DOLT
发表于 2025-3-25 05:59:49
Book 1999lutionized not only manufacturing and test procedures but also the whole area of quality specification with the introduction of active control into the functioning telescope. Other subjects covered here are alignment of telescope optics, atmospheric optics, including adaptive optics, reflecting coat
overwrought
发表于 2025-3-25 09:19:05
0941-7834 escope optics in the comprehensive manner of Vol. II.IncludeThis volume is concerned essentially with the modern developments in reflecting telescope optics. In the last twenty years, modern technology has revolutionized not only manufacturing and test procedures but also the whole area of quality s
Collision
发表于 2025-3-25 12:40:05
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平躺
发表于 2025-3-25 17:13:02
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发酵剂
发表于 2025-3-25 20:11:45
Book 1999ings and ancillary equipment (adapters and baffles). Although an independent work, Vol. II is heavily cross-referenced with Vol. I. It is richly illustrated and gives, together with Vol. I, the most complete list of references available; it can also therefore be regarded as a source book.
懒鬼才会衰弱
发表于 2025-3-26 03:09:49
Manufacture and test procedures, I am particularly grateful for the generous information given during visits to the workshops of REOSC in Paris, Carl Zeiss in Oberkochen and Horst Kaufmann in Crailsheim. The former are two of the world’s major producers of large astronomical optics, the latter an example of an excellent small work
Collision
发表于 2025-3-26 06:33:32
Sensitivities, alignment of telescopes and test procedures in function,rrors fall into two classes: decentering errors and axial despace errors. It is useful to recall here the relevant results from RTO I, bearing in mind that the notation is identical and is defined in Appendix A therein.
Trypsin
发表于 2025-3-26 12:12:17
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痛恨
发表于 2025-3-26 15:22:24
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Parameter
发表于 2025-3-26 18:47:01
Atmospheric optics, adaptive optics, telescope quality for interferometry,ur of large air masses has only become significant for telescope optics in the last 35 years. It is therefore logical and inevitable that the subject of telescope optics has reached a stage where the mechanical, opto-mechanical and optical production problems (see Table 3.11) are largely solved, whe