標(biāo)題: Titlebook: Handbook of X-ray and Gamma-ray Astrophysics; Cosimo Bambi,Andrea Santangelo Living reference work 20220th edition High Energy Astrophysi [打印本頁(yè)] 作者: magnify 時(shí)間: 2025-3-21 16:32
書(shū)目名稱Handbook of X-ray and Gamma-ray Astrophysics影響因子(影響力)
書(shū)目名稱Handbook of X-ray and Gamma-ray Astrophysics影響因子(影響力)學(xué)科排名
書(shū)目名稱Handbook of X-ray and Gamma-ray Astrophysics網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱Handbook of X-ray and Gamma-ray Astrophysics網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱Handbook of X-ray and Gamma-ray Astrophysics被引頻次
書(shū)目名稱Handbook of X-ray and Gamma-ray Astrophysics被引頻次學(xué)科排名
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書(shū)目名稱Handbook of X-ray and Gamma-ray Astrophysics年度引用學(xué)科排名
書(shū)目名稱Handbook of X-ray and Gamma-ray Astrophysics讀者反饋
書(shū)目名稱Handbook of X-ray and Gamma-ray Astrophysics讀者反饋學(xué)科排名
作者: Junction 時(shí)間: 2025-3-22 00:17
Michael J. Pivovaroff,Takashi Okajimaa number of more widely distributed genera such as . that have subcentres in Melanesia. These taxa may represent the genral flora prevalent in the Melanesian Arcs and the tropical parts of Australia and New Zealand in the Miocene and early Pliocene prior to the invasion of more competitive Oriental elements.作者: 腐敗 時(shí)間: 2025-3-22 02:12
Kristin K. Madsen,David Broadway,Desiree Della Monica Ferreiralusion) and for Fiji by . (1975). Also included are those species collected in the New Hebrides in 1971 by . that have been reliably identified. A number of small and insignificant species are excluded (mainly nolids and acontiine and hypenine noctuids) that have probably been overlooked by most collectors and are therefore under-recorded.作者: LAVA 時(shí)間: 2025-3-22 04:52
Hideyuki Mori,Peter Friedrichn technologies: Time-of-Flight, Structured-Light and Active Stereoscopy, and provide qualitative results for any user to understand the underlying technology within 3D camera, as well as practical guidance on how to get the most of them for a given application..作者: Trabeculoplasty 時(shí)間: 2025-3-22 11:58
Carolyn Atkinsmand response programs can stabilize the energy market by shifting the electricity demand to off-peak durations. This part of the book examines the motivations, issues, and challenges involved in multi-tenant data center demand response. Further, it summarizes the formulated problems and the possible solutions.作者: CLEAR 時(shí)間: 2025-3-22 16:20
Bianca Salmaso,Alberto Moretti,Jessica Gaskinmand response programs can stabilize the energy market by shifting the electricity demand to off-peak durations. This part of the book examines the motivations, issues, and challenges involved in multi-tenant data center demand response. Further, it summarizes the formulated problems and the possible solutions.作者: Incommensurate 時(shí)間: 2025-3-22 17:41
M. W. Bautz,A. D. Holland,D. H. Lumbyou can start publishing..Key to successfully publishing is the need to:.Although there are a number of different types of articles that you can publish for peer review, this chapter focuses on some of the more common ones, namely the publication of a:作者: Interferons 時(shí)間: 2025-3-22 23:43
Luciano Gottardi,Stephen Smithyou can start publishing..Key to successfully publishing is the need to:.Although there are a number of different types of articles that you can publish for peer review, this chapter focuses on some of the more common ones, namely the publication of a:作者: aplomb 時(shí)間: 2025-3-23 04:32 作者: 摻假 時(shí)間: 2025-3-23 08:03
Nicolas M. Barrière,Marcos Bavdaz,Maximilien J. Collon,Ivo Ferreira,David Girou,Boris Landgraf,Giuseuggesting alternation of land and marine facies until further episodes of uplift occurred in the Eocene. From then onwards land in the area was probably significant to substantial, as will be seen when the geology is discussed in more detail.作者: Throttle 時(shí)間: 2025-3-23 17:15
Silicon Pore Optics,such as Athena and ARCUS, operating in the 0.2–12 keV band, with angular resolution aiming for 5 arcsec. SPO has also shown to be a versatile technology that can be further developed for gamma-ray optics, medical applications, and material research.作者: 澄清 時(shí)間: 2025-3-23 21:07
Facilities for X-ray Optics Calibration,ies. These facilities are also regularly used to support the development of new types of optics for future missions. In this chapter, we describe currently available facilities and list some of the key missions that used them for calibration. Future facility developments needed to support the next-generation X-ray missions are also discussed.作者: FICE 時(shí)間: 2025-3-24 00:53
X-Ray Detectors for Astrophysics,escribe in this paper the basic physical processes on which the detection of photons is based and give an overview of the relevant detector classes and their actual use in space missions. It should also be noted that some of the detectors are used in other fields, including medicine and material science, but we will not address this.作者: Preserve 時(shí)間: 2025-3-24 05:55 作者: 刺耳 時(shí)間: 2025-3-24 09:59
