Stable Levitation in the Low Velocity Range with the Damper Coils in Electrodynamic Suspension System

Author(s):  
Ryotaro Betsunoh ◽  
Shunsuke Ohashi
1984 ◽  
Vol 108 ◽  
pp. 139-140
Author(s):  
N. V. Bystrova

The large velocity range of the HI clouds belonging to the Magellanic Stream, as found by Haynes (1979), makes it reasonable to search for some low LSR velocity neutral hydrogen possibly belonging to the Stream. This gas, if any, would be severely blended by the local galactic gas.


Author(s):  
Tomoki Ikoma ◽  
Koichi Masuda ◽  
Chang-Kyu Rheem ◽  
Yusuke Yoshimura ◽  
Hisaaki Maeda

This paper describes performance of a vertical axis type marine turbine with variable-pitch blades for marine current power utilization. A cyclic mechanism is applied to pitch control of turbine blades. In this paper, the experimental model is developed, which type is variable pitch control one. At the first, conditions of marine currents around Japanese islands is explained, the necessarily of development of marine turbines in low to middle current velocity range is shown. Effectiveness of pitch control of a vertical axis turbine is described from results of CFD calculations. In the calculations, as the basic model, which pitch angles are fixed, that of a past experimental study is applied. From these investigations, the vertical axis type water turbine with variable-pitch blades for model experiment in a channel is developed. Detail of the model developed is introduced. The model experiment is explained. In the experiment, performance of the self-starting and the number of rotations of the turbine is measured. From the results, effectiveness of the pitch control is shown. However, the characteristics are different between past quasi-statistical investigation with the single stream theory and the experimental results. From the experiments, it is confirmed that the turbine of the variable-pitch types can start by itself in very low velocity range in which conventional vertical axis turbines cannot start and also rotate even if the inertia moment is acted.


1987 ◽  
Vol 122 ◽  
pp. 215-216
Author(s):  
M. E. Dollery ◽  
M. J. Gaylard ◽  
R. J. Cohen

Eight of thirty-four previously unobserved IRAS sources were found to be relatively strong 1612 MHz OH emitters. Five of these emit at 1667 MHz. Of the eight half are high velocity range, population I type stars, the other half are low velocity range, population II type stars. The pump efficiencies are in the range 0.018 ≤ e ≤ 0.163.


2011 ◽  
Vol 308-310 ◽  
pp. 1420-1425 ◽  
Author(s):  
Guang Yan Huang ◽  
Shun Shan Feng ◽  
Guang Wu ◽  
Shun Ping Li

Based on the cavity expansion theory, an analysis model of normal penetration of slender nose projectile into armor targets was established, and the variation relation curve of penetration depth and initial velocity when initial velocity is below ballistic limit was obtained. By carrying out ballistic impact test using 85mm smoothbore gun, various projectile nose shapes and armor target thickness and their effect on damage were considered. The research results have indicated that the damage of target is mainly ductile reaming and the shape of crater is almost the same as the projectile nose embedded in the target. Within a relatively low velocity range, nose shape has a greater influence on penetration depth. In contrast, within a relatively high velocity range, the target thickness has a greater influence on penetration depth. It can provide theoretical basis for the design of projectile noses and analysis of anti-penetration performance of armor targets.


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