scholarly journals Determination of the practical accuracy of the operation of the safety friction clutch with a variable gain installed in the forging equipment ensuring the absence of breakdowns

2019 ◽  
Vol 680 ◽  
pp. 012012
Author(s):  
K O Kobzev ◽  
E S Bozhko ◽  
A V Mozgovoi ◽  
A G Iliev ◽  
A A Kovaleva
Keyword(s):  
Variable Gain ◽  
Friction Clutch ◽  
Practical Accuracy

ASSESSMENT OF PURITY OF SWITCHING OFF AND INCREASE IN RELIABILITY OF WORK OF THE MASTER CLUTCH WITH THE FRICTION DISKS WORKING IN OIL

2020 ◽  
pp. 49-56
Author(s):  
Yu. I. Krykhtin ◽  
V. I. Karlov ◽  
S. E. Chervoncev
Keyword(s):  
Internal Friction ◽  
Technical Design ◽  
Tracked Vehicle ◽  
Automatic Installation ◽  
Transmission Oil ◽  
Friction Clutch ◽  
Technical Solutions ◽  
Moving Layer

Methodology of determination of moment of conduct is worked out are leashes, at the shutdown of master clutch with the disks of friction, working in transmission oil, tracked vehicle by mass a 17,5 t, taking into account tensions of internal friction in moving layer of oil. Solutions are proposed on reduction of partial transmission of moment from a leading disk to slave, for example, use of technical design with automatic installation of spacing between all disks of friction at switching off of main friction clutch The developed technical solutions increase reliability of work of the clutch with the friction disks working in oil and also can be used for new projects and modernizations of the existing designs.

Determination of the Source of an Electrical Overstress Event to a Digital Variable Gain Amplifier Module

2014 ◽  
Author(s):  
Thiri Htun ◽  
Steve Brockett
Keyword(s):  
Mechanical Damage ◽  
Variable Gain Amplifier ◽  
Variable Gain ◽  
Root Cause ◽  
Physical Evidence ◽  
Electrical Stress ◽  
Destructive Analysis ◽  
Electrical Overstress ◽  
Non Destructive

Abstract This paper presents a systematic approach of failure analysis to determine the source of electrical overstress condition to a digital variable gain amplifier (DVGA) module where the failure was due to attenuation accuracy. Having consideration of the physical evidence on the failed devices and the root cause of the failure gives an insight of how the mechanical damage caused an electrical overstress exposure to the devices. The paper provides information on destructive analysis and non-destructive analysis conducted for determining the root cause of the failure of the DVGA module. Analysis revealed that devices failed due to an electrical overstress exposure through mechanical damage to the passivation of the metal-2 lines. The mechanical damage occurred during die-sort testing due to misalignment of the probes which delivered unintended electrical stress to the devices.

Determination of Suitable MRF-Region for Practical Prediction of Engine Cooling Fan Performance

2011 ◽  
Author(s):  
Yuji Kobayashi ◽  
Itsuhei Kohri ◽  
Yukio Matsushima
Keyword(s):  
Predictive Accuracy ◽  
Boundary Surface ◽  
Cooling Systems ◽  
Automotive Engine ◽  
Fan Performance ◽  
Multiple Parameters ◽  
Engine Cooling ◽  
Cooling Fan ◽  
Practical Accuracy

Recently, CFD technology has become popular to the prediction of the engine cooling performance for the design of the automotive engine cooling systems. Particularly, the practical prediction of the cooling fan performance is one of the important issues. In the design phase of the vehicle development, combinations of multiple parameters are generally examined. Certainly, the unsteady calculations such as LES or LBM, which require high resolution of the space, give good accuracy meanwhile they spend much time for their executions so that they are not always practical. Therefore, the steady RANS coupling with MRF method is indispensable. However, it has been pointed out that, in case of complicated layout around the fan of an actual vehicle, the size of the MRF-region dominates predictive accuracy while the symmetry of the flow structure is taken account. Then, in this study, attracting on the discontinuity at the boundary surface of the MRF-region, authors found the method to determine adequate MRF-region to predict the fan performance in practical accuracy. This paper deals with the outline of the method and their applications.

