標(biāo)題: Titlebook: Experiments on Cosmic Dust Analogues; Proceedings of the S Ezio Bussoletti,Carlo Fusco,Giuseppe Longo Conference proceedings 1988 Kluwer Ac [打印本頁(yè)] 作者: Buren 時(shí)間: 2025-3-21 17:01
書(shū)目名稱Experiments on Cosmic Dust Analogues影響因子(影響力)
書(shū)目名稱Experiments on Cosmic Dust Analogues影響因子(影響力)學(xué)科排名
書(shū)目名稱Experiments on Cosmic Dust Analogues網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱Experiments on Cosmic Dust Analogues網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱Experiments on Cosmic Dust Analogues被引頻次
書(shū)目名稱Experiments on Cosmic Dust Analogues被引頻次學(xué)科排名
書(shū)目名稱Experiments on Cosmic Dust Analogues年度引用
書(shū)目名稱Experiments on Cosmic Dust Analogues年度引用學(xué)科排名
書(shū)目名稱Experiments on Cosmic Dust Analogues讀者反饋
書(shū)目名稱Experiments on Cosmic Dust Analogues讀者反饋學(xué)科排名
作者: 嚴(yán)厲批評(píng) 時(shí)間: 2025-3-21 23:48 作者: 機(jī)械 時(shí)間: 2025-3-22 03:32 作者: 搖擺 時(shí)間: 2025-3-22 07:17
978-94-010-7863-4Kluwer Academic Publishers 1988作者: faucet 時(shí)間: 2025-3-22 12:34
Experiments on Cosmic Dust Analogues978-94-009-3033-9Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: 分發(fā) 時(shí)間: 2025-3-22 15:42
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/e/image/319116.jpg作者: 分發(fā) 時(shí)間: 2025-3-22 19:01 作者: 鋼筆尖 時(shí)間: 2025-3-22 22:54
,Mary Butts and England’s Nature,oduced new impulses to simulation and modelling of the nucleus and its behaviour in the solar radiation field. Since 1969 several attempts of laboratory simulation had been made, first by Russian groups in Leningrad and Dushanbe (Kajmakov and Sharkov, 1972; Dobrovolsky and Kajmakov, 1977; Dobrovolsk作者: 值得尊敬 時(shí)間: 2025-3-23 02:14
Clean Energy Production Technologiesmeasurements such as scattering, extinction and emission with models ultimately derived from some sort of laboratory data. In this long-standing effort, there are two distinctly different approaches which I would like to outline in the beginning by reference to figure 1. First there is the approach 作者: doxazosin 時(shí)間: 2025-3-23 06:55 作者: SPALL 時(shí)間: 2025-3-23 12:28 作者: CRAB 時(shí)間: 2025-3-23 14:27
Nanoparticles in Biomedical Applications,essential for the optical properties of the medium because they can condense and make solids or large molecules which have optical wide bands whereas atom ions or small molecules (H, H., He, H....) only have narrow lines and cannot give a continuous absorption in a large range of wavelengths.作者: Microgram 時(shí)間: 2025-3-23 21:22
Shilpi Srivastava,Atul Bhargavaorphous material, takes place by itself due to the combined action of temperature and time and thus does not present experimental problems. Because of its spontaneous decay, the amorphous state is metastable and the conversion to the crystalline phase at a given temperature may take seconds or billi作者: COLIC 時(shí)間: 2025-3-24 00:22 作者: 遭遇 時(shí)間: 2025-3-24 06:25 作者: 慢跑鞋 時(shí)間: 2025-3-24 09:09
Conference proceedings 1988ons are mostly lacking. It appeared then very tempting to gather together experimentalists, ob- servers and theoreticians working in the field of cosmic dust and in related areas. The Workshop held in Capri (Italy) from September 8th till 12th 1987 gave the participants a unique opportunity for exch作者: 袋鼠 時(shí)間: 2025-3-24 14:43
Semra Unal,Oguzhan Gunduz,Muhammet Uzun a limited facet of experiments on grain analogs and does not generally treat the different technique in great depth. The references take care of this deficiency. In the silicate working group, particular aspects could be considered more critically and in greater detail.作者: 我說(shuō)不重要 時(shí)間: 2025-3-24 18:33 作者: Defraud 時(shí)間: 2025-3-24 21:52
Ali Haider,Muhammad Ikram,Asma Rafiqsome major questions remain still controversial. According Mathis (1986a) it is crucial to note that the words “interstellar dust” refer to different materials as soon as we consider different space regions as the diffuse ISM, the outer edges of dense clouds, the dark central regions of these clouds.作者: dictator 時(shí)間: 2025-3-25 00:28
Shilpi Srivastava,Atul Bhargavaons of years depending on the activation energy involved. For the silicates which are of interest here, the transition takes place within a reasonable amount of time at temperature in the order of 500 to 1000°C.作者: Misgiving 時(shí)間: 2025-3-25 05:13
Solid Carbon in Spacesome major questions remain still controversial. According Mathis (1986a) it is crucial to note that the words “interstellar dust” refer to different materials as soon as we consider different space regions as the diffuse ISM, the outer edges of dense clouds, the dark central regions of these clouds.作者: 死亡 時(shí)間: 2025-3-25 10:50 作者: output 時(shí)間: 2025-3-25 12:26
0067-0057 ce conditions are mostly lacking. It appeared then very tempting to gather together experimentalists, ob- servers and theoreticians working in the field of cosmic dust and in related areas. The Workshop held in Capri (Italy) from September 8th till 12th 1987 gave the participants a unique opportunit作者: 憎惡 時(shí)間: 2025-3-25 16:39
