. Check again to be certain high vacuum valves #1 & #2 are closed. (Rapid oxidation of hot diffusion pump oil can lead to a serious explosion)!
12. Slowly open chamber air-release valve. Total venting back to atmospheric pressure takes approximately 20 minutes.
13. Disconnect the roughing pump from the chamber vacuum manifold.
14. Raise chamber about 50mm after it has been brought back to atmospheric pressure.
15. Walk around chamber to be sure all hoses and wires are free and clear and that there is ample slack to permit full upward motion of chamber.
16. Check the position of the overhead crane bridge to allow clearance and then switch crane power to "off" position.
17. Raise chamber to fully open position against up-limit switch. 18. Carriage drive switch can now be used to move bottom of
vacuum chamber to desired position. 19. For best long term chamber performance it is necessary to
leave the chamber at a pressure of 10 to 100 microns. This is easily done with the roughing pump only. (See: Pump down operation summit vacuum chamber checklist).
*See manufacturers' data.
SOP 51 Page 17
MIRROR STRIPPING, CLEANING, AND COATING SUPPLIES CHECKLIST
Items:
1. 5 Natural Chamois3 , well washed in Liquinox solution.
2. 8 Natural sponges3 , purified by pounding and HCL acid soak.
3. 4 Acid Vapor MasksS
4. 4 liters Photrex Methanol Absolute1 (Baker Reagent)
5. 4 liters Trichloroethylene1 (Baker Reagent)
6. 4 liters Xylenes1 (VWR Reagent)
7. 4 liters Acetone1 (U.S.P.-F.C.C Baker)
8. 4 liters Liqui-Nox1 Detergent Concentrate
9. 1 Kg. Calcium Carbonate Powder1
10. 2 cartons of "Miracloth" material
11. 1 Kg. Potassium Hydroxide Pellets1 (Baker Reagent)
12. 1 Kg. Sodium Hydroxide Pellets1 (Baker Reagent)
13. 2 Kg. Cupric Sulfate 5-Hydrate1 , Fine Crystal (Baker Reagent)
14. 20 liters 1 Normal Hydrochloric Acid1 (Baker Reagent)
15. 2 Boxes "Pylox" glovesS
16. 2 Boxes Neoprene glovesS
17. 2 Boxes Nitrile-Rubber gloves S
18. 4 pair protective gogglesS
19. 1 face shields
20. 5 Nalgene Mixing Buckets1
21. 20 Boxes x 90 wipes each "Kaydry" paper towels (VWR) 1
22. 10 bags x 30 pads each cotton wipers (Balzers)
23. 10 PVC yellow Tyvek Jumpsuits 4 (Large)
24. 10 Tyrel White Jumpsuits 4 (Large)
25. 10 Surgeons Caps
26. 10 Surgeons Masks S
27. 6 pair of rubber bootsS
28. 1 box of plastic booties
29. 1 garden hose (50 ft.) with outlet end cut off
30. 40 gallons of De-ionized water
31. 4 water filters
32. 1 large roll of Polyethylene film4
1. VWR Scientific, P. O. Box 29697 Honolulu, HI 96820
SUPPLIERS
2. Cole-Parmer Instrument Co. 7425 North Oak Park Avenue Chicago, ILL. 60648
3. McMaster-Carr Supply Co. P. O. Box 54960, Los Angeles, CA 90054-0960
4. Consolidated Plastics Company, Inc. 1864 Enterprise Parkway Twinsburg, Ohio 44087
5. Lab Safety Supply P. O. Box 1368 Janesville, WI 53547-1368
SOP 51 Page 18
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Mt. Palomar
Presentation by R. Thicksten
CALIFORNIA INSTITUTE OF TECHNOLOGY
PALOMAR OBSERVATORY
PROCEDURE FOR WASHING
AND
ALUMINIZING
THE 200 INCH MIRROR
Revised September 21, 1991
Edited from the notes of:
Earl Emery Bruce Rule Robert Thicksten
200 IIOi Au,,"'1 - Revised 9/21/91 - RPT
Preparation for Mirror Wash
Inspect the surface of the mirror to determine if there is any material which may have come in contact with the surface that may need special cleaning attention.
Oil is removed by using solvents before preceding with soap wash.
During the wash it is necessary to prevent water from getting into the cell area below the mirror where the delicate support system for the mirror is located. To prevent this, a Mylar dam is placed around the perimeter of the mirror and should protrude about 4 inches above the surface. A skirt is then taped below the dam to prevent any over-spills or leaks in the dam from reaching the cell. A pan is installed in the center of the mirror, and is sealed to the glass with an O-ring and· bol t-on clamp assembly. The pan is supported by the flange that carries the coude' pedestal. In the center of the pan is a lifting handle which, after installation, is replaced by a drain assembly which passes liquids through the mirror and cell below.
Clean the outside perimeter of the glass with acetone and alcohol so that tape will adhere well.
Tape a plastic drop-cloth around the perimeter of the glass about 12 inches below the lip edge and let it extend down below cell.
Put double-sided, 4 inch wide masking tape around the perimeter as close to the lip as possible.
Attach/Install a single 8 inch wide Mylar (or similar acid resistant material) to double sided tape and the seal bottom edge wi th 4 inch wide gaffers tape. Note that Mylar should extend about 4 inches below and about 4 inches above the lip of the glass.
Apply second course of- gaffers tape over and extending about 3 inches below the first.
Install the center pan using O-ring and drain tube. Make sure the bottom pass-through plate has been removed for the tube to pass through.
Install the drain hose from the drain tube to floor drain.
Make sure all sponges, buckets and chamois are thoroughly cleaned in Orvus and distilled water before the wash.
\
2
MIRROR WASH
Soak
Mix ab·out 1/4 cup of Orvus soap with about one gallon of distilled water in a plastic bucket. Make up 3 to 4 buckets. Have one person standing by to make fresh soap solution as needed.
Do not use tap water which might contaminate the sponges with particles that could scratch the mirror.
Wet the surface with the soap solution and period of 15 to 20 minutes to allow the soap away as much dirt as possible.
keep it wet to lift and
for a float
Note .that it is important that from now until the mirror is dried, it be kept wet in order to prevent drying marks.
Rinse
Rinse using filtered tap water at low pressure through an ordinary garden hose (all metal fittings removed) for about 10 minutes. Pay special attention to the Mylar to mirror gap as soap will collect there.
When the rinse is complete, a worker is placed in the center of the mirror. This worker, along wi th other members of the wash team gathered around the perimeter, begin patting the surface with sponges soaked with Orvus soap and distilled water.
The procedure is to pat the surface 3 to ~ times, turn the sponge over, pat 3 to 4 times again and then rinse the sponge in the soap bucket. The idea behind this patting procedure is that debris that might scratch the surface 1s picked up and discarded before doing so. Rubbing could, of course, carry the debris across the surface and scratch it.
Rinse
After the entire surface has been patted/washed 1 t is again rinsed for 10 to 15 minutes and then washed again. Be sure to change bucket solution, at the least, between every wash.
If the mirror is to be aluminized, proceed to ACID WASH section.
3
200 mOl Al.L\~ - Revised 9/21/91 - ~T
Clean Sponges
After the second wash, wash the sponges thoroughly to insure that no particles that might have been picked up by the sponges during the patting wash remain.
With clean sponges, apply the soap solution to the surface in a wiping motion - do not press down, but rather drag the sponge across the surface. Rinse in soap solution after 2 long swipes -one each side of sponge.
Rinse
Rinse with tap water 10 - 15 minutes.
Repeat wash, this time using light pressure in sponges when wiping.
Rinse with tap water a minimum of 20 minutes, during which time the man can be removed from the center of the mirror and the Mylar dam can be removed. Do not allow the mirror to dry!
Using distilled water poured from buckets, rinse the mirror with about 15 gallons.
Dry the mirror with clean chamois.
(00 lNOt Au...., - Revised 9/21/91 - RPT
ACID WASH
After·a hose rinse, respirators and protective clothing are put on by workers to protect them from the acids and caustic chemicals that will be used to remove the aluminum coating. Also, fans are set up to suck fumes from the work area and exhaust them outside.
Apply Green River Solution
A solution of 1 quart hydrochloric acid, HCl, mixed 'with 2 quarts water and 1 ounce cupric sulfate, CuS04' makes up what is referred to as "Green River" solution (the cupric sulfate having turned the diluted acid green).
This solution is carefully poured from plastic buckets over the surface from the perimeter. A dam of disposable, lent-free paper lab towels is normally placed around the mirror, about half way to the center. Another dam is placed around the center hole of the mirror. These dams will slow the flow of the acid from the surface and allow more time for the chemical to dissolve the aluminum. After a few minutes, have workers begin wiping the surface with lab towels to aid in the removal of the aluminum. This is a dangerous time in the aluminizing _process, as workers must stretch out over the glass to reach the" ,entire surface. The worker that is in the center pan must position himself in a squatting position as one cannot kneel in the acid that is flowing to the drain beneath him. Also workers must be careful that the fume masks and safety goggles are well secured - if they fall off and hit the surface, damage to the mirror could result. After about 5 to 10 minutes the honeycomb structure of the Pyrex glass is evident.
Rinse
After about 30 minutes or so, if there is no longer any evidence of aluminum, all lab towels are removed and a 10 minute hose rinse is begun.
Apply Potassium Hydroxide KOH solution, followed BY Calcium Carbonate.
The next step is to apply a caustic solution to the surface to remove any aluminum particles which still may be adhering to the
_ surface.
Mix 1 part KOH with 25 parts water and apply evenly over the surface.
