The QSO Team records weather conditions every night of the year. Our logs indicate that:
The graph below shows that there can be significant variations from
year to year.
Taking into account the average time lost to weather and time used by overheads (e.g. slewing the telescope and initiating the guiding), the effective average number of hours per night for each instrument is:
The following plot compares the Image Quality (seeing) as measured by
MegaCam
in the r and the u band with the seeing measured by the Mauna Kea
Atmospheric Monitor (MKAM) located on a tower between the CFHT and
Gemini osbervatories. MegaCam measurements were corrected for the
airmass and wavelength. The wavelength corrected applied follows a
lambda^0.6 relationship. The seeing is generally well below 1 arcsec but
does vary over time.
In the plot below, the u band data has been offset by 0.25", which
represents the offset measured with MegaCam between the r and the u
bands. The r band and u band data now overlap.