Reflectometry and BRDF data with Iris:
This corresponds to a 1.1% reflectivity loss per month at 530nm (average over 5 months), about twice higher than usual.
Regular washing in September improved reflectivity by 8.5% in average. Reflectometry and BRDF data with Iris (before/after wash respectively):
These numbers are actually close (some are even slightly higher!) than what is quoted in the litterature for a new coating. In October, rain leaked through the dome shutter and contaminated M1 (lots of long ugly white stripes across the mirror): in the bad areas (about 20% of the mirror), about 6% loss was measured but it was well recovered with washing in November (only about 1.8% less compared to previous wash). The reflectivity and BRDF improved to:
Mirror washed on the 21st, see the plots of reflectivity and scattering [1] (the numbers after the last aluminizing are also plotted for reference). All data with the Minolta.
See the plots of reflectivity [2] and scattering [3] for that period (data with the Minolta).
Reflectivity decreases in average by 2.5% per year and scatter increases by 2.0% per year. There seems to be a seasonal trend as the slopes are much higher in 'summer' (October to April) when the site humidity is higher (32-55%), which makes the dust stick more easily onto the glass: summer slope for R and SC is about 0.63% per month, whereas it is only about 0.05% per month in 'winter' (May to September, RH is 12-32%).
Numerical data: in parenthesis (last column) is the number of points sampled on the mirror for each result. Each point on the mirror is sampled 3 times (averaged by the reflectometer). On some dates (like 10Jan98), we also indicate the variations (+/-) in the data. For the first row, replace "before/after CO2 cleaning" by "before/after Al". The case "before Al" means the mirror was CO2 dusted and measured just before realuminizing.
DATE |
% Reflectivity before CO2 cleaning |
% Reflectivity after CO2 cleaning |
% Scattering before CO2 cleaning |
% Scattering after CO2 cleaning |
Elapsed time (weeks) between new Al and CO2 |
||||
400nm | 700nm | 400nm | 700nm | 400nm | 700nm | 400nm | 700nm | ||
2-Sep-98 +/- |
87.42 0.47 |
84.22 0.13 |
93.46 0.74 |
89.11 0.50 |
4.49 0.71 |
4.40 0.39 |
1.47 1.41 |
0.77 0.71 |
new aluminium (3) |
10-Sep-98 | 95.16 | 90.1 | 94.53 | 89.75 | 0.61 | 0.43 | 0.49 | 0.35 | 1 (1) |
14-Oct-98 | 94.1 | 88.89 | 95.23 | 90.05 | 1.06 | 0.80 | 0.63 | 0.54 | 6 (2) |
13-Nov-98 | no data | 10 (0) | |||||||
11-Dec-98 | 91.59 | 87.23 | 93.58 | 89.08 | 1.95 | 1.61 | 1.51 | 1.18 | 14 (4) |
10-Jan-99 +/- |
91.62 1.78 |
86.91 0.83 |
93.69 0.9 |
88.76 0.78 |
1.77 0.01 |
1.98 0.04 |
1.41 0.16 |
1.32 0.22 |
18 (4) |
19-Feb-99 | 91.18 | 86.46 | 92.24 | 87.58 | 3.34 | 3.34 | 3.12 | 2.55 | 23 (3) |
19-Mar-99 | 92.34 | 87.46 | 92.59 | 88.06 | 2.61 | 2.56 | 2.69 | 2.11 | 27 (3) |
17-Apr-99 | 92.27 | 87.55 | 92.63 | 87.93 | 2.94 | 2.45 | 2.91 | 2.24 | 31 (3) |
16-May-99 | 92.18 | 87.64 | 92.43 | 87.89 | 2.75 | 2.38 | 2.69 | 2.18 | 35 (3) |
13-Jun-99 | 92.58 | 87.87 | 92.75 | 88.12 | 2.54 | 2.25 | 2.44 | 2.02 | 39 (3) |
10-Jul-99 | 91.59 | 87.7 | 91.61 | 87.91 | 2.75 | 2.39 | 2.66 | 2.16 | 43 (3) |
8-Aug-99 | 91.44 | 87.61 | 91.78 | 87.91 | 2.57 | 2.3 | 2.38 | 2.01 | 47 (3) |
4-Sept-99 | 91.45 | 87.21 | 92.35 | 87.84 | 2.81 | 2.42 | 2.55 | 2.09 | 51 (3) |
3-Oct-99 | 91.31 | 86.96 | 91.56 | 87.06 | 3.21 | 2.61 | 3.09 | 2.55 | 55 (3) |
30-Oct-99 | 90.96 | 86.87 | 91.19 | 87.3 | 3.24 | 2.80 | 3.25 | 2.45 | 59 (3) |
29-Nov-99 | 91.08 | 86.7 | 3.64 | 3.28 | 63(3) no cleaning | ||||
23-Dec-99 | 90.52 | 86.39 | 91.84 | 87.42 | 4.04 | 3.48 | 3.62 | 2.75 | 67 (3) |
22-Jan-00 | 71 no data taken | ||||||||
6-Feb-00 | 87.88 | 84.63 | 88.98 | 85.63 | 5.57 | 4.86 | 5.14 | 4.05 | 73 (3) |
17-Mar-00 | 87.34 | 87.34 | 88.1 | 85.18 | 5.55 | 5.03 | 5.35 | 4.25 | 78 (3) |
21-Mar-00 | 88.3 | 84.69 | 92.66 | 89.03 | 5.62 | 4.68 | 2.20 | 1.09 | 78(3) WASH |
See the efficiency plots of the CO2 cleaning: reflectivity [4] and scattererometry [5]. Average gain per cleaning session is R+0.70% and SC-0.30% in the visible.
Aluminizing, see the plot [6] of reflectivity and scattering before and after aluminizing (last one was in Apr 97).
Aluminized together on August 26, 1999. Measurements with the Minolta.
See the f/13.5 [7] mirror reflectometry and scatterometry.
See the f/7.5 [8] mirror reflectometry and scatterometry.
Last update: 18 April 01
Links
[1] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/60_wash_mar00.gif
[2] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/60_r.gif
[3] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/60_sc.gif
[4] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/60co2gainr.gif
[5] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/60co2gainsc.gif
[6] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/60_bef_al_sep98.gif
[7] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/60_f135.gif
[8] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/60_f75.gif
[9] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/1.5%20Followup_Nov2009.pdf