標(biāo)題: Titlebook: Astromineralogy; Thomas Henning Book 2010Latest edition Springer-Verlag Berlin Heidelberg 2010 Accretion.Casini cosmic dust analyser.Spitz [打印本頁] 作者: JADE 時間: 2025-3-21 16:42
書目名稱Astromineralogy影響因子(影響力)
書目名稱Astromineralogy影響因子(影響力)學(xué)科排名
書目名稱Astromineralogy網(wǎng)絡(luò)公開度
書目名稱Astromineralogy網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Astromineralogy被引頻次
書目名稱Astromineralogy被引頻次學(xué)科排名
書目名稱Astromineralogy年度引用
書目名稱Astromineralogy年度引用學(xué)科排名
書目名稱Astromineralogy讀者反饋
書目名稱Astromineralogy讀者反饋學(xué)科排名
作者: MODE 時間: 2025-3-21 23:39
Sandra Krause-Steger,Melanie Roskioptical data of astronomically relevant materials can be measured and how such data can be applied to interpret astronomical spectra. The identification of minerals in space from infrared spectroscopy will be summarized.作者: buoyant 時間: 2025-3-22 04:14
Thomas HenningComprehensive and coherent account of astromineralogy..Largely extended 2nd edition..Explains complicated life cycle of cosmic dust..Shows synergies from astronomical observations and laboratory astro作者: 種族被根除 時間: 2025-3-22 05:34
Lecture Notes in Physicshttp://image.papertrans.cn/b/image/163579.jpg作者: Narcissist 時間: 2025-3-22 09:09
https://doi.org/10.1007/978-3-642-13259-9Accretion; Casini cosmic dust analyser; Spitzer infrared space telescope; astrochemistry; astromineralog作者: 大溝 時間: 2025-3-22 14:56
978-3-642-13258-2Springer-Verlag Berlin Heidelberg 2010作者: arrhythmic 時間: 2025-3-22 18:23 作者: Accede 時間: 2025-3-23 00:56
https://doi.org/10.1007/978-3-642-58558-6cs. The main topics are calculation of solid-gas chemical equilibria, the basic concepts for calculating dust growth under non-equilibrium conditions, dust processing by annealing and solid diffusion, a discussion of non-equilibrium dust formation in stellar winds, and in particular a discussion of 作者: 保守黨 時間: 2025-3-23 02:38 作者: 輕快來事 時間: 2025-3-23 09:03 作者: 前兆 時間: 2025-3-23 12:32
https://doi.org/10.1007/978-3-642-17054-6er conditions that are not reproducible on Earth. Already relatively simple in-situ measurements provide information about the properties of dust particles. Measurements of interplanetary dust have shown for the first time the fluffy and porous structure of interplanetary dust as well as the existen作者: BUOY 時間: 2025-3-23 14:41
Forschung erfolgreich vermarktenbeyond the giant planets, presolar grains or “astrominerals” with solar and non-solar isotopic compositions are expected to be even more abundant in cometary IDPs than in primitive meteorites. Non-solar D/H and .N/.N isotopic enrichments in chondritic IDPs are associated with a carbonaceous carrier.作者: nonchalance 時間: 2025-3-23 20:27 作者: judicial 時間: 2025-3-23 22:17
Sandra Krause-Steger,Melanie Roskioptical data of astronomically relevant materials can be measured and how such data can be applied to interpret astronomical spectra. The identification of minerals in space from infrared spectroscopy will be summarized.作者: 偶像 時間: 2025-3-24 03:53 作者: grudging 時間: 2025-3-24 09:12
Book 2010Latest edition progress in ground-based observations and laboratory astrophysics form the basis for this updated and widely extended second edition.Beyond addressing the specialist in the field, the book is intended as a high-level but readable introduction to astromineralogy for both the nonspecialist researcher and the advanced student.作者: facetious 時間: 2025-3-24 14:18 作者: gonioscopy 時間: 2025-3-24 17:43 作者: Texture 時間: 2025-3-24 22:54
Formation and Evolution of Minerals in Accretion Disks and Stellar Outflows,the composition and evolution of the mineral mixture in protoplanetary accretion discs. An overview is given over the data on dust growth, annealing, and on solid diffusion for astrophysically relevant materials available so far from laboratory experiments.作者: critic 時間: 2025-3-25 02:37 作者: Intractable 時間: 2025-3-25 05:15
https://doi.org/10.1007/978-3-642-58558-6the composition and evolution of the mineral mixture in protoplanetary accretion discs. An overview is given over the data on dust growth, annealing, and on solid diffusion for astrophysically relevant materials available so far from laboratory experiments.作者: 不持續(xù)就爆 時間: 2025-3-25 09:28 作者: Predigest 時間: 2025-3-25 12:30
,From Dust Astrophysics Towards Dust Mineralogy – A Historical Review,cted at 217?nm in the interstellar extinction curves was commonly assigned to graphite grains. Beginning in 1968, observations of the vibrational bands of the SiO. group in circumstellar as well as in interstellar dust provided ample evidence for the ubiquitous occurrence of silicate grains in the G作者: 思考才皺眉 時間: 2025-3-25 16:50
