Figure: 30-m usage statistics for 1994.
Fig. 2 shows how the 30m telescope was used during the year 1994. This is not the scheduled time but how the telescope was actually used. For example, if an observation could not be carried out because of high wind (the major cause for loss of telescope time), the time lost is attributed to the segment ``Stop Wind''. Please note that the telescope status is recorded every 2 hours which means that e.g. technical problems of shorter duration may not be included in the statistics.