Titlebook: Reflecting Telescope Optics I; Basic Design Theory Raymond N. Wilson Textbook 2004Latest edition Springer-Verlag Berlin Heidelberg 2004 Ga

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套索

978-3-662-30863-9Springer-Verlag Berlin Heidelberg 2004

偏見

Reflecting Telescope Optics I978-3-540-76581-3Series ISSN 0941-7834 Series E-ISSN 2196-9698

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Textbook 2004Latest editionr and format corrections on 17 pages, a number of corrections or additions of substance could be incorporated. These included minor corrections to Figs. 1. 3 b) and 2. 8 and to the text of Fig. 5. 18. The most important change of all was probably the complete revision of the historical treatment of

ALTER

Major telescopes from Lord Rosse to about 1980,were able, in spite of the limitation of secondary spectrum, to compete with or even excel reflectors with apertures up to 1.22 m (Herschel) was a measure of the two great weaknesses of the reflectors of the time: the poor efficiency through low reflectivity and the problems of mechanical manipulation in such sizes.

Obloquy

Historical introduction,ny excellent accounts exist as chapters in more general works, in biographies or accounts of specific projects, but only a few books are devoted solely to the historical development. The works of King (1955) [1.1] and Riekher (1957, 1990) [1.2] are notable. The recent second edition of Riekher has b

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Field correctors and focal reducers or extenders,the field aberrations of the mirror system. If the mirror system does not correct the axial image at the focus in question (e.g. the prime focus of an RC telescope), the field corrector will also be required to achieve this. Normally, field correctors are substantially afocal, i.e. they only have a