The Mineralogy of Cometary Dust,arts of the solar nebula where temperatures remained low enough so that interstellar grains could have survived. The small glassy silicates in comets may indeed be interstellar grains. The CAI and the widespread, abundant crystalline silicates must have condensed in the hot inner solar nebula; their作者: 吸氣 時間: 2025-3-25 23:39
The In-Situ Study of Solid Particles in the Solar System,directly measured yet, their conditions of entry into the solar system reveal the forces that are acting on them. The forces depend on the properties of dust and allow for a comparison to astrophysical models of dust size, composition and structure. In-situ measurements with improved dust detectors 作者: 葡萄糖 時間: 2025-3-26 00:14 作者: aspersion 時間: 2025-3-26 06:07
The Most Primitive Material in Meteorites,to ~200?ppm..Isotope abundance anomalies are the key feature based on which the presolar nature of a given grain is ascertained. They also allow identifying likely stellar sources for the grains. The major source of SiC, the oxide and the silicate grains are Red Giant/AGB stars, while some (~1%) of 作者: ALIAS 時間: 2025-3-26 09:36 作者: Guileless 時間: 2025-3-26 13:50
https://doi.org/10.1007/978-3-642-17054-6arts of the solar nebula where temperatures remained low enough so that interstellar grains could have survived. The small glassy silicates in comets may indeed be interstellar grains. The CAI and the widespread, abundant crystalline silicates must have condensed in the hot inner solar nebula; their作者: 消音器 時間: 2025-3-26 18:38
https://doi.org/10.1007/978-3-642-17054-6directly measured yet, their conditions of entry into the solar system reveal the forces that are acting on them. The forces depend on the properties of dust and allow for a comparison to astrophysical models of dust size, composition and structure. In-situ measurements with improved dust detectors 作者: 誘騙 時間: 2025-3-27 00:06 作者: SOW 時間: 2025-3-27 04:55
Die Forschung selbst nachhaltig gestaltento ~200?ppm..Isotope abundance anomalies are the key feature based on which the presolar nature of a given grain is ascertained. They also allow identifying likely stellar sources for the grains. The major source of SiC, the oxide and the silicate grains are Red Giant/AGB stars, while some (~1%) of 作者: 結(jié)構(gòu) 時間: 2025-3-27 08:15 作者: prosperity 時間: 2025-3-27 13:15 作者: Cleave 時間: 2025-3-27 16:43 作者: ETHER 時間: 2025-3-27 20:17
The Mineralogy of Interstellar and Circumstellar Dust in Galaxies,environment in which it is found. Dust can therefore be used as a tracer and probe of the physical and chemical conditions where it is detected. We present an observational overview of interstellar and circumstellar dust using spectroscopy at infrared wavelengths. Thanks to the contributions made by作者: 空氣 時間: 2025-3-27 22:04
The Mineralogy of Cometary Dust, other minerals. While forsterite Mg.SiO. and enstatite MgSiO. are the most common silicate minerals, both the olivine and pyroxenes also show a wide range in Mg/Fe in at least some comets. Carbon in the dust is enriched relative to CI chondrites; a significant fraction of the carbon is in the form 作者: 高興一回 時間: 2025-3-28 04:19 作者: cacophony 時間: 2025-3-28 06:59
The Astromineralogy of Interplanetary Dust Particles,beyond the giant planets, presolar grains or “astrominerals” with solar and non-solar isotopic compositions are expected to be even more abundant in cometary IDPs than in primitive meteorites. Non-solar D/H and .N/.N isotopic enrichments in chondritic IDPs are associated with a carbonaceous carrier.作者: Prosaic 時間: 2025-3-28 12:35
The Most Primitive Material in Meteorites,er phases of isotopically anomalous noble gases and isolated from the bulk meteorites using harsh chemical treatments. Diamond was the first and may occur with an abundance ￣1‰, but it is not clear what fraction of the observed nanometer-sized diamonds is truly presolar. Others found by this approac作者: troponins 時間: 2025-3-28 14:48 作者: Indelible 時間: 2025-3-28 19:49
nd politics in our own communities? From Machiavelli to the fake news phenomenon, this book provides a compelling introduction to the politics behind one of the world’s most enduring pop culture figures..978-3-030-42869-3978-3-030-05776-3作者: 補(bǔ)角 時間: 2025-3-29 01:07