Again, dams are placed on the surface, and after application, the solution is agitated with lab towels. After 2 to 3 minutes, CaC03 powder is dusted/spread over the surface. Using lab towels, the
5
200 ltni ALI..M - Revise:] 9/21/91 - RPT
powder is mixed with the KOH solution on the surface and then this mixed solution wiped over the surface for about 5 minutes -rinse before drying starts.
Repeat.
Rinse
Rinse for about 30 minutes - pay special attention to the dam, the CaCo3 will want to stay between the glass and Mylar.
Apply nitric acid solution.
Mix 1 part HN03 with 1 part water and apply to the surface - do not leave this on the glass for more than 2 minutes.
-Apply the diluted solution of nitric acid over the surface -again dams are used and the solution agitated with lab towels.
Rinse
Rinse for about 30 minutes - again, pay special attention to the dam area.
All protective clothing can now be removed and returned for washing and storage.
At the end of the rinse the Mylar dam is carefully removed to insure that there is no splash-back from the wet Mylar to the glass surface. During "this, as well as preceding steps, no part of the surface is allowed to dry. If any portion of the surface dries, there will be some type of drying mark left which means returning to an acid wash.
Final Rinse .
Distilled water,. about 20 gallons, is: now poured over the glass. As some water will go over the outside perimeter, workmen standby to mop up any spills.
- The skirt which has protected the mirror cell is now removed.
6
200 lOOi ALl.l't1 - Revised 9/21/91 - RPT
DRYING AND ETHYL ALCOHOL WIPE-DOWN
Disposable lint free cotton gloves are put on and the mirror surface is dried using lint-free disposable paper lab towels. Towels are changed frequently.
Once the surface has been dried, immediately precede to wiping the surface with ethyl alcohol. A lab towel is held in one hand and a plastic squeeze bottle is used to apply a small amount of alcohol to the towel. The towel is then wiped across the surface in one pass and discarded. After about 20 minutes of wiping with alcohol, "black breath" tests are begun.
Breathing onto the surface should spread a even layer of moisture which will be evident for a few seconds when viewed against a distant light source (our fluorescent work-lights work OK for this). During the few seconds available, wipe marks or other surface defects will be apparent. When the breath test shows a smooth even surface stop wiping. The alcohol bath can take an hour or more.
W~~e the perimeter/side of the glass with ethanol.
The mirror is immediately placed into the tank and pumping begun.
7
200 IIOi AU..., - Revis~ 9/21/91 - RPT
PREPARATION FOR ALUMINIZING.
It is a good idea to test the system a month or so ahead of the engineering/aluminizing run to insure that the system is functioning properly, all gauges are working etc. In the past, opticians have even melted the aluminum on to the filaments during this test procedure. Experience has shown that melt-in is not necessary.
Verify that electrical leads in the tank lid have been changed from the melt-in mode (single filament firing) to the mode for pair firing and fast firing. At this point the tank lid should be on it's supports on the observing floor.
Inspect the filaments visually.
Replace broken filaments and its firing partner using filaments.
8 loop
Load filaments. Wearing clean cotton gloves, use the special long-nosed pliers to install 3 loops of aluminum per filament (315 filaments in all). Each loop is 0.47 inch long aluminum wire, 0.040 inch in diameter. For fast fire filaments (total 35) use 5 loops of aluminum.
Check for continuity and possible shorts of all filaments using an ohm meter.
Record which filaments were replaced in the filament log-sheet.
Clean the tank. Remove debris, clean surfaces with solvent (acetone) as needed.
Check that the tank-to-mirror a-ring is clean, greased (silicone vacuum grease) and properly seated.
Insure that the port windows inside the tank lid have been stripped and cleaned for easy viewin~ of the glow discharge and filament firing. ,
On the tank lid, clean and grease the main flanges that seal to the rubber grooves in the base. Also clean « grease the base grooves.
If desired, put several clean glass test slides/plates on the stainless steel plug in the Cassegrain hole and around the outer shelf for possible test purposes.
8
2CXl I~ ALlM - Revised 9/21/91 - ~T
Assemble Tank
With the mirror prepared, raise the four guide posts into position and lift the tank over the mirror. Lower the tank slowly until the O-ring mirror seal is a few inches above the lip of the mirror. Using a bright light source, watch to insure that the Dring does not come off as the tank is lowered around the mirror. Stop - when the tank is about 4 inches from contacting the cart. Raise the cart until contact is made and slack is apparent on the lifting cables.
Lower the crane hook and disengage. i
Lower the cart so vacuum ports are ready for contact. At this point the tank is separated from the pumping manifold by 2 feet or so. Clean upper and lower flanges and clean and grease (lightly) a-rings on manifold and roughing interfaces between tank and pumping s.ystem.
Move tank into contact with the vacuum ports; align and bolt upper and lower ports together.
Put the pair firing transformer (same as for 84" tank) and fast fire transformer on top of the tank at a convenient place towards the direction of the aluminizing console (control). Do not put these transformers on the tank before this step or the tank will be unbalanced for lifting.
9
m l~ ALlJtl - Revised 9/21/91 - RPT , ~
PUMP-DOWN
On the observing floor:
Activate all circuit breakers
Turn on air compressor for pneumatic valves
Turn on water cooling to all 3 roughing pumps
Make sure drain-hoses are properly located.
Make sure water is flowing through each pump.
At the Control Console:
Install water lines to intermediate and bypass D.P.s. Check water flow.
Install gauges to tank.
Install glow discharge and other electrical to tank.
Turn on main power.
Check control board to insure all valves are closed.
Turn on the TC gauges.
Prepare pump-down chart recorder to record tank pressure.
Turn on the 3 roughing pumps (Stokes, Kinney, eX LeBold) and moni tor their individual, isola ted base pressures. They should reach less than 50 microns in less that 15 minutes.
I
Open the Stokes pneumatic valve, RV2 ~o the D.P.s and fore-line. , Open the two mechanical gate hand valves, BV1 eX BV2 one for each pump at about foot level on the D.P.s.
When the D.P. fore-line pressure is less than 50 microns turn on D.P. 's and the 2 refrigeration compressors for D.P. cold traps (on observing level).
Turn on the 2 separate water valves for D.P. cooling. The water temperature should be stabilized, by ~egulating flow, at 115 -120 F. This takes about an hour.
The tank may be rough pumped whi I e the D . P. "s are heating up using the Lebold and Kinney to pump the tank. Open the pneumatic valves, RV1, FV2,RV3 eX RV4 between the pumps and the tank. Make ~ the valve FVl to the D.P.s from these pumps stays closed.
10
200 loo-! AWl - RevisEd 9/21/91 - (:$>T
While the tank is pumping down connect the firing circuits. The fire lead of the small transformer connects to the inner or outer lug, with a shorting cable between inner « outer lug. The large transformer hot leads CORnect to lugs marked 1 through 10 on the Lucite bar. Both transformer ground leads connect to bolts on the steel structure. Make sure all Variacs are turned off and all knife switches are open.
When the tank pressure is below 1000 microns, (30 minutes or so) activate blower switch from time to time. When the pressure is low enough the blower will stay on. The pressure will fall fairly quickly (15 minutes) below 10 microns.
When the tank is below 50 microns, close valve FV2 and open valve FV1 to put the Kinney on backing for the D. P. 's along with the Stokes. This leaves only the Lebold roughing the tank.
When the 'tank is below 50 microns, turn on the emergency bypass and intermediate D.P. IS. Check water cooling and proper heater operation on these 4 pumps.
Turn on ion gauges.
Turn on the chart recorder.
Moni tor D. P. gauges ION 2 « ION 3 to enSUl:e they are w_'!fking properly - the pressure should be at or approaching 10 . "'-"-TCRR.. Gl'giAS.
When the bypass, intermediate and main D.P.s have come to temperature and the high vacuum io~auges ION 2 « ION 3 indicates a pressure of less than 25 *' 16 microns, open D.P. gate valve DPV1 or DPV2 making sure the fore-line pressure does not exceed 100 microns (GAUGE TC1) for more than 30 seconds. It. may be necessary to cycle the valves open and closed a few times.
, -5 The pump down will take about 5-6 hours to about 1 X 10 -3 -*-~~~ tII •• us. After the tank pressure has reached about 1 X 10 m.J,.-~ :IS (about 2 hours), fill the liquid N2 trap. Carefully monitor the filling of the large plate surrounding the filler hole. It has- an O-ring seal. Avoid spilling Ln2 around the filling hole. Ln2 could freeze the O-ring seal and cause a leak.
Glow Discharge
-5 ~.-e~ When the tank pressure is about 1 X 10 .~ ••• R8, initiate the glow' discharge procedure. connect an oxygen cylinder to the Kerotest valve on the tank feed-through. Set the pressure to 3-5 p.s.i. (Flush the air out of the hose before connection)
Isolate the tank by closing the main roughing valve RV1 and the gate valves DPV1 & DPV2 on both D.P.s. Crack the kerotest valve very slowly and let the pressure as read on gauge TC6 rise slowly to 30 microns.
11
200 JrDi All.f!l - Revised 9/21/91 - RPT
Turn on glow discharge (control console) and run current up to 10 amps (200 V) for 3 minutes. Monitor and control the current button (up - down) as the current can fluctuate fast and considerably. Observe the glow discharge through the port if the there is a lot of arcing, lower the current a bit, but not so low that the glow cannot be seen.
After glow discharge, open the roughing valve RV1. After a couple of minutes the pressure should be less than 10 microns Open the D.P. gate valves DPV1 &: DPV2 one at a time; the fore-pressure as measured at gauge Tel, should not exceed 100 microns - as before.
Repeat the Glow discharge 6 times. After each cycle, the pressure should return the previous value in 20 - 25 minutes or so. Proceed to next cycle.
-5 After last glow discharge, wai t for vacuum to be near 2 x 10 m~1C
~:I;3S. Make sure the liquid nitrogen trap is full.
Filament Firing
Activate paired firing circuits. Set the Variac to 105 volts. Install clamp-on ammeter and the chart recorder clamp-on ammeter to monitor proper time on of filaments. Note: you will be moving the rotary selector though 360 degrees - 0 - 180 paired filaments, avoid getters marked G (obsolete).
Prepare chart recorder.
Attach the recorder's clamp-on amp meter to one of the firing lines. This meter will not give any indication while plugged into the recorder. Use another meter, attached to the same line, to calibrate/measure/check current as recorded on the chart.
Check that there is at least a 1(4 roll of chart paper in the recorder.
I , Put the 'v/mv' to the 'v' position.
Put the 'var/cal' to the 'cal' position.
Put the 'h/o/min' switch to the 'hI position.
Put the 'speed' selector to 'I' position.
Put the 'range' switch to the 10 volt position.
Put the 'm/o' to the '0' position.
Install recorder pen.
Turn on the Power
12
200 lOOi ALL.'I! - Revised 9/21/91 - I::?T
Use the green knob to align the pointer to zero on left side.
swttch the 'm/olswitch to the 'm' position.
Record the gauge readings on the log-sheet.
Set the Variac to 105 volts and turn it on.
Set the recorder speed to 10cm/hr and volts to 2V. This should give a recorded first spike that may be off the paper, but the melt-in/firing waveform will be large enough (peak to peak) to read easily.
When firing the filaments, switch the recorder speed from 'hr' to 'mini and then back - this saves paper.
Set the rotor switch to the filament pair to be fired.
While watching the recorder, press and hold the firing switch button. The current will surge and then drop and then slowly rise again as the aluminum melts and then begins to vaporize. As it starts to drop off linearly and gets just below the low point that was reached after the spike, release the button - this s6buld take about 8 to 10 seconds. A timer will turn off the supply automatically after 12 seconds.
Note the filament number on the recorder paper as each filament pair is fired.
Continue until all filament pairs have been fired.
13
200 l~ AlJ.l'I1 - Revised 9/21/91 - Ji?T , ':>
FAST FIRING OF FILAMENTS
Immediately after paired firing, prepare for fast fire. Put Variac at 68 volts and turn the Variac circuit breaker on. Throw the knife switches in prescribed pattern as below:
Tine (sec.) 0 1.7 3.3 5.0 6.6 8.3 10.0 11.6 13.3 15.0 16.6 18.3 20.0
~ife en 1-2 1-2-3 2-3-4 3-4-5 4-5-6 5-6-7 6-7-8 7-8-9 8-9-10 9-10 10
~ife off 2 3 4 5 6 7 8 9 10
Thus each knife is closed for 5 seconds, the time deemed correct to prevent filament being heated while bare of aluminum (1987).
This value was determined by activating the circuit - knife # 1 and watching through the window port for telltale visual evaporative process. This time may vary slightly according to filament age, aluminum contact initially etc. However in failure of 1987 aluminizing, the timing was grossly off. The filament was on for 9 seconds, for 4 of those seconds the filaments were bare of aluminum. - Earl Emery
14
200 ltci Al1."'1 - Revised 9/21/91 - RPT
SHUTDOWN
Close North and South gate valves DPVl & DPV2 to the manifold.
Turn off the North & South D.P.s as well as the Booster D.P.s.
Turn off the Intermediate and Safety bypass D.P.s.
Note - do not close the main roughing pump valve RVl until the intermediate and the emergency bypass D. P. s have cooled. The blower and roughing pumps must back these D.P.s. until they cool.
When all Intermediate and the Safety Bypass D.P.s have cooled:
Close main roughing valve, RV1.
Turn off the blower pump.
Turn off all ion gauges.
Introduce oxygen to the tank through the Kerotest valve at about 3-5 p.s.i. Use one bottle.
"& After oxygen, introduce air to the tank through the filter port.
Turn off water flow to D.P.s and roughing pumps.
Disconnect gauges to tank.
Disconnect water hoses to tank.
When temperatures of North, South and the Booster D.P.s reach ambient temperature.
Close valves IN THIS ORDER, BV1,BV2,FV1, RV2, RV3 and RV4.
Turn off the roughing pumps.
Turn off all TC gauges.
Turn off refrigerant condensors.
After 30 minutes, turn off water flow to roughing pumps.
15
200 I;fjj .:J:u.l - Revised 9/21/91 - f:FT
pump-down log sheet
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Roque de Los Muchachos
Presentation by B. Mack
Summary Presentation: The Current Plans for Future Observatories
Contents:
1 . Columbus Project 2. Gemini Project 3. JNLT 4. Magellan 5. VLT
B. Atwood K. Raybould M. Nakagiri A. Schier M. GrossI
Columbus Project
Presentation by B. Atwood
The Columbus Report
ESO Workshop:
Cleaning and Coating Large Mirrors
Eso Headquarters, Garching
7 and 8 October 1991
Bruce Atwood and Barry A. Sabol
I Columbus Aluminization Configuration
II Aluminization Experiments-The Columbus List
ill Aluminization Experiments at Ohio State
1. Our equipment Diffusion Pump system Thickness monitor RGA Power supply and transformers Monochromator with
absolute reflectance accessory 2. Gas evolution during aluminization 3. Effect of background gasses on reflectivity 4. Pumping schemes 5. Filament geometry and source function 6. Power supply strategies
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ALilldINIZING EXPERTh1ENTAL AND DESIGN ACTIVITIES
(version 25 March 1991)
Improved Optimization of Filament Locations
• w / 0 baffles • w/baffles
.0". w / baffles and plasma • increase to 5 rings • optimize in single filament plane
Model Aluminum Distributions vs. Reality
O. comparison of model to chamber thickness measurements .
• thickness measurements by transmission
Verify the Properties of "higher density" and "astronomy standard" aluminum coatings
[samples from Las Campanas] [samples from Italy] [samples from Sunnyside] [samples from :MM:T small chamber]
• higher reflectivity • lower emissivity • washability (snowability)
Study Aluminizing in Argon
• reflectivity vs argon pressure • reflectivity vs oxygen pressure • profile variations from scattering • ionization of the argon?
Study Plasma-Assisted Aluminizing
• reflectivity and adherence measurements • ion assisted aluminum properties .• antenna design • special chamber requirements
Chemistry and Logistics of Coating Removal
• quantify the aluminum removal recipe from silica • quantify the silver, gold, chrome removal recipes • conduct experiments with potassium ferro cyanide • conduct experiments with Printed Circuit Board
etchant • quantify the effects of the silica recipes on E6
- long term damage tests - aluminum removal rates
• consider alternate removal schemes • integrate coating removal into cell design • design edge seal in detail (polish the edge) • design scheme to apply chemicals to the mirror • design scheme to clean the mirror
Impact of Mirror Support and Ventilation on Coating
• measure leak rates of mirror supports • measure leak rates of ventilation units • measure leak rates of the honeycomb structure • quantify the contaminants • estimate the tolerable leak rates in dirty vacuum • measure leak rates of butyl rubber seals • estimate the tolerable leak rates in clean vacuum
Filament Power Considerations
• measure filament transformer properties • price high current feedthroughs • design and build filament power supplies • estimate standard filament power and load • measure leak rates of transformers
Pumping Designs
• estimate required pumping speed • quantify getter pumping scheme • cryopanel design and test . • experiment with hydrogen gas effects • compare commercial cryopumps to cryopanels
Chamber Design
• specify number and location of ports • specify flange configuration • chamber testing requirements • interior coating (epoxy, AI, stainless, Ni ?)
Bell Jar Preparation and Handling • design fixtures for filaments and pumps • develop loading procedure • study integration of cleaning and coating procedure
ALUMINIZING EXPERllvIENT AL AND DESIGN ACTIVITIES
(version 25 March 1991)
Improved Optimization of Filament Locations
Model Aluminum Distributions vs. Reality
Verify the Properties of "higher density" and "astronomy standard" aluminum coatings
Study Aluminizing in Argon
Study Plasma-Assisted Aluminizing
Chemistry and Logistics of Coating Removal
Impact of Mirror Support and Ventilation on Coating
Filament Power Considerations
Pumping Designs
Chamber Design
Bell Jar Preparation and Handling
BASELINE liST OF ALIDv1INIZING SYSTEM FEATURES
250 -- 300 filaments, 400 -- 600 Watts each
··4 -- 5 rings of filaments
Filaments in a single plane
1.0 -- 1.5 meters above the mirror
Filament shutters and baffles
Dedicated low voltage wiring to each filament
Strip mirror horizon pointing
Install chamber horizon pointing
Clean mirror horizon pointing
Aluminize horizon pointing
Chamber divided into clean / dirty sections
Blowout valve between sections
Roughing Pumps: Roots blowers backed by rotary pumps
HiVac Pumps: Cryopumps or Cryopanels
Residual Gas Analyzer
Quartz Crystal Thickness Monitors (- 8)
Pressure Gauges
Bleed Valves
Edge Seals for ventilation, washing, aluminizing
Dual O-ring flange seal in keystone groove
3 . -- 4 one meter vacuUm ports on the top hat
Dummy mirror cell baseplate with 1.0 meter op'ening
Thermocouple readout system (shared with telescope?)
