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標(biāo)題: Titlebook: Compendium of Practical Astronomy; Volume 1: Instrument Günter Dietmar Roth Book 19941st edition Springer-Verlag Berlin Heidelberg 1994 Ast [打印本頁]

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作者: 冒號    時間: 2025-3-21 22:49
Rekursions- und Iterationsverfahren,There were two principal factors which motivated the people of ancient times to concern themselves with the stars: the link of celestial objects with religious concepts, and the everyday need to determine the time.
作者: 斷言    時間: 2025-3-22 03:09
Modern Sundials,Modern sundials have become a favorite ornament in houses and gardens. Their design and construction are not difficult with some knowledge of spherical astronomy, and suggestions for improved constructions appear occasionally in the literature [10.1].
作者: Acupressure    時間: 2025-3-22 08:10

作者: Ascendancy    時間: 2025-3-22 12:03

作者: 性上癮    時間: 2025-3-22 12:59

作者: 性上癮    時間: 2025-3-22 19:20
https://doi.org/10.1007/978-981-16-8197-4 of being able to record the images of faint objects not within reach of the eye. Once developed, photographs also provide a permanent document which can be unbiasedly inspected and analyzed at any convenient time.
作者: 死貓他燒焦    時間: 2025-3-23 01:03

作者: 飛行員    時間: 2025-3-23 03:07
Spatiotemporal Modeling of Influenzana which occur on the celestial sphere. This is a field that today is often neglected, and yet it is still the foundation of many branches of astronomy for observations and research, even if this is not always clearly evident. Every observer is confronted with problems involving spherical astronomy
作者: 不能和解    時間: 2025-3-23 07:39

作者: Lasting    時間: 2025-3-23 11:27
Spatiotemporal Processes of Plant Phenologycording device, be it a conventional photographic plate, a sophisticated electronic detector, or merely the human eye. This may be achieved by enhancing the light-collecting area or by sharper imaging, with the aims of improved angular resolution in order to separate closely adjacent objects and hig
作者: 消散    時間: 2025-3-23 15:32

作者: 強(qiáng)有力    時間: 2025-3-23 19:14

作者: 公豬    時間: 2025-3-23 23:35

作者: 厚顏    時間: 2025-3-24 03:04

作者: 中國紀(jì)念碑    時間: 2025-3-24 08:24
https://doi.org/10.1007/978-3-662-46751-0ight but extends far into infrared and ultraviolet wavelengths. In 1887, Heinrich Hertz succeeded in generating and detecting electromagnetic waves in the radio range. It seemed reasonable to investigate whether or not the Sun emits such rays. In 1890, T.A. Edison in the United States and O. Lodge i
作者: 爭議的蘋果    時間: 2025-3-24 11:44

作者: 整潔漂亮    時間: 2025-3-24 17:13

作者: 天文臺    時間: 2025-3-24 22:06
Springer-Verlag Berlin Heidelberg 1994
作者: dermatomyositis    時間: 2025-3-24 23:50
https://doi.org/10.1007/978-3-031-01665-3 removal of this uncertainty has itself become a primary focus of astronomical research. As with many other mathematical methods, Gauss’s . was originally developed to meet the stringent requirements which arise in the processing of astronomical measurements, and thus serves as a compliment to the t
作者: chandel    時間: 2025-3-25 06:37

作者: 不自然    時間: 2025-3-25 08:16

作者: PUT    時間: 2025-3-25 13:29
aterial which may have a different meaning and/or application in English-speaking countries from that in Germany. When the first English edition of this work, Astronomy: A Handbook (translated by the late A. Beer), appeared in 1975, it contained 21 chapters. This new edition is over twice the length and conta978-3-642-45688-6
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作者: visual-cortex    時間: 2025-3-26 10:35

作者: inchoate    時間: 2025-3-26 13:20
ing reader. We feel that this is a unique publication in that it contains valuable material that cannot easily-if at all-be found elsewhere. We are grateful to the authors for reading through the English version of the text, and for responding promptly (for the most part) to our queries. Several aut
作者: nonplus    時間: 2025-3-26 17:26

