نتایج جستجو برای: gaseous phase
تعداد نتایج: 610777 فیلتر نتایج به سال:
Gaseous beryllium metaborate, Be(B02)2,has been identified mass spectrometrically in the vapor above the beryllium-boron-oxygen system. A st-jdy of this system by differential thermal analysis» and Knudsen effusion using a vacuum balance and mass spectrometer, showt-i solid DeoBo0, to be the only condensed mixed oxide phase present with a melting point of 1495 ± 5C. The following thermodynamic ...
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جریانهای آشفته گاز همراه با ذرات جامد در بسیاری از فرآیندهای صنعتی و زیست محیطی نظیر صنایع معدنی، شیمیایی، تبدیل انرژی و کنترل آلودگی هوا کاربرد دارد. در این پایان نامه برای پیش بینی خواص جریان آشفته گاز-جامد رو به بالا در یک لوله عمودی با شار ثابت و یک لوله افقی، مدلی سه بعدی به روش چهارطرفه اویلرین-لاگرانژین ارائه شده است. فاز گاز با معادلات متوسط زمانی رینولدز مومنتوم و انرژی و الگوی جریان آ...
At this article we will study the Effect of Particle Radius on the Co-Flow Premixed Flame of Organic Particle Cloud. This analytical research frame work is thermal-diffusion model with assumption that the lewis number is unit. The structure of the flame is presumed to consist of three zone: a preheat vaporization zone where the rate of the gas-phase chemical reaction is small, a reaction zone ...
Our former study reported that Fe-Sn spinel (Fe3-xSnxO4) was easily formed when SnO2 and Fe3O4 were roasted under CO-CO2 atmosphere at 900-1100 °C. However, the formation procedure is still unclear and there is a lack of theoretical research on the formation mechanism of the Fe-Sn spinel. In this work, the reaction mechanisms between SnO2 and Fe3O4 under CO-CO2 atmosphere were determined using ...
The present study is a critical assessment of thermochemical data for gaseous ruthenium oxides based on available experimental data. A full analysis and reinterpretation are presented with proposition new accurate standard formation enthalpies values: Δf H°298(RuO4, g) = −197.6 ± 5.5 kJ mol−1, H°298(RuO3, −53.0 10 H°298(RuO2, 158 20 mol−1 H°298(RuO, 301 28 mol−1.
In this paper we present some test results of our newly developed Multi-Phase Chemo-Dynamical Smoothed Particle Hydrodynamics (MP-CD-SPH) code for galaxy evolution. At first, we present a test of the “pure” hydro SPH part of the code. Then we describe and test the multi-phase description of the gaseous components of the interstellar matter. In this second part we also compare our condensation a...
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