078 Ohio State/Colum:bus Proiect
1E ~----------------------------------------~ ~totaI ~a6E-7
2 3
: : · . : : · . · . · . · . : ~
4
· .-· ·
5 6
tE-iO+,----~----~--~----~--~----~--~~--~ 0.00 0.50 1.00 1.50 2.00 2.50 3.00 3.50 4.00
Time (minutes)
101
Ohio State/Columbus Project 1E~6~------------------------------------~
-c- 1E-07 ~ ",. AMU16 0
1::.. CD
AMU15 "-::l en AMU14 en 1E~8 CD ~
a.. co t:: AMU13 co a..
(Ratios as expected for Methane)
1E-10+---~--~--~~--~--~--~--~--~--~ 0.00 0.20 0.40 0.60 0.80 1.00 1.20 1.40 1.60 1.80 2.00
Time (minutes)
'C" >-o l:::-CD '-::s U) U) CD '-a.. ca 1:: <1l a..
1.0~
Ohto State/CotulT-lDUS Project
AMU28
AMU29
AMU30
AMU27
1 E-1 a Initial total pressure 1 E-6 0.00 0.20 0040 0.60 0.80 1.00 1.20 1.40 1.60 1.80 2.00
Time (minutes)
012 Ohio State/Columbus Project
lnitfaa total pressure 7.3E-7
1E-O ......... _-
AMU 78 (A/(OH) 3?)
1E~~~~~~~~----~------~----~----~ 0.00 0.50 1.00 i.50 2.00 2.50 3.00
Time (minutes)
1E-04
lE-05 :;:
Q) 1E-06 ... :: ::J en en Q) '--a.. . ttl t:: ttl 0..
:: ---
1E-07 = . : --
1E-08 ~ = : --
1E-09 0.00
104 Ohio State/Columbus Project
Jrnttab tofal! Pressure 9E-7 85& Angstroms deposited
H2
V H2O
J
~ - ..... V .
0.50 1.00 1.50 2.00 2.50 3.00 Time (minutes)
~ '--
~
087 Ohio State/Columbus Project
Initial total pressure 8E-6 Small ait ·feak Note 02 gettering
~ 1 E-06:::r--__ --9-
:::l en en CD "-
~ 1E-07 H~
t:: ctS a..
iE-08
1E-09+---~--~--~--~--~~--~--~--~--~ 0.00 0.50 1.00. 1.50 2.00 2.50 3.00 3.50 4.00 4.50
Time (minutes)
----0 c CD -:J
'UJ fI) CD -CL as 1:: as 0...
1E-05
1E-06
1E-08
1'00 Ohi:Q State/Col:umbu.s Project
H 2
1E~'+---~--~--~--~~--~--~--~--~--~ o. 00 5. 00 10. 00 15.00 20. 00 25. 00 30.00 35.00 40.00 45.00 50.00
TIm"a- (minutes)
106a1pt Ohio State/Columbus Project
Initial total pressure 7.8E-6
1E-08
1E~+---~----~--~--~----~--~----~--~ 0.00 2.00 4.00 6.00 8.00 10.00 12.00 14.00 16.00
Time (minutes)
c "-0 t::. CD "-::l tn tn CD "--a..
ctS t: <tS a..
1E-05
1E-06
1E-07
1E-08
1E-09
{)"o~ Qlaalpt
Ohio State/Columbus Project
Very low initial H2O
H 2
. ... _ ....
HO 2
1 E-1 O-t---,-----r--~----r-~--r____-~-_,__-_i 0.00 0.50 1.00 1.50 2.00 2.50 3.00 3.50 4.00 4.50
Time (minutes)
Ohio State/Columbus Project 1.00E-OS_
- 0 --
-c--a C.
--& -:l -(I) (I) 0 CJ)
0 - 0 c-as 1.00E-06:
0 0 r
as 0 0 CL -- 0 CIt C -as ~ (ij --c
"-
1 . OOE-07-t-----r---....-.,--1..,--,.11--r-T""'"T'-'.------,I..----.---,,.---,---r"""T"""l~
1.00E+02 1.00E+03 1.00E+04 Reaction time (seconds)
I Columbus Aluminization Configuration
II Aluminization Experiments-The Columbus List
, "
m Aluminization Experiments at Ohio State
1. Our equipment Diffusion Pump system Thickness monitor RGA Power supply and transformers Monochromator with
absolute reflectance accessory 2. Gas evolution during aluminization 3. Effect of background gasses on reflectivity 4. Pumping schemes 5. Filament geometry and source function 6. Power supply strategies
Coating Thickness. Distribution Helical Fifament
1.20...,.....-----------i ------------, I 90
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~ 0° •. 4060
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Azimuth
• 30 60
- ... Elevation=90 ······8····· Elevation=67.5-··EJ····· Elevation=45
... 3-.... E1evation=22.5 ······8-·· Elevation=O
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Gemini Project
Presentation by K. Raybould
1. Start anagressive program, to de.n1onstate the· feasibility of producing durable lo.wemissivity coatings. . .
2. Investigate methods for cleaning the primary mirror in-situ.
1. SCIENCE REVIEW MEETING IN US 18119 JULY 1991 .' .. .
Concluded that one of the highest priority for the Gemini project is'the capabifity to' deposit low emissivity durable coatings.
Tef,escope emissivity specification 40/0 . (excluding scattering and sky contribution) .
..
Te~escope emissivity can degrade to 5% before the mirror emissivity must be reduced to the post coating level.
Target emissivity of 2%.
SCIENCE REQUIREMENTS· .
GEMINI DEVELOPMENT PLAN FOR LOW EMISSIVITY COATING
IN-SITU MIRROR- CLEANING
-
PROGRAM FOR DESIGN, PROCUREMENT, INSTALLATION AND COMMISSIONING
Primary mirror (silver coated)
Secondary mirror (silver coated) , C.' '
. . .;
O.Smm bevel around secondary mirror
. Secondary mirror support vanes (12mm) 0.40/0
Primary mirror bore (hole in centre) 0.00/0
Diffraction, at edge of secon.da,ry(1 0 microns)..O.2%
Scattering off mirror surfaces (APART) ? .
Other sources ? .
LOW EMISSIVITY DURABLE COATING I . DEVELOPMENT PROGRAM I
~:.;.:.;.;.:-:.;.:.:.:.;.:.;.:.:.:. ," '-:.- .:."': ',' {o ..... • ...... ,'. :.' '.' .................. .; ••••• ;. •• ;.;.; •••••••• : ... ;.:.: •••• :.:.:.: ..... x-............. ,':. ";';' ... :' ',' .. • ••• ,' ... ',' • .;.:.,' ..,." .... : .•.•.. ,' .•.•. : ...... ',' .••....• : •. { .. ·····ti::;:i:·:i<i·:·:·:f·:·:·:~f,.:-;k·:·:·:(ifu·:#?:.?,:. ·:"'f
AIMS-
1. Literature search on potential coating tech~iques. Silver is the prefered film for its low em'issivity in the IR.
2. Small scale testing of a few promising te~hniques. Durability of coating to be tested with accelerated environmental testing. .
3. Coat 1.3m IR telescope optics.
4. Ift-3 are. successful, investigate methods of boosting the relectance fn the blue and UV end of the spectr'um.
5. Develop methods for cleaning the primary mirror in-situ.
,PROGRAM FOR DESIGN, PROCUREMENT r :'
INSTALLATION AND. COMMISSIONING ; ":O;:::X:;·::;::·:-:::·:·:·:·;·;::~'~'··:·.~·· '.:.' '''; . .;>; •• : ..... ;.: '.:.:..:v:' .... .., :,:,,:-:.:.;.:« . • .,<. • • ,', ...... ;.0: • •••• ',.. •• •• :««.. . "'. :« . 'oX • y: "';:'.. .• . 'v..: :.:.;.: .. 0:-' ....... :.: ... : .... \.-:-».: ...... :-:.«;. :: .... :::
.1. Develop sputtering process hardware design for ~esting in the 4.2m chamber. ' . - .
2. Design and specification'
3. Procurement
4. Test assembly at manufacturers
5. Ship
6. Assemble on site
8. Coat primary mirror
uv LAS
ER-C
l.l~
ANiN
Q: O
F A
ST
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NO
MIC
AL
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LE
SC
OP
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IRR
OR
S
Con
tact
: .
Dr. W
ayne
:',K
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a:
STI
Op,
tron
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27
55 .N
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Bell
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(206
) 82
8-35
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CU~RREMTSTATUS
• T
echn
ical
Iss
ues
Rel
ated
to
Las
er C
lean
ing
Ast
ron
om
ica
l Tel
esco
pes
Det
erm
inin
g o
ptim
um
tech
niq
ue
(e.
g.,
lase
r pu
lse
ener
gy,
# o
f sh
ots
/site
, p
uls
e r
epet
ition
rat
e) -
de
pe
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s on
co
nta
min
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t
Sol
ving
eng
inee
ring
issu
es s
uch
as
be
st m
eth
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fo
r de
liver
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lase
r be
am a
nd r
emov
al o
f exp
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d d
ust
• S
TI O
ptr
on
ics
is In
tere
sted
in W
orki
ng W
ith O
bs'e
rvat
orie
s to
Dev
elop
T
his
Ap
plic
atio
n
Col
labo
ratin
g w
ith
Uni
vers
ity o
f Was
hing
ton'
AS
tron
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De
pa
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en
t on
join
t pro
po
sal'
In d
iscu
ssio
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wit
h N
atio
nal O
ptic
al A
stro
no
my
Obs
erva
tory
-P
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e co
nta
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ayne
Kim
ura
at S
TI O
ptr
on
ics
for
mor
e in
form
atio
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I
·.·STi·
to#mC
:>NI@
··
, BAC
KGR
:OU
,N:D
• T
ele'
seap
e M
irro
rs D
eg
rad
e'O
vert
ime
:
Incr
ease
of e
mis
sivi
ty a
nd s
catt
erin
g, d
ecre
ase
of r
efle
ctiv
ity
Rec
oatin
g la
rge
dia
me
ter m
irro
rs e
xpen
sive
and
ris
ky
Nee
d b
ett
er i
n si
tu c
lean
ing
tech
niq
ue
s
• P
ossi
ble
Sol
utio
n:
Use
Las
.er C
lean
ing,
Cap
able
of e
asy
and
sf:lf
e in
situ
cle
an
ing
.
