
doi: 10.2172/6194407
The properties of a system to control the figure of a large telescope primary mirror that is composed of many individual segments are studied. The geometry considered, employing hexagonal mirrors, allows a simple and economical control system. The system is shown to be reliable and effective in continuously maintaining the figure to the precision required for optical astronomy. 10 figures.
General Physics, Equipment 420200* -- Engineering-- Facilities, Equipment, & Techniques, Control Systems, Mirrors, Optical Equipment, Orientation, 42 Engineering, 71 Classical And Quantum Mechanics, 657005 -- Theoretical Physics-- Optics, Telescopes
General Physics, Equipment 420200* -- Engineering-- Facilities, Equipment, & Techniques, Control Systems, Mirrors, Optical Equipment, Orientation, 42 Engineering, 71 Classical And Quantum Mechanics, 657005 -- Theoretical Physics-- Optics, Telescopes
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 0 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