J. W. den Herder,M. Feroci,N. Meidinger supply and demand sides of the multi-tenant data center (in terms of computation which is a function of energy consumption). The supply side comprises the grid, on-site renewables, storage (batteries), and backup generator, whereas the demand side comprises the sum of individual demands from tenants.作者: Accessible 時(shí)間: 2025-3-24 14:26
Norbert Meidinger,Johannes Müller-Seidlitzliar with. As such, I will be covering best practice approaches on method development, method validation, data analysis, how to achieve quality assurance and how to record information into laboratory books.作者: 地牢 時(shí)間: 2025-3-24 17:01
X-Ray Optics for Astrophysics: A Historical Review,follows the use of X-ray optics from the first rocket-borne instruments in the 1960s through to the observatories flying today and being developed for future use. It also includes a brief overview of the challenges of fabricating X-ray optics and the various technologies that have been used to date.作者: tinnitus 時(shí)間: 2025-3-24 20:49
Charge Coupled Devices,ance to the X-ray CCDs, including instrument considerations and examples, together with performance over time. While design considerations such as noise and QE are described, long-term operational problems arising from radiation damage and contamination are also considered.作者: 轉(zhuǎn)換 時(shí)間: 2025-3-25 00:57 作者: Formidable 時(shí)間: 2025-3-25 06:13
CMOS Active Pixel Sensors,s with specific applications in X-ray imaging and space-based X-ray astronomy. Some new developments in monolithic APS (MAPS) which make them competitive to the more established technologies are covered as well. The sensor developments for several planned and proposed X-ray space telescopes are described.作者: 提煉 時(shí)間: 2025-3-25 09:34
Living reference work 20220th edition last parts are dedicated to analysis techniques in X-ray and Gamma-ray astronomy: spectral analysis, imagining analysis, timing analysis, and polarimetric analysis. Presenting the state of the art in X-ray and gamma-ray astronomy, this is both a valuable book for students and an important reference resource for researchers in the field..作者: 清楚說(shuō)話 時(shí)間: 2025-3-25 12:53 作者: 數(shù)量 時(shí)間: 2025-3-25 18:44
Single-Layer and Multilayer Coatings for Astronomical X-Ray Mirrors,easuring techniques in use for characterizing thin film coatings. Important aspects of stability are presented, and we provide a thorough review on the issue stress, which will play an essential role in next-generation high angular resolution imaging telescope.作者: myelography 時(shí)間: 2025-3-25 23:22
Collimators for X-Ray Astronomical Optics,sion from a spatially extended source or a faint point source. The improvement of the angular resolution and the effective area is intensively pursued for the next-generation X-ray optics. In parallel, it is a vital issue to reduce the stray light as low as possible to fully achieve the expected performance of these future X-ray optics.作者: exostosis 時(shí)間: 2025-3-26 03:22 作者: 散布 時(shí)間: 2025-3-26 07:10 作者: CAGE 時(shí)間: 2025-3-26 12:09 作者: Firefly 時(shí)間: 2025-3-26 14:03
Michael J. Pivovaroff,Takashi Okajima 1963; ., 1965). Elements of this vegetation include a majority of the Melanesian Arc and austral genera mentioned in the previous chapter as well as a number of more widely distributed genera such as . that have subcentres in Melanesia. These taxa may represent the genral flora prevalent in the Mel作者: 構(gòu)成 時(shí)間: 2025-3-26 17:06 作者: Osteoarthritis 時(shí)間: 2025-3-26 22:32
Nicolas M. Barrière,Marcos Bavdaz,Maximilien J. Collon,Ivo Ferreira,David Girou,Boris Landgraf,Giuseks in the sequence (. & ., 1970). The first emergence of land in the area was probably in the Upper Jurassic, an event possibly associated with the Rangitata Orogeny of New Zealand. The sedimentary sequence in some areas is broken then, with some evidence of metamorphism, and does not resume until t作者: 微塵 時(shí)間: 2025-3-27 03:31
Richard Willingalee specifications of the main 3D cameras available in the mass market. The authors present a deep metrological analysis of the main camera based on the three main technologies: Time-of-Flight, Structured-Light and Active Stereoscopy, and provide qualitative results for any user to understand the unde作者: Debark 時(shí)間: 2025-3-27 06:30 作者: 微生物 時(shí)間: 2025-3-27 09:56 作者: 規(guī)章 時(shí)間: 2025-3-27 17:39 作者: 盤旋 時(shí)間: 2025-3-27 18:44
Bianca Salmaso,Alberto Moretti,Jessica Gaskin is critical in preserving the electrical infrastructure (i.e., the grid) in emergency situations, such as extreme weather events. Further economic demand response programs can stabilize the energy market by shifting the electricity demand to off-peak durations. This part of the book examines the mo作者: 許可 時(shí)間: 2025-3-27 23:08
J. W. den Herder,M. Feroci,N. Meidingerllen behind that of owner-operated data centers due to the use of an uncoordinated model. Coordinated power management is proposed as a solution to improve the efficiency of multi-tenant data centers. To achieve coordinated power management, the operators must address the dynamic natures of both the作者: 痛苦一生 時(shí)間: 2025-3-28 03:36 作者: 領(lǐng)先 時(shí)間: 2025-3-28 09:12 作者: Oscillate 時(shí)間: 2025-3-28 13:47 作者: 標(biāo)準(zhǔn) 時(shí)間: 2025-3-28 16:09 作者: Ceramic 時(shí)間: 2025-3-28 21:13 作者: Tracheotomy 時(shí)間: 2025-3-28 23:17 作者: 占卜者 時(shí)間: 2025-3-29 06:43 作者: Neuropeptides 時(shí)間: 2025-3-29 07:40 作者: 刪減 時(shí)間: 2025-3-29 13:44
X-Ray Optics for Astrophysics: A Historical Review,reduction in background and a consequent very large improvement in sensitivity. The X-ray optics also permit use of small-format, high-performance focal-plane detectors and, of course, especially for high-angular-resolution optics, provide a wealth of imaging data from extended sources. This review 作者: laparoscopy 時(shí)間: 2025-3-29 19:04
Geometries for Grazing Incidence Mirrors, Wolter I geometry and derivatives from this optical prescription have been the design used by most X-ray telescopes flown on satellite missions. In this chapter, we will review the motivations for the broad adoption of the Wolter I design and study in detail the equations that govern the optical pr作者: avulsion 時(shí)間: 2025-3-29 19:52
Lobster Eye X-ray Optics,ing incidence (reflective) X-ray imaging systems used in astronomy and other applications are based on the Wolter 1 (or modified) arrangement. But there are also other designs and configurations proposed for future applications for both laboratory and space environments. Kirkpatrick-Baez (K-B)-based作者: HARP 時(shí)間: 2025-3-30 00:07 作者: exercise 時(shí)間: 2025-3-30 05:41 作者: definition 時(shí)間: 2025-3-30 11:59 作者: Gratulate 時(shí)間: 2025-3-30 13:43 作者: 消瘦 時(shí)間: 2025-3-30 19:56
Collimators for X-Ray Astronomical Optics,otect the mirror from severe in-orbit thermal environment or to limit the mirror’s field of view. Although the latter may be a disadvantage in the viewpoint of observational performance, the collimation of incident X-rays allows us to block X-rays with large off-axis angles. Thus, the mount of the X作者: 間接 時(shí)間: 2025-3-31 00:20
Technologies for Advanced X-Ray Mirror Fabrication,or to enable accurate and efficient X-ray reflection. The performance of an X-ray mirror, and ultimately that of the telescope, is linked to the processes and technologies used to create it. The goal of this chapter is to provide the reader with an overview of the different technologies and processe作者: neutralize 時(shí)間: 2025-3-31 01:45 作者: SLAY 時(shí)間: 2025-3-31 05:45
Facilities for X-ray Optics Calibration,d. This calibration requires a specialized facility that can approximate an astronomical point source and accommodate the mirrors and other telescope components, including an appropriate detector system. The X-ray source and telescope are typically housed in a vacuum chamber to permit easy propagati作者: 叢林 時(shí)間: 2025-3-31 11:14
X-Ray Detectors for Astrophysics,from focusing mirrors characterized by their effective area and angular resolution to a simple collimated system where photons from a small solid angle on the sky are selected. An overview of these optical systems is given in Section 1 of this handbook (.). In this section, we give an introduction t作者: 厭惡 時(shí)間: 2025-3-31 14:27
Proportional Counters and Microchannel Plates, workhorse for almost four decades. Although the principle of such a detector seems to be rather simple, over time, it underwent considerable performance improvements, and the lifetime under orbital conditions was extended tremendously. Particularly the invention of position-sensitive proportional c作者: 不能強(qiáng)迫我 時(shí)間: 2025-3-31 20:19
Charge Coupled Devices,es, and in the case of the “great observatories” of XMM-Newton and Chandra have been returning science data for over 20?years. The CCD optimized for X-ray detection is often different from its variant working in the visible light region. This chapter describes the key performance parameters of relev作者: 飲料 時(shí)間: 2025-4-1 00:05 作者: Euthyroid 時(shí)間: 2025-4-1 04:51 作者: Vulvodynia 時(shí)間: 2025-4-1 09:36
DEPFET Active Pixel Sensors,ck silicon sensor is fully depleted by the principle of sideward depletion. They have furthermore in common to be back-illuminated detectors, which allows for ultrathin and homogeneous photon entrance windows. This enables relatively high quantum efficiencies at low energies and close to 100% for ph作者: esoteric 時(shí)間: 2025-4-1 12:59 作者: 字的誤用 時(shí)間: 2025-4-1 17:46 作者: strdulate 時(shí)間: 2025-4-1 21:52 作者: 信任 時(shí)間: 2025-4-2 00:38 作者: 宇宙你 時(shí)間: 2025-4-2 04:44
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