WHT mirror reflectivity

The V-band reflectivities of the WHT primary, secondary and Nasmyth (tertiary) mirrors are measured at regular intervals with a hand-held reflectometer.

Primary mirror

The dates of cleaning and measured reflectivities are stored here: Reflectivity_results_page

The primary mirror was aluminised each autumn (after the summer dust storms) up to 1998, and was cleaned with CO2 snow every couple of months, humidity permitting, during 1997-9. There was no aluminising during 1999. It appears that each CO2 cleaning only partially restores reflectivity, and by June 2000 it was only 81%. The mirror was then experimentally washed with detergent and warm water, which raised reflectivity to 85%, and then aluminised, raising reflectivity to 88%. ING plans to wash the mirror in situ every few months, but this hasn't yet (May 2002) been possible. The aim of reducing intervals between aluminising is to reduce the number of nights lost, and manpower costs, and lessen the risk of damage (during craning) to ING's most irreplaceable component.

The UV reflectivity cannot be measured with the reflectometer, and experience at other telescopes suggests that it might not be fully restored by snow-cleaning. The UV reflectivity is now being monitored via observations of standard stars. The UV/V reflectivity ratio (measured more accurately than the absolute values) was within a few % of the expected values when measured in Jan and Jul 1999, and in Feb 2000, suggesting that snow cleaning is as effective in the UV as at V band.

The primary mirror suffered its most serious accident yet on 1999 May 6, when a 1.5-kg component of the top-end focus drive fell vertically onto the bare mirror. The surface now bears a few deep scratches, which were ground out prior to the Jun 2000 aluminising to avoid spreading of any cracks. The area affected is negligibly small.

Secondary mirror

The secondary mirror is less exposed to the elements than is the primary, and is aluminised every few years. It was experimentally washed in Oct 2000. Log of reflectivity measurements:
881126         aluminised
950620   0.88  using light-box + photometer
951120         aluminised
000524   0.87
001025   0.78
001025   0.87  after water washing
001031   0.88  after aluminising
020326   0.88 

Nasmyth flat

The Nasmyth flat is also well protected (particularly when stowed to allow light to reach the Cassegrain focus). Before ~ 1997, it was cleaned about once per year with PL25 spray-on/peel-off film, but is now CO2-cleaned about once every 2 months. We plan soon to replace the Al coating with Ag. Log of reflectivity measurements:
901212         aluminised
960325         aluminised
000524   0.75
000525   0.84  after water washing
000918   0.83
001129         aluminised
001130   0.89  
001221   0.89
010130   0.90
010403   0.89 
010404   0.88  after CO2-snow cleaning
010605   0.87
010718   0.87
010905   0.87
011105   0.79
011204   0.81
020107   0.80  before CO2-snow cleaning 
020107   0.85  after CO2-snow cleaning 
020326   0.87  before CO2-snow cleaning 
020326   0.85  after CO2-snow cleaning 
020416   0.83
020531   0.85  before CO2-snow cleaning 
020531   0.83  after CO2-snow cleaning 
020708   0.84  before
020712   0.88  after
020816   0.82  before
020816   0.87  after

Other WHT mirrors

INGRID feed flat (Ag coated, in cass A&G):
0001           re-silvered (good for 2 years?)
0011?    0.79                                          
0012?    0.92  after cleaning
001121   0.89  after cleaning, but looks bad, needs recoating

Chris Benn (crb@ing.iac.es)

2002 Jun 3