Fre
quen
t cle
anin
g po
ssib
le (
e.g.
, da
ily)
-en
sure
s co
ntin
ual
op
timu
m te
lesc
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e p
erf
on
na
nce
.
.
Cle
an d
uri
ng
da
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min
imiz
e te
lesc
ope.
do
wn
time
,
.',
• U
V L
aser
Cle
anin
g o
f Sm
all Diame~er M
irro
rs H
as A
lread
y B
een
Dem
onst
rate
d
UV
lig
ht b
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han
visi
ble
or
IR l
igh
t
Exc
imer
UV
lase
rs r
eadi
ly a
vaila
ble co
mmer
cial~y STlt~IH _·_
.. CS
RE
VIE
W O
F B
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IC C
LE
AN
ING
ME
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• M
elec
ular
Con
tam
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val '
P
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chem
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dis
soci
'atio
n
• m
ole
cula
r bin
din
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nerg
ies
are
typ
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lly s
ever
al e
V
• ea
sily
bro
ken
by: ~V Ji
gta~
. P
hoto
ther
mal
pro
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'.,
....
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ire
ct a
bso
rptio
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f UV
lase
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by
con
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nt
• m
inim
izes
lase
r ene
rgy
need
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sur
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• P
artic
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emov
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. . .
Ab
sorp
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Gen
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ion
of o
pto
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s w
ave
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nce
off
sur
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. .
• re
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s pu
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lase
r sou
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suc
h as
an
exc
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r la
ser
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Ele
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stat
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or
Effe
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KITT PEAK NATIONAL OBSERVATORY
SCHEDULES AND STAFFING
FOR MAINTENANCE OF TELESCOPE OPTICS
COATING SCHEDULES:
ALL TELESCOPE OPTICS ARE REALUMINIZED ONCE A YEAR EXCEPT
FOR THE 2.1 METER AND 4 METER TELESCOPES. DUE TO THE TIME . . .
AND EFFORT REQUIRED FOR REALUMiNIZING THE 2.1 METER AND 4
METER TELESCOPE OPTICS, THEY ~E BEING REALUMINIZED EVERY .
THREE TO FIVE YEARS.
WASHING SCHEDULES:
ALL TELESCOPE MIRRORS ARE WASHED A MINIMUM OF ONCE EVERY
SIX MONTHS.
STAFFING:
• PART TIME SERVICES OF ONE ENGINEER FOR SCHEDULING AND TECHNICAL SUPPORT.
• PART TIME SERVICES OF TWO TRAINED TECHNICIANS FOR WASHING, COATING, AND OVERSEEING ALL MIRROR HANDLING.
• PART TIME SERVICES OF REGULAR MOUNTAIN OPERATIONS TECHNICIANS TO ASSIST IN MIRROR REMOVALS.
KITT PEAK ALUMINIZING CAPABILITIES
2.4 METER & 4 METER COATING CHAMBER FACILITIES
I. Both coating chambers are pennanently installed in fixed locations
(aluminizing rooms) and all optics are transported to the aluminizing rooms
for coating.
. . II. The aluminizing rooms are fully equipped to handle all mirror operations.
Each room has overhead cranes to handle the optics and washing facilities
for stripping and cleaning the mirrors.
III. It has been· Kitt Peak's experience that the use of stationary coating , "
chambers and fully equipped aluminizing rooms has provided quick turn-
around times and minimum down time due to equipment failures. About
the only maintenance required on any. of the chambers is the standard
preventive maintenance activities.
NOTE
Originally, the 4-meter chamber was designed to be moved to the main floor of the 4-meter building for aluminizing the primary mirror and the mirror was to be installed in the chamber on its cell. In practice, it was found to be much easier, quicker, and safer to remove the mirror from its cell and transport the mirror to the chamber on the ground floor of the building.
COATING CHAMBER DETAILS
1. Only aluminum coatings are currently being done in both chambers.
2. Both chambers are only capable of using filament arrays for evaporations.
3. Both chambers are using diffusion pumps and meissner traps.
4. Only the 4·meter chamber has glow discharge capabilities which is not
currently in use.
s. Both chambers have never experienced any major mechanical problems in
over twenty years of use and the coatings produced in both chamb_ers are of
equal quality.
PERFORMANCE Of COATING CHAMBERS
4 METER CHAMBER
DESIGN PERFORMANCE SPECIFICATION;
Coating Uniformity: ±5%
Depositio~ Thickness: ~loooA
DELIVERED PERFORMANCE;
Coating Uniformity: ±27% thickness variation under the best conditions.
Deposition Thickness: Maximum thickness seldom approached 800A (Usually 400A - 600A)
CURRENT PERFORMANCE;
In 1985, modifications were made to the filament· arrays, the filament baffles, and power distribution circuit.
Coating Unifonnity: Better than ±lO%.
Deposition Thickness: Approximately loooA
2.4 METER CHAMBER
DELIVERED AND CURRENT PERFORMANCE:
Coating Uniformity: ±lO%
Deposition Thickness: 800A - lDOOA
4 METER CHAMBER MODIFICATIONS
FILAMENT ARRAY ARRANGEMENTS:
ORIGINAL FILAMENT CONFIGURATION
MODIFIED FILAMENT CONFIGURATION
BAFFLE ARRANGEMENT:
The baffles were catching much of the evaported material.
The baffles were raised closer to the filaments increasing the angle of incidence of the deposition on the substrate from 20 degrees to 45 degrees.
PERFORMANCE:
The ±10% coating uniformity achieved with these changes was adequate for all known NOAO coatings. The cost for further uniformity improvements was prohibitive.
MIRROR REFLECfIVITY MEASUREMENTS FOR REALUMINIZED MIRRORS
TELESCOPES CHAMBER 3500A 5500A ?JJJJ.JA
WIYN 3.5M 4 METER 91.7% 89.5% 95.3%
0.9M 4 METER 85.2% 87.1% 94.9%
U of A (2M) 41v1.ETER 88.7% 89.0% 95.4%
#1 VACUUM 2.4 METER 89.2% 90.3% 95.4%
#2 VACUUM 2.4 METER 88.1% 90.2% 95.7%
McMATH MAIN #1 2.4 METER 89.5% 90.3% 95.4%
McMATH WEST AUX #1 2.4 ME1ER 88.5% 90.5% 95.9% !
. r : ,
McMATH EAST AUX #1 2.4 MElER 90.0% 90.2% 96.2%
COUDE FEED #2 2.4 METER 88.5% 89.5% 95.7%
MIRROR CLEANING PRIOR
TO ALUMINIZING
1. ALL LARGE TELESCOPE OPTICS ARE STRIPPED AND CLEANED IN
THE ALUMINIZING ROOM.
2. THE MIRRORS ARE REMOVED FROM THEIR HANDLING CARTS OR
CONT A1NERS AND PLACED ON STANDS OVER THE FLOOR DRAINS
FOR STRIPPING AND CLEANING.
3. IMMEDIATELY AFTER THE MIRRORS HAVE BEEN CLEANED THEY
ARE PLACED IN THE CHAMBERS FOR COATING.
4. THE COATING CHAMBERS ARE PREPPED AND READIED FOR
FIRING PRIOR TO BRINGING THE MIRRORS INTO THE ROOM FOR
CLEANING.
PROCEDURE FOR STRIPPING AND CLEANING MIRRORS PRIOR TO ALUMINIZING
The following solutions are used in this process:
Solution "A":
Solution "B":
Solution "C":
Mix Hydrochloric Acid (HCL, 37%), Reagent grade, with distilled water in a ratio of 1: 1.· Then add 28 grams of Copper Sulfate (CuS04), Reagent grade, per liter. of solution and shake until dissolved. .
Mix distilled water with Potassium Hydroxide (KOH), Reagent grade, in a ratio 20: 1 and shake until dissolved.
Mix Nitric A~id (HN03' 70%), Reagent grade, with distilled water in a ratio of 1:1.
1. Rinse mirror' thoroughly with filtered tap water.
** Wear Protective Rubber Gloves for the Following Steps **
2. Remove any oil spots with Acetone or Xylene. 3. Apply Solution "A" to mirror surface. Using lint-free tissues soaked in solution
"A", rub the surface briskly to remove the coating. 4. Rinse mirror thoroughly with filtered tap water. 5. Repeat steps 3 and 4 until old coating is completely removed. 6. Apply solution "B" to mirror surface and rub briskly with lint-free tissues. 7 . . Rinse mirror thoroughly with filtered water. 8. Reapply solution "B", spread a light coating of Calcium Carbonate (Reagent
grade) over the entire surface, and rub the surface with lint-free tissues. 9. Rinse mirror thoroughly with filtered tap water.
10. Repeat steps 8 and 9 several times. 11. Apply solution "c" to mirror surface and rub briskly with lint-free tissues. 12. Rinse mirrior thoroughly with filtered tap water for 5-10 minutes.
** Remove Gloves **
13. Apply enough distilled water to thoroughly rinse off tap water. 14. Wipe surface dry with lint-free tissues. Do not let standing water air-dry on
surface. 15. Use filtered gaseous nitrogen (Nz) to blow off any dust or lint. 16. Mirror is now ready for aluminizing.
