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Titlebook: Radio, Submillimeter, and X-Ray Telescopes; N. G. Basov Book 1976 Springer Science+Business Media New York 1976 X-ray.astronomy.developmen

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书目名称Radio, Submillimeter, and X-Ray Telescopes
编辑N. G. Basov
视频video
丛书名称The Lebedev Physics Institute Series
图书封面Titlebook: Radio, Submillimeter, and X-Ray Telescopes;  N. G. Basov Book 1976 Springer Science+Business Media New York 1976 X-ray.astronomy.developmen
描述This volume contains the results of research and development connected with the creation oftelescopes intended for the new regions of the spectrum mastered by astronomy: the x-ray, submillimeter (far infrared), and radio regions. The creation of x-ray, submillimeter, and radio telescopes and the receiver apparatus connected with them is a complicated and, in many respects, unusual problem. Therefore, the experience accumulated at the Institute of Physics can prove useful to specialists working in this field, This volume is intended for scientists, engineers, and builders occupied in research and development in the fields of x-ray, submillimeter, and radio astronomy as well as for students of advanced courses in these specialties, V CONTENTS A Reflecting X-Ray Telescope for an Orbital Astrophysical Station. • • • • • • • • • 1 I. L, Beigman. L. A. Vainshtein, Yu. P. Voinov, D. A. Goganov, N. I. Komyak, S. L. Mandel‘shtam, I. P, Tindo, N, A, Shatskii, and A. I. Shurygin Mirror Systems for X-Ray Telescopes. • • • • • • • • • • • • • • • • • • • • • • • • • • • • 13 I. L. Beigman, L, A. Vainshtein, Yu. P. Voinov, and V. P, Shevel‘ko Extra-Atmospheric studies in the Submillimeter Range
出版日期Book 1976
关键词X-ray; astronomy; development; fields; physics; radio astronomy; telescope
版次1
doihttps://doi.org/10.1007/978-1-4899-2660-9
isbn_softcover978-1-4899-2662-3
isbn_ebook978-1-4899-2660-9
copyrightSpringer Science+Business Media New York 1976
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Limiting Dimensions of a Fully Steerable Parabolic Mirror for a Radio Telescope,g power and sensitivity. In addition to the corresponding demands on the radio receiving apparatus and the allowance for the wavelength range used, the above-mentioned demands on radio telescopes are connected with an increase in their dimensions. The question of the maximum possible size for the fu
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