scholarly journals Some Problems on Materials Tests in High Temperature Hydrogen Base Gas Mixture

1980 ◽  
Vol 66 (3) ◽  
pp. 418-424 ◽  
Author(s):  
Tatsuo SHIKAMA ◽  
Tatsuhiko TANABE ◽  
Masakazu FUJITSUKA ◽  
Heitaro YOSHIDA ◽  
Ryoji WATANABE
Author(s):  
Tatsuo Shikama ◽  
Tatsuhiko Tanabe ◽  
Yoshikazu Sakai ◽  
Masakazu Fujitsuka ◽  
Heitaro Yoshida ◽  
...  

AIChE Journal ◽  
2011 ◽  
Vol 58 (1) ◽  
pp. 312-321 ◽  
Author(s):  
Kwangkook Jeong ◽  
Shivaji Sircar ◽  
Hugo S. Caram

2018 ◽  
Vol 8 (11) ◽  
pp. 2841-2852 ◽  
Author(s):  
Galina Sádovská ◽  
Edyta Tabor ◽  
Milan Bernauer ◽  
Petr Sazama ◽  
Vlastimil Fíla ◽  
...  

The δ and θ Al2O3 phases well stabilized Fe(iii) in Td or Oh coordination, which were identified as the active species in high temperature decomposition of N2O in a complex gas mixture produced by oxidation of ammonia.


Author(s):  
Lee Frederickson ◽  
Kyle Kitzmiller ◽  
Fletcher Miller

High temperature central receivers are on the forefront of concentrating solar power research. Current receivers use liquid cooling and power steam cycles, but new receivers are being designed to power gas turbine engines within a power cycle while operating at a high efficiency. To address this, a lab-scale Small Particle Heat Exchange Receiver (SPHER), a high temperature solar receiver, was built and is currently undergoing testing at the San Diego State University’s (SDSU) Combustion and Solar Energy Laboratory. The final goal is to design, build, and test a full-scale SPHER that can absorb 5 MWth and eventually be used within a Brayton cycle. The SPHER utilizes air mixed with carbon particles generated in the Carbon Particle Generator (CPG) as an absorption medium for the concentrated solar flux. Natural gas and nitrogen are sent to the CPG where the natural gas undergoes pyrolysis to carbon particles and nitrogen is used as the carrier gas. The resulting particle-gas mixture flows out of the vessel and is met with dilution air, which flows to the SPHER. The lab-scale SPHER is an insulated steel vessel with a spherical cap quartz window. For simulating on-sun testing, a solar flux is produced by a solar simulator, which consists of a 15kWe xenon arc lamp, situated vertically, and an ellipsoidal reflector to obtain a focus at the plane of the receiver window. The solar simulator has been shown to produce an output of about 3.25 kWth within a 10 cm diameter aperture. Inside of the SPHER, the carbon particles in the inlet particle-gas mixture absorb radiation from the solar flux. The carbon particles heat the air and eventually oxidize to carbon dioxide, resulting in a clear outlet fluid stream. Since testing was initiated, there have been several changes to the system as we have learned more about the operation. A new extinction tube was designed and built to obtain more accurate mass loading data. Piping and insulation for the CPG and SPHER were improved based on observations between testing periods. The window flange and seal have been redesigned to incorporate window film cooling. These improvements have been made in order to achieve the lab scale SPHER design objective gas outlet flow of 650°C at 5 bar.


1980 ◽  
Vol 11 (9) ◽  
pp. 1589-1598 ◽  
Author(s):  
Tatsuo Shikama ◽  
Tatsuhiko Tanabe ◽  
Masakazu Fujitsuka ◽  
Masahiro Kitajima ◽  
Heitaro Yoshida ◽  
...  

2006 ◽  
Vol 26 (4) ◽  
pp. 347-359 ◽  
Author(s):  
Yongxia Sun ◽  
A. G. Chmielewski ◽  
S. Bułka ◽  
Z. Zimek

1994 ◽  
Vol 343 ◽  
Author(s):  
Noboru Yoshikawa ◽  
Atsushi Kikuchi

ABSTRACTA gas mixture consisting of TiCl4, H2 and N2 was fed into an externally-heated steel tube, and TiN was deposited on the inner wall by CVD. Microstuctures of the films were observed and their relationships with the preferred crystal orientations were studied. Distributions of the film growth rate and gas concentrations along the axial direction were calculated.By comparing the film microstructures with the calculated local deposition conditions, it is shown that formation of the films with (110) preferred orientation correlated with the conditions at high temperature and low partial pressure of TiCl4 on the substrate.


2017 ◽  
Vol 6 ◽  
pp. 35-41
Author(s):  
Volodymyr Blintsov ◽  
Sergiy Hrynchak

The ways of improving the design of ship openings with the implementation of a method for reducing the intensity of the exit of flue gases through an opening (doors, hatches) of the emergency premise of the ship are considered. The output of flue gases from the emergency premise is proposed to be controlled by the control of gas–air currents with the help of a system of jet water–gas ejectors. Ejectors are equipped with devices for collecting flue gases from the emergency premise of the ship and the collectors of the output of the vapor–gas mixture back to the emergency premise. In case of fire, in the shortest possible time, a high temperature rises in the area of exit from the emergency premise of the ship and a large amount of smoke spreads along the corridors and premises of the ship. These factors require immediate sealing of the emergency premise, which limits the operational access of emergency teams to combat fire. The considered air suppression methods in the ship's aperture and devices for their implementation contribute to screening of heat energy and localization of flue gases in the emergency premise without its sealing to ensure prompt access of emergency teams.


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