TELESCOPE MIRROR WASHING
CURRENT PRACTICE (ALL TELESCOPES):
1. Mask off surface of mirror from rest of telescope with plastic sheeting and tape.
2. Position telescope to permit wash solution to drain out holes provided for water removal.
3. Wash mirror in accordance with the approved wash procedure (see attachment).
4. Remove any excess water from the cell area with a wet or dry shop vacuum cleaner.
5. Remove plastic sheeting.
EXPERIENCE:
For several years strippable plastic coatings were successfully used for
cleaning mirrors, but has been discontinued due to the potentially
hazardous chemicals some of them contain.
CLEANING PROCEDURE FOR COATED MIRRORS
1. Required Supplies:
a. Two 20-liter, hand-operated, pressure sprayers. b. Two liters of reagent grade alcohol. c. One tablespoon of Alconox (Phosphorus-free detergent soap). d. . Ten liters of distilled water. e.One half liter of acetone or xylene. f. Several clean sponges. g. Several boxes of lint-free tissues.
II. Cleaning Procedure:
a. Clean spray containers thoroughly with distilled water and alcohol.
b. Fill "Rinse" container
c. Fill "Wash" container
d. Use acetone or xylene to remove any oil stains.
e. Spray mirror with "Wash" until all loose particles are removed and gently rub surface with wet sponges.
f. Spray with "Rinse."
g. Use tissues to tamp surface dry. DO NOT RUB!
PRIMARY MIRROR HANDLING
2.1 & 4 METER J'ELESCOPES
MIRROR REMOVAL AND INSTALLATION:
1. THE LARGE TELESCOPE MIRRORS ARE REMOVED AND
INST ALLED WITH THEIR CELLS ONTO MOBILE HANDLING CARTS.
a) 4 METER USES THE 4 METER COATING CHAMBER CART.
b) 2.1 METER USES A SEPARATE CART DESIGN SPECIFICALLY
FOR THE TASK.
MIRROR HANDLING FOR WASHING, AND COATING:
1. THE LARGE MIRRORS ARE HANDLED SEPARATELY WITH THE AID
OF OVERHEAD CRANES AND CENTER LIFTING FIXTURES FOR
MOVING THEM ON AND OFF OF THEIR CELLS, INTO THE
CLEANING BAY, AND ONTO THE COATING CHAMBER CARTS FOR
ALUMINIZING.
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an 8 .. moptical .. infrared telescope project
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m Outgasing the Vacuum Chamber
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VLT
Presentation by M. Grossi
VL T MIRROR MAINTENANCE CONCEPT
GENERAL
OBJECTIVES:
• Maintaining High Optical Performance - specular reflectance - homogeneity - long term stability
• Safety - personnel
. - mirrors
• Reliability
ESOIVL TIMGRlwrkshpt 111. 1
VL T MIRROR MAINTENANCE CONCEPT
GENERAL
REQUIREMENTS for PRIMARIES (TERTIARIES) exposed to dirty environment
• Broad Band Reflectance (i < 1 OO) R > 86 % from 300 nm to 20 pm
• Homogeneity better 0 / -1 %
• in situ optical performance control
• Coating Renewal • in situ Cleaning
• Standard Coating: Aluminium
• Coating Options: - Improved Mechanical Stability - Improved Reflectance
ESO/VL T/MGR/wrkshpt 1/1.2
VL T MIRROR MAINTENANCE CONCEPT
GENERAL
REQUIREMENTS FOR OTHER MIRRORS placed in environment with contamination control
• Broad Band Reflectance R > 96 % from 500 nm to 20 Jim R > 80 % from 300 nm to 500 nm
• Long Term Stability > 15 a
• Wear (abrasive) Resistant Surface
• in situ optical performance control
• in situ Cleaning
ESO/VL T/MGR/wrkshpt1/1.3
VLT COATING RENEWAL
PRIMARIES (AND TERTIARIES)
REQUIREMENTS
• Handling Concept
• Coating Renewal Procedure - Coating Removal - Mirror Cleaning - Coating
• Safety
• Reliability
• Telescope. Down Time < 48 hours
• Consumables
• Investment
ESO/VL T/MGR/wrkshpt 1/2. 1
VL T COATING RENEWAL FOR PRIMARIES
HANDLING CONCEPT
REQUIREMENTS (Mirror Maintenance Building MMB 1.8 km for from telescopes)
• Procedures - Dismounting the Cell from telescope - Attachment of Coverage - Dismounting M3-Tower - Transfer Cell to MMB - Dismounting Mirror from Cell - Transfer Mirror to Coating Carrier
• Mirrors covered and horizontally faceup during all handling operations
• Handling Devices - redundant - self-aligning - force control for movements
• Reliability, Safety
• Duration: < 10 hours
• Personnel Requ: 2(1) mechanician 1 mech.operator 1 controller
ESO/VL T/MGR/wrkshpt 1/3. 1
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VL T COATING RENEWAL FOR PRIMARIES
HANDLING CONCEPT
Out-ot-Cell Procedure: ADVANTAGES
• Simple single vacuum vessel
• minimum vessel volume (~ 80 m 3 for substrate + carrier)
• consequent high vacuum design of substrate carrier
• Simple long term storage
• high reliable vacuum quality and thus coating quality
• mirror washing on eye level
• No risk of chemical attack for the cell due to washing
• No vacuum requirements for M-Cell
• No delicate alignment and sealing procedure for the mirror
Out-ot-Cell Proc: DISADVANTAGES
• Dismounting the mirrors out of cells
• Mirror handling from cell to carrier
ESO/VL T/MGR/wrkshpt 1/3.2
VL T 8M-COATING UNIT
LOADING CONCEPT
DRAWER CONCEPT: Advantages
• Minimum Volume and vacuum exposed surface in loading section
• Simple Substrate Carrier integrated in vacuum vessel design
• All lubricated eleme.nts (wheels, drives, gears, damping elements) on atmospheric side
• Natural barrier against carry-in of dirt from floor
• No vacuum area safety risks for Personnel
DRAWER CONCEPT: Disadvantages
• Contamination risk during washing
• Prolonged air exposition for vac vessel
• Additional vertical movement for closing the coating chamber
ESO/VL T/MGR/wrkshpt 1/4. 1
fLT 8M (oafi)1g {)J111
LOAlJING CONCEPT
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VL T COATING RENEWAL FOR PRIMARIES
FILM REMOVAL AND MIRROR CLEANING
CONCEPT
• Cleaning rear and side surfaces
• Automated front side treatment - purging away dirt, dust, bird
droppings, oil and grease - removal of old coating - chemical neutralizing - drying
• Particle contamination control - drying - mirror loading in coating plant
• Pre-cleaning prior to coating (in vacuo)
ESO/VL T/MGR/wrkshpt 1/5. 1
VL T COATING RENEWAL FOR PRIMARIES
FILM REMOVAL AND MIRROR CLEANING
PROCEDURE
• Cleaning rear and side walls, lateral pads, axial tripods: - manually with alcohol - in lifting area - while M 1 is hanging, prior to front
side treatment
• Crane operation: Setting mirror on Coating Cart, removal of lifting tool and top cover
• Moving mirror into Washing Area (coating carrier on rails)
• Allow recovery of contamination control
• Attachment of Washing Unit (manual) - mirror hole plugged tightly by
collecting tank - Spilling protection on outer mirror
edge
ESO/VL T/MGR/wrkshpt1/S.2
VL T COATING RENEWAL FOR PRIMARIES
FILM REMOVAL AND MIRROR CLEANING
PROCEDURE (cont'd)
• Machine process for AI-Coatings
- Soaking and large o Tap water rinsing, dirt removal: (recycled)
- Dirt removal, o 3x detergent, 50 0 C
(mechan .lchem.) Jet spraying
- Detergent o 2x Tap water rinse removal o 1 x Tap water spraying
- AI - film o 2x NaOH, 5% aqu. removal rinsing (recycled)
- Lie residues, o 1x HCI, 5% aqu. O-Iayers removal + CuSO 4, rinsing
- Neutralizing o 1 x buffer (e.g. NH40H)
5.5 < pHf < 6.5 o 3x H20 dist.,rinse
- Drying o 1 x Ethanol, rinsing
o 2x Ethanol> 96%, rinsing, fresh
o air draught support
(sucking or blowing)
ESO/VL T/MGR/wrkshpt1/S.3
". -
VL T COATING RENEWAL FOR PRIMARIES
FILM REMOVAL AND MIRROR CLEANING
PROCEDURE (cont'd)
• Motor driven removal of Washing Unit
• Opening contamination control area and loading Coating Unit
• Down-pumping to 1 x 1 0-3 mbar
• Pre-cleaning by Glow Discharge in air (~ 0.02 mbar)
ESO/VL T/MGR/wrkshptl/5.4
VL T COATING RENEWAL FOR PRIMARIES
FILM REMOVAL AND MIRROR CLEANING
MECHANICAL WASHING UNIT: Advantages
• Minimum wear load on mirror - well controlled mechanical purging
operation (spraying) - homogeneous permanent treatment
of surface - minimum duration (chemical action) - no contact of surface with solids
• stainless drying
• minimum liquid consumption (recycling)
• minimum particle contamination
• safe handling of aggressive chemicals and vapours
NOTE: Process can be fully automatic if no AI droplets have to be removed!