作者: 使迷惑    時間: 2025-3-26 22:21
Randomly Prompted Speaker Verification,and other scientists. In this regard, instructors affiliated with public and private educational institutions and also amateur astronomers can participate in educating interested persons in this most fascinating of subjects. Astronomy is—particularly at the introductory level—arguably the most approachable of all the sciences.
作者: insincerity    時間: 2025-3-27 03:39

作者: 彈藥    時間: 2025-3-27 06:18
Astronomy Education and Instructional Aids,and other scientists. In this regard, instructors affiliated with public and private educational institutions and also amateur astronomers can participate in educating interested persons in this most fascinating of subjects. Astronomy is—particularly at the introductory level—arguably the most approachable of all the sciences.
作者: CYT    時間: 2025-3-27 12:45

作者: 訓(xùn)誡    時間: 2025-3-27 16:13

作者: genesis    時間: 2025-3-27 20:47

作者: JEER    時間: 2025-3-27 22:13
Spatiotemporal Processes of Plant Phenologye requirements simultaneously. Rather, an observing instrument is optimized for a specific purpose and is often named after a particular type of construction or observational mode (e.g., zenith telescope, transit circle, binoculars, rich-field telescope, coronograph, astrograph, or Schmidt camera).
作者: 無可爭辯    時間: 2025-3-28 05:47
https://doi.org/10.1007/978-3-662-46751-0ission from the Sun, and in 1901, E. Nordmann in France searched for solar short wave radiation, all with negative results. Thus, at the turn of the last century, it seemed conclusive that no radio rays from the Universe reached the Earth.
作者: 協(xié)定    時間: 2025-3-28 09:01

作者: gruelling    時間: 2025-3-28 11:09

作者: 變化    時間: 2025-3-28 16:00
Book 19941st edition. We feel that this is a unique publication in that it contains valuable material that cannot easily-if at all-be found elsewhere. We are grateful to the authors for reading through the English version of the text, and for responding promptly (for the most part) to our queries. Several authors have
作者: arrhythmic    時間: 2025-3-28 21:55
Introduction to Astronomical Literature and Nomenclature,s, and also all of time back to the origin of the Universe as deduced from stellar dating and cosmological theory. Apart from meteorites and the very nearest celestial bodies which can be reached directly by spacecraft, astronomical researchers are spatially separated from the objects of their study
作者: 芳香一點    時間: 2025-3-29 00:15
Fundamentals of Spherical Astronomy,na which occur on the celestial sphere. This is a field that today is often neglected, and yet it is still the foundation of many branches of astronomy for observations and research, even if this is not always clearly evident. Every observer is confronted with problems involving spherical astronomy
作者: 茁壯成長    時間: 2025-3-29 04:42

作者: 繞著哥哥問    時間: 2025-3-29 09:58
Optical Telescopes and Instrumentation,cording device, be it a conventional photographic plate, a sophisticated electronic detector, or merely the human eye. This may be achieved by enhancing the light-collecting area or by sharper imaging, with the aims of improved angular resolution in order to separate closely adjacent objects and hig
作者: buoyant    時間: 2025-3-29 11:25
Telescope Mountings, Drives, and Electrical Equipment,ounting. The telescope mounting is a complex structure of many parts and is far less easily comprehended than the optical path in the telescope; some parts are even more difficult for the amateur telescope maker to manufacture than a primary mirror. Thus, the major problem has always been the manufa
作者: CAND    時間: 2025-3-29 15:38

作者: 軟膏    時間: 2025-3-29 21:59

作者: Bumptious    時間: 2025-3-30 01:43
Principles of Photometry,incident radiation is described completely by its flux, its direction, its color (wavelength), its polarization, the time of arrival, and—in certain cases—also by the location of the receiver. Photometry involves the measurement of radiation summed over a more or less extended wavelength region. Dep
作者: 油氈    時間: 2025-3-30 06:19

作者: 有效    時間: 2025-3-30 11:30

作者: opportune    時間: 2025-3-30 12:33
Aufbau und Funktion der normalen Hauttet, sind die Anhangsgebilde der Haut (Haare, N?gel, Talg- und Schwei?drüsen). Die Subkutis ruht in der Tiefe den Faszien auf. Die Haut des erwachsenen Menschen ist durchschnittlich 2 m. gro? und wiegt 3, unter Einrechnung des Fettgewebes bis zu 20 kg. Ihre Dicke schwankt zwischen 1,5 und 4 mm, wovo




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