mirror_align_random_horizontal

Telescope: LSTN-01

Description: Fluctuations of the mirror alignment angle with respect to nominal alignment in the horizontal component (in azimuth or y direction in dish coordinates). The three terms are added up as independent (i.e., by squares; therefore he square of the horizontal mirror alignment error is \(\sigma^2 = \sigma_0^2 + \sigma_c^2 + \sigma_s^2\)). The values here are usually derived from fits to the measured point spread functions, with the single mirror point-spread function adapted beforehand. Note that, since this affects the angles of the mirrors, the impact on the combined spot size is twice as large.

Model Version	Value
5.0.0	0.0019 deg, 28.0 deg, 0.0, 0.0
6.0.0	0.0019 deg, 28.0 deg, 0.0, 0.0