ESO/VL T/MGR/wrkshpt 1/5. 5
VL T COATING RENEWAL FOR PRIMARIES
FILM REMOVAL AND MIRROR CLEANING
MANAGEMENT PLAN
• Pilot Washing Unit (PWU) or < 3.6 m mirrors: Requirements
• PWU Engineering, • Manufacturing
external
• Process Development for AI Testing with 3.6m and NTT mirror
• Washing -Unit for 8 m mirrors: Requirements
• WU Engineering, • Manufacturing
external
• Installation in MMB
• Process Application and Tuning for VL T 8 m mirrors
ESO/VL T/MGR/wrkshpt 1/5.7
VL T COATING RENEWAL FOR PRIMARIES
FILM REMOVAL AND MIRROR CLEANING
CONTAMINATION CONTROL CONCEPT
• Washing in Clean Zone
• Clean Zone - completely separated from MMB - cleanroom class: < 5000 per cf - air exchange rate according to HEPA
filters « MAK requirements) - gowning and filter masks (MAK) for
personnel - starting procedure: complete cleaning
and switch on ventilation 3 days in advance
• Proper interface design: Clean Zone / Coating Unit
• Finishing washing with minimum personnel present (automatic removal of Washing Unit, automatic loading)
ESO/VL T/MGR/wrkshpt 1/5.6
VL T 8M-COATING UNIT
COATING TECHNOLOGY
C'()tsJ'~cfi(;)N Clean Zo,,~
tli"or tlaintel1C1nce Buildjng
ESO/VL T/MGR/wrkshpt 1/6. 1
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Spectral reflectance of various opaque metal films obtained at nearly normal incidence of the light beam. The films were deposited by evaporation in high vacuum. (according to Carl Zeiss, FRG).
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VL T 8M-COATING UNIT
FILM SYSTEMS
NEW COATINGS DEVELOPMENT PLAN
• Film layer design
• (small) Sample manufacturing
• Adherence, wear test MIL 13508C ( cheese-cloth rubbing)
• Accelerated aging (80 a C, 20%RH, 5 x 3 days)
• 1: 1 Coating Process Development
• Reflectance Measurement
• Removal Procedure Development
• Film density Check (Pt/C replica)
• APPLICATION
ESO/VL T/MGR/wrkshpt 1/7.2
VL T 8M-COATING UNIT
COATING -TECHNOLOGY
CDoting rJeofYletty ·lJori ~ iacf-()p) I "/' \
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ESOIVL TIMGRlwrkshpt116. 1
VL T 8M-COATING UNIT
COATING TECHNOLOGY
PVD TECHNIQUES used CURRENTLY on PRODUCTION SCALE for OPTICAL COATINGS
source type indicated substrate conditions
indicated
EVAPORATION Ion Plating (IP) Resistance heated Activated * Electron Beam heat * DC, RF Bias * Low Volt.Arc heat * Reactive * Hollow Cathode Arc Reactive IP (RIP)
SPUTTERING DC magnetron sp. RF sputtering RF magnetron sp. Ion beam sp.
Activated Reactive Evaporation Biased ARE High Rate Reactive Sputtering DC/RF Bias Sputtering
ESO/VL T/MGR/wrkshpt 1/6.2
VL T 8M-COATING UNIT
COATING TECHNOLOGY
COATING by EVAPORATION
• Emission characteristic of source type - coil (or basket) shape filaments
• Source arrangement after J. Strong - single source ring Osource > 0mirror - Os > 8.4 m - H > 4.2 m above mirror surface
• Moderate filament load (~ 1 5 mg/cm) minimizing droplet formation
• EI. Power .Requ: ~ 21 0 kW no. filaments: ~ 400
• Vacuum vessel (coating partition): D x H ~ 8.5 x 5.5 m
Volume ~ 300 to 340 m 3
vac exposed metal surface ~ 300 m 2
• Residual pressure: < 2 x 10-5 mbar
• In vacuo cleaning: Glow discharge
NOTE: AI alloys & wets; W stranded superior. No dielectric materials.
ESO/VL T/MGR/wrkshpt 1/6. 3
, , . ~ ,
Fig. 53 a Various types of resistance heated evaporation sources.
Fig
. 61
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VL T 8M-COATING UNIT
COATING TECHNOLOGY
RESIDUAL PRESSURE REQUIREMENTS
Common performance rule for optical coatings:
current density < gas atoms r G
4.37 x 105
10 % current density of film material r F
OF ......... film density [g/cm3] M F ••...... molar mass of film [g/mol] MG ....... molar mass of gas [g/mol] PG ....... residual gas pressure [mbar] T G ........ gas temperature [K] rD ......... deposition rate [nm/s]
Example:
rD = 10 nm/s, of(AI) = 2.7 g/cm 3,
Air 20°C
Result: PG < 2 x 1 0-5 mbar
ESO/VL T/MGR/wrkshpt 1/6.5
100
90
80 ...- 70 ~ 0 ---Q) 60 () c 50 ~ ...... () Q) 40
'+-Q)
30 a:
20
10
0
Fig.11
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I I A
/1 1\ V . 260 sec at 1,5 . 10-4 Torr
j
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'/
0,2 0,4 0,6 0,8 1,0 3,0 5,0 7,0 9,0 11,0 Wavelength (~m)
Reflectance of two AI coatings prepared under extremely different evaporation conditions in the wavelength region from 0,22 to 11 microns.
VL T 8M-COATING UNIT
COATING TECHNOLOGY
SPUTTERING: Advantages
• Vacuum vessel height/volume small HCh-SPUT ~ 2.5 m ~ 1/2.7 HCh-EVAP
V Ch-SPUT ~ 150 m3 ~ 1 /2.7 V Ch-EVAP
• Less foreline pumping capacity
• Low el.power requirement PSPUT < 1 /2 PEVAP
• Flexibility in film material Multi layer dielectric film stacks
feasible .
• No loading (high target lifetime)
• Reliable automatic process
• Excellent homogeneity (no droplets)
• Small scale simulation feasible
• Price (coating unit, transport, installations)
ESO/VL T/MGR/wrkshpt 1/6.6
VL T 8M-COATING UNIT
COATING TECHNOLOGY
SPUTTERING: Disadvantages
• Water cooling systems required
• Periodic Cleaning of sources (surroundings)
• Moving parts in vacuum close to mirror surface required
ESO/VL T/MGR/wrkshpt 1/6.7
VL T 8M-COATING UNIT
COATING TECHNOLOGY
PRECLEANING (in vacuo)
• By irradiation IR or UV - dedicated to substrate - dedicated to contamination
• By Glow Discharge - efficient - versatile . . - InexpenSive
ESO/VL T/MGR/wrkshpt 1/6.8
VL T 8M-COATING UNIT
PUMPING
REQUIREMENTS
• Residual pressure: ... < 2 x 10-5 mbar
• Working pressure (sputtering): ........... ~ 2 x 10-3 mbar
• Pumping Duration: ... < 4 hours
• Reliability (oil backstreaming)
SOLUTIONS
• Roughing with roots blower + rotary vane pump to > 0.08 mbar
• High vacuum pumping with High Vac Pump + Meissner Trap: - Bath-cryo pump - Diffusion pump with LN2 Baffle
(Silicon Oil DC 704) (- Refrigerator cryo pump)
- Throttle position for Sputtering
ESO/VL T/MGR/wrkshpt 1/B. 1
VL T 8M-COATING UNIT
PUMPING
CONSUMABLES (preliminary)
• Electrical power SPUTTERING EVAPORATION - Foreline pumps 65 1 25 kW
idle (low p) 45 90 kW - Diffusion pumps 1 00 - Bath-Cryo pumps 0
• Cooling Water - DIF System
- CRYO System
• LN 2 / 8 hour batch
125
5
100 kW o kW
130 I/min
10 I/min
- Pumps/Baffles 600 600 - Meissner Trap 1500
• LHe / 8 hour batch - CRYO 40(7) (JltsJ. c~srgi'lI1~ ~oJ
'Wrcluded. )
·2000
40(7) I
ESOIVL T/MGRlwrkshpt1/8.2
VL T 8M-COATING UNIT
PURCHASE
MANAGEMENT PLAN
• Requirements 8m Coating Unit (loading concept, film requ., film quality, [coating technology], power requ., pumping system, precleaning)
• Engineering FEA • Design Substr. Carrier
• Manufacturing • Process Developmnt • EU Perform. test
FEA Vac Vessel
• Transport on site • Weight load tests, witness tests • Acceptance test with mirror
• Development alternative films
ESO/VL T/MGR/wrkshpt 119.1
VL T 8M-COATING UNIT
QUALITY ASSURANCE
PLANNINGS
• Activities prior to production - starting clean zone - 1 test run with witness plates
• Quality Control during production - film thickness check (witness) - adhesion tape test (at the edge) - reflectance measurement (in situ) - monitoring selected parameters of sequences for washing and coating
- final visual observation (dark field ilumination)
• Maintenance plan - weight load tests - cleaning coating equipment
ESO/VL T/MGR/wrkshpt 1/10. 1
Discussions on Topics for Future Observatories
Mirror Handling for Re-coating S. Prat
Coating and Coating K. Raybould Equipment
Cleaning Mirrors in situ P. Giordano the Telescopes
Mirror Handling for Re-coating
Presentation by S. Prat
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1. GENERAL PREPARATION
* Position telescope
"lock tube
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* Bring carriage under M1
duration manpower
2H 3
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* Disconnect all lines to M1 unit
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duration manpower
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duration manpower
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END OF FIRST DAY: TOTAL 11 H
I IN MAINTENANCE BUILDING I OPTION oFF' .. CELL CoATIItJ ~
5. PREPARATION OF M1 UNIT
.. Roll in carriage in the preparation
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.. Remove cover and store
duration manpower
1H 3
6. PREPARATION OF M1 MIRROR
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duration manpower
'3 H
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duration manpower
tH 3
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duration manpower
OFF- CELL
./
END OF SECOND DAY: HANDLING 6 H + WASHING + PREPARE FOR COATING
///////./////.///
I Ml COATING I
PREPARATION TIME
M1 ALONE M1 IN CEll
1. GENERAL PREPARATION
2. PREPARATION OF M1 UNIT
3. REMOVAL OF M1 UNIT
4. TRANSPORT OF M1 UNIT
5.
