A photometric night is defined here as one with over 6 continuos hours of cloudless sky.
A spectroscopic night as one with at most 3/8 cloud cover for 6 or more continuous hours.
These graphs have been calculated from data averaged over a period of 24 years (1965 - 1989, excluding 1968). Tabla 1 lists the number of hours per night available throughout the year.
Please note that these statistics are representative of the definitions as stated above and DO NOT reflect the number of hours in which the telescope were used.
Diurnal temperature variations are normally 50 to 68 degrees fahrenheit and during the nighttime hours the variations are about 6 to 11 degrees fahrenheit throughout the year. For infrared observing the winter months are the best. The amount of precipitable water in the atmosphere is comparable then to that of the better known IR observing sites.
Maximum Hrs. Average Hrs. Average Hrs.
Month Possible Photometric Observational **
January 8.5 6.7 7.7
February 9.5 7.9 8.9
March 10.5 8.1 9.2
April 11.5 7.4 9.5
May 12.1 5.2 8.1
June 12.4 5.0 8.3
July 12.3 5.2 7.4
August 11.8 5.7 8.0
September 10.9 5.7 7.6
October 9.9 5.5 7.2
November 8.9 6.0 7.2
December 8.2 6.6 7.3
* Determined from statistics from 1965 to 1989.** Observational is spectroscopic plus photometric hours. See definitions in section on Quality of Nights.