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Titlebook: Observing Photons in Space; A Guide to Experimen Martin C. E. Huber,Anuschka Pauluhn,Alex Zehnder Book 2013Latest edition Springer Science+

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樓主: Addendum
41#
發(fā)表于 2025-3-28 16:05:58 | 只看該作者
The mid- and far-infrared range: radiation emission processes from interstellar dust and gas,lecules in the gaseous state. Together, these signatures provide unique diagnostic probes of the physical and chemical conditions of the cool and dusty Universe. This article summarizes the contribution of space-based observations in the thermal infrared to our understanding of the Universe. In part
42#
發(fā)表于 2025-3-28 20:18:51 | 只看該作者
43#
發(fā)表于 2025-3-29 01:31:34 | 只看該作者
Imaging through Compton scattering and pair creation, 0.3 MeV to ≈ 300 GeV. The principles of measurement of both kinds of telescopes are explained and an overview of early Compton and pair telescopes is given. The properties and capabilities of COMPTEL and EGRET aboard NASA’s . are described. These two instruments have performed the first-ever all-sk
44#
發(fā)表于 2025-3-29 04:52:53 | 只看該作者
45#
發(fā)表于 2025-3-29 09:30:49 | 只看該作者
Far-infrared imaging and spectroscopic instrumentation,genic instruments and telescopes introduced. We give an introduction to direct detection techniques for imaging and spectroscopy and review the current state of the art in instrumentation and detector technology. We discuss the history of space-borne infrared missions dedicated to photometric survey
46#
發(fā)表于 2025-3-29 13:20:47 | 只看該作者
47#
發(fā)表于 2025-3-29 16:30:46 | 只看該作者
High-accuracy positioning: astrometry, light. A theoretical expression for the limiting accuracy is derived under idealized conditions and generalized to take into account more realistic circumstances, such as additive noise and finite pixel size. Its application is discussed in relation to different space-astrometry techniques includin
48#
發(fā)表于 2025-3-29 20:58:40 | 只看該作者
Interferometric imaging from space,ular resolution. The van Cittert–Zernike theorem forms the theoretical foundation of interferometric measurements and for the reconstruction of images from interferometric data. The closure phase method and phase self-calibration techniques retain useful phase information even if the individual phas
49#
發(fā)表于 2025-3-30 02:28:45 | 只看該作者
50#
發(fā)表于 2025-3-30 07:36:47 | 只看該作者
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