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TOTAl DAY 1
PREPARATION OF M1 UNIT
PREPARATION OF M1 MIRROR
CELL
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. PREPARATIONS FOR WASHING
AFTER WASHING
PREPARE FOR COATING
TOTAl DAY 2
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Coating and Coating Equipment
Questionnaire by K. Raybould
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4 .... .. . SECTION A-A
4.2m ALUMINISING TANK WiTH SPUTTERING TEST EQUIPMENT
APP II Figure 6
• ..
EVALUATION OF COATING UNIFORMITY PRODUCED BY SPUTTERING
S.P.Worswick and A.S.Monk ROO
A;pherical surfaced mirror with a radius of curvature of approximately 25')mm and a diameter of 150mm was used for this test. The mirror has a ,;entral hole, with a linear extent of one third the diameter of the mi~ror, which allowed the radial deposition of the sputtered coating as proposed for the 8m mirror.
Th,~ mirror surface was checked, in its uncoated state, using a scatter pl~te interferometer with a hel~um neon laser as the source of il~urnination. The resultant fringe pattern was photographed and anllysed using WISP software. The test was set up twice with the fr~nges running in two directions, at 90 degrees to each other, across th! mirror. The mirror surface is of good quality with localised surface de~iations at the lambda/8 level and RMS deviations of 0.04 lambda (s~e Figure 1).
Teits of two sputtered coatings were undertaken. The first set (tested 30~h May 1990) was on a coating which showed a band of reduced reflectivity at the overlap region where the sputtering source was switched on an~ off. Th·~ interferometer was set up with fringes running both perpendicular and parallel to this band to look for a dtep function or slope in the reflected wavefront which might be associated with'this feature. The uniformity of the fringes limit such an effect to the lambda/8 level and the RMS values from the measurements are again at the 0.04 lambda level (see Figure 2).
Th= second test was of the surface produced by the sputtering run made on the 11th September 1990 when the magnetron was powered off with a ra~p-down voltage. The area of reduced reflectivity was much smaller anj could only just be detected under close inspection. A similar set of fringes to the previous tests were produced, again looking for distortions in the reflected wave front arising from the overlap re1ion in the coating (see Figure 3). As with the previous test no noticeable localised fringe shifts are present and the measured RM3 values are still about 0.04 lambda.
t ____ 5-\b~7
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Figure 1: Tests of uncoated spherical mirror.
Figure 2: Tests of sputtered aluminium coating. Direction of overlap region marked with arrow.
Figure 3: Tests of sputtered aluminium coating with magnetron ramp-down. Direction of overlap region marked with arrow.
EVALUATION OF COATING UNIFORMITY PRODUCED BY SPUTTERING
S.P.worswick and A.S.Monk RGO
A 3pherical surfaced mirror with a radius of curvature of approximately 250mm and a diameter of 150mm was used for this test. The mirror has a ~entral hole, with a linear extent of one third the diameter of the mi~ror, which allowed the radial deposition of the sputtered coating as proposed for the 8m mirror.
Th,~ mirror surface was checked. in its uncoated state. using a scatter plate interferometer with a hel.ium neon laser as the source of illumination. The resultant fringe pattern was photographed and analysed using WISP software. The test was set up twice with the frLnges running in two directions, at 90 degrees to each other. across th,~ mirror. The mirror surface is of good quality with localised surface de,iations at the lambda/8 level and RMS deviations of 0.04 lambda (s~e Figure 1).
Te3ts of two sputtered coatings were undertaken. The first set (tested 30:h May 1990) was on a coating which showed a band of reduced reflectivity at the overlap region where the sputtering source was switched on an~ off. Th,~ interferometer was set up with fringes running both perpendicular anj parallel to this band to look for a step function or slope in the reflected wavefront which might be associated with'this feature. The uniformity of the fringes limit such an effect to the lambda/8 level ani the RMS values from the measurements are again at the 0.04 lambda le,el (see Figure 2).
Th~ second test was of the surface produced by the sputtering run made on the 11th September 1990 when the magnetron was powered off with a ra~p-down voltage. The area of reduced reflectivity was much smaller anj could only just be detected under close inspection. A similar set of fringes to the previous tests were produced, again looking for di3tortions in the reflected wave front arising from the overlap reJion in the coating (see Figure 3). As with the previous test no noticeable localised fringe shifts are present and the measured RMS values are still about 0.04 lambda.
91
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Figure 1: Tests of uncoated spherical mirror.
Figure 2: Tests of sputtered aluminium coating. Direction of overlap region marked with arrow.
Figure 3: Tests of sputtered aluminium coating with magnetron ramp-down. Direction of overlap region marked with arrow.
Cleaning Mirrors in situ the Telescopes
Presentation by P. Giordano
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In-situ cleanln~ for the VLT
1.1.1 SensltIyity
Past e.xpenence at La Silla shows that the average loss of reDecUvity is of the order of 10% per surlace and per year. For a three-mirrors telescope (e.g. Nasmyth) the total loss per year is estimated to be of the order of 20% (jt is assumed that because of its usual or1entation the secondary mirror Is less affected) i.e. 1.8% per month. Therefore the re.flectMty R.. N months after coaUng. should be
R = R<) 0.982N
where R<) Is the initial reflecUvity after coating. The loss of refiedMty Is equivalent to a reduction of the light collecting area of the telescope. The consequence on the effective cUameter of the telescope 15 shown in the table hereafter. under the assumpUon that dust contamtnaUon is the only conl:Iibutor to signal reduction.
Months after coaUn~ o 3 6 9 12 15 18 21 24 EffecUve D tame ter 8000 7790 7580 7370 7170 6980 6790 6610 6430
A loss of reflectivity of 2~~ after one year also means that even under good seeIng conditions (0.4 arc seconds) where optical quallty should be the limiting factor (and, where best scientific results are e.xpected). the dust contamination reduces the performance by the same amount as optJca.l quallty.
With a monthly cleaning procedure whJcb would compensate for 90% the loss of reflecUvtty due to dust contamtnatlon the evolution of the dfecUve diameter of the telescope would be as follows
Months after tQgUne Q 6 12 H~ 21 3Q 36 42 4a Loss of reDectMty
200b-2896-0) 0 10% 200k 28% 35% 10%- 35%-
12) 0 1% 2% 3% 4% 5% 6% 7% 8% EffecUve Diameter (1) 8000 7580 7170 6790 6430 7580- 7170- 6790- 6430-
(2) 8000 7960 7910 7870 7830 7790 7740 7700 7660
- LOss of reflectivity and effecUve dJameter with :'w1thout in-situ cleaning. recoaUng ls and Without in-sHu cleaning procedure. supposed to take place after 2 years. 0): without cleaning: (2): with cleaning.
The conclusion is that monthly cleaning whIch would compensate for 9()OA> the loss of reflectivity due to dust polluUon would allow to keep the sJgna] throughput above 92% of ~1~~ ',..t~...,l r-I',,,.-.+~,,,,..-"I (f...-r.("t... t"' ........... ~~ ....... ,-f, ".~,L. .-. r,.... .. _ .. _ ~ .. '- r _ _ ,. _~ ___ , , __ ""
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TMAfscan ... Ver 1.12 [ESO_SEN2.USN) 11:09:31 10-02-1991 Page 1
COMMENTS: REFERENCE MIRROR MT4: Exposed 89 hours to dust pollution
SOURCE INFORMATION: WaveLength = 670 nm Incident Angle 25.0 degrees
RMS ROUGHNESS BANDWIDTH LIMITS: (0.010, 1.000] 1/tm
MEASUREMENT SUMMARY: =============================~====~=;=============~==============
0.0 50.0 (%) # 0.0 180.0 REFL RMS TIME DATE
===========================~=====================================
1 1. 003E-04 4.887E-05 90.3 7.1 08:51:44 06-24-1991 2 6.335E-05 4.314E-05 91. 7 5.5 08:52:01 06-24-1991 3 1.13SE-04 5.239E-05 91.7 7.5 08:52:10 06-24-1991 4 5.983E-OS 4.97SE-05 91.7 S.4 08:S2:19 06-24-1991 S 1.135E-04 8.144E-OS 91.7 7.4 08:52:28 06-24-1991 6 1. 126E-04 6.736E-OS 91. 7 7.4 08:S2:S2 06-24-1991 7 7.390E-OS 3.874E-OS 91.7 6.0 08:S2:S9 06-24-1991 8 1. 328E-04 4.799E-OS 91. 7 8.3 08:S3:05 06-24-1991 9 4.090E-05 2.46SE-05 91. 7 4.4 08:53:13 06-24-1991
10 5.119E-OS 4'.138E-OS 91.7 5.0 08:53:20 06-24-1991 =================================================================
STATISTICAL SUMMARY: ============================================================================
MINIMUM MAXIMUM **** LINEAR **** AVERAGE STD DEV
** LOGARITHMIC * AVERAGE STD DE
=========================~========================;=========================
0.0, 0.0) 4.090E-OS 1.328E-04 8.619E-OS 3.198E-OS 8.043E-05 0.2
(SO.0,180.0) 2.465E-05 8.144E-05 4.957E-05 1.560E-05 4.739E-05 0.1
REFL{%) 90.3 91.7 91.6 0.4 91. 6 N/A ----------------------------------------------------------------------------RMS(Angstroms) 4.4 8.3 6.4 1.3 6.3 N/A ----------------------------------------------------------------------------I Measurements = 10
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