0067-0057 h will be of some help for future works. In addition to the scientific efforts, the Capodimonte Observatory and the Istituto Universitario Navale sought to give978-94-010-7863-4978-94-009-3033-9Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: membrane 時(shí)間: 2025-3-25 20:43 作者: 撕裂皮肉 時(shí)間: 2025-3-26 00:55
,Mary Butts and England’s Nature,mpeding an effective scaling up to the true cometary conditions. Furthermore, the lack of detailed analytical methods such as spectrometry or chromatography did not allow a detection of chemical changes induced by irradiation. Anyhow, destruction of ice samples by micro-explosions or larger outburst作者: 入伍儀式 時(shí)間: 2025-3-26 04:34 作者: 極為憤怒 時(shí)間: 2025-3-26 09:46 作者: Recessive 時(shí)間: 2025-3-26 12:46
Green Nanotechnology for Biofuel Productionstream of water vapor, from a reservoir of throughly degassed triple-distilled water, was directed at the plate, through a capillary tubing with a diffuser on its tip. An ice layer, consisting of 10. – 10. water molecules was deposited on the plate during ～ 45 min. A stream of gas (Ar, CO, N., CH., 作者: 賭博 時(shí)間: 2025-3-26 20:02
Conference proceedings 1988technical problems about these items were discussed in great detail. Though no definite answers were given, useful indications come out which will be of some help for future works. In addition to the scientific efforts, the Capodimonte Observatory and the Istituto Universitario Navale sought to give作者: 點(diǎn)燃 時(shí)間: 2025-3-26 21:52
Comet Nucleus Sample Return Missionave been accomplished in NASA and ESA, the objective of which was to conduct an assessment of candidate mission concepts and to define key design, operations and technology requirements. These studies have by now provided a technical baseline to sufficient extent to generate performance, schedule pl作者: textile 時(shí)間: 2025-3-27 01:40
Initial Comet Simulation Experiments at DFVLRmpeding an effective scaling up to the true cometary conditions. Furthermore, the lack of detailed analytical methods such as spectrometry or chromatography did not allow a detection of chemical changes induced by irradiation. Anyhow, destruction of ice samples by micro-explosions or larger outburst作者: PET-scan 時(shí)間: 2025-3-27 07:00 作者: 悅耳 時(shí)間: 2025-3-27 12:29
Ion Bombardment: Techniques, Materials and Applicationscules, electrons or photons (from visible to X wavelengths). The purpose of this paper is to review some work made in our laboratory in the last 5 years (with a quotation to the results obtained in other laboratories), by describing irradiated materials, used techniques and astrophysical application作者: CAMP 時(shí)間: 2025-3-27 13:59
The Structure and Dynamics of Amorphous Water Ice and Trapping of Gases in Itstream of water vapor, from a reservoir of throughly degassed triple-distilled water, was directed at the plate, through a capillary tubing with a diffuser on its tip. An ice layer, consisting of 10. – 10. water molecules was deposited on the plate during ～ 45 min. A stream of gas (Ar, CO, N., CH., 作者: Androgen 時(shí)間: 2025-3-27 18:54 作者: 圓柱 時(shí)間: 2025-3-28 01:23
Initial Comet Simulation Experiments at DFVLRoduced new impulses to simulation and modelling of the nucleus and its behaviour in the solar radiation field. Since 1969 several attempts of laboratory simulation had been made, first by Russian groups in Leningrad and Dushanbe (Kajmakov and Sharkov, 1972; Dobrovolsky and Kajmakov, 1977; Dobrovolsk作者: 朋黨派系 時(shí)間: 2025-3-28 03:49 作者: 相反放置 時(shí)間: 2025-3-28 10:09
Experiments on the Formation, Properties and Processing of Cosmic Dustc dust. An earlier, similar report (Donn, 1985) included material covered at this meeting in sessions on ices and on carbon type matter. The attempt was to include all relevant processes for silicates not contained in the reviews of optical phenomena and grain irradiation. Many of the phenomena disc作者: 吹氣 時(shí)間: 2025-3-28 11:22
Solid Carbon in Spaceant role in the gas phase composition of molecular clouds. In addition, metallic components are important because they carry the charge inside dense clouds regulating the ion-molecule chemistry in these regions. Despite these facts and active research which is presently lasting since over 50 years, 作者: 有效 時(shí)間: 2025-3-28 15:21 作者: 令人苦惱 時(shí)間: 2025-3-28 19:46
Laboratory Production of Amorphous Silicatesorphous material, takes place by itself due to the combined action of temperature and time and thus does not present experimental problems. Because of its spontaneous decay, the amorphous state is metastable and the conversion to the crystalline phase at a given temperature may take seconds or billi作者: 外形 時(shí)間: 2025-3-28 23:18 作者: 刺穿 時(shí)間: 2025-3-29 07:09 作者: interpose 時(shí)間: 2025-3-29 11:04
https://doi.org/10.1007/978-3-642-67335-1Chemie; anorganische Chemie; organische Chemie