Galactic orbits of stars

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley
Keyword(s):  
Globular Cluster ◽  
Potential Field ◽  
High Velocity ◽  
Velocity Vector ◽  
Variable Stars ◽  
The Sun ◽  
Proper Motions ◽  
Rr Lyrae ◽  
The Galaxy

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.

Distance to SN 1987A and the LMC

1999 ◽  
Vol 190 ◽  
pp. 549-554
Author(s):  
Nino Panagia
Keyword(s):  
Angular Size ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Light Curves ◽  
Distance Modulus ◽  
Absolute Size ◽  
Sn 1987A

Using the new reductions of the IUE light curves by Sonneborn et al. (1997) and an extensive set of HST images of SN 1987A we have repeated and improved Panagia et al. (1991) analysis to obtain a better determination of the distance to the supernova. In this way we have derived an absolute size of the ringRabs= (6.23 ± 0.08) x 1017cm and an angular sizeR″ = 808 ± 17 mas, which give a distance to the supernovad(SN1987A) = 51.4 ± 1.2 kpc and a distance modulusm–M(SN1987A) = 18.55 ± 0.05. Allowing for a displacement of SN 1987A position relative to the LMC center, the distance to the barycenter of the Large Magellanic Cloud is also estimated to bed(LMC) = 52.0±1.3 kpc, which corresponds to a distance modulus ofm–M(LMC) = 18.58±0.05.

International determination of the total motion of the pole

1961 ◽  
Vol 13 ◽  
pp. 29-41
Author(s):  
Wm. Markowitz
Keyword(s):  
Secular Motion ◽  
The Future

A symposium on the future of the International Latitude Service (I. L. S.) is to be held in Helsinki in July 1960. My report for the symposium consists of two parts. Part I, denoded (Mk I) was published [1] earlier in 1960 under the title “Latitude and Longitude, and the Secular Motion of the Pole”. Part II is the present paper, denoded (Mk II).

Time and Latitude in South Africa

1972 ◽  
Vol 1 ◽  
pp. 27-38
Author(s):  
J. Hers
Keyword(s):  
South Africa ◽  
Cape Town ◽  
Astronomical Observations ◽  
Royal Observatory ◽  
The Republic ◽  
Astronomical Determination ◽  
Limited Accuracy ◽  
Better Than

In South Africa the modern outlook towards time may be said to have started in 1948. Both the two major observatories, The Royal Observatory in Cape Town and the Union Observatory (now known as the Republic Observatory) in Johannesburg had, of course, been involved in the astronomical determination of time almost from their inception, and the Johannesburg Observatory has been responsible for the official time of South Africa since 1908. However the pendulum clocks then in use could not be relied on to provide an accuracy better than about 1/10 second, which was of the same order as that of the astronomical observations. It is doubtful if much use was made of even this limited accuracy outside the two observatories, and although there may – occasionally have been a demand for more accurate time, it was certainly not voiced.

Large-scale Motion of Solar Filaments

2000 ◽  
Vol 179 ◽  
pp. 205-208
Author(s):  
Pavel Ambrož ◽  
Alfred Schroll
Keyword(s):  
Magnetic Flux ◽  
Proper Motion ◽  
Time Scale ◽  
Large Scale ◽  
Accuracy Of Measurements ◽  
Solar Filaments ◽  
General Movement ◽  
Scale Motion ◽  
Velocity Scatter

AbstractPrecise measurements of heliographic position of solar filaments were used for determination of the proper motion of solar filaments on the time-scale of days. The filaments have a tendency to make a shaking or waving of the external structure and to make a general movement of whole filament body, coinciding with the transport of the magnetic flux in the photosphere. The velocity scatter of individual measured points is about one order higher than the accuracy of measurements.

Practical Realization of a Reference System for Earth Dynamics by Satellite Methods

1975 ◽  
Vol 26 ◽  
pp. 341-380 ◽  
Author(s):  
R. J. Anderle ◽  
M. C. Tanenbaum
Keyword(s):  
Reference Frame ◽  
Polar Motion ◽  
Pole Position ◽  
Control Points ◽  
Significant Information ◽  
Crustal Motion ◽  
Average Reference ◽  
Future Data ◽  
Existing Data

AbstractObservations of artificial earth satellites provide a means of establishing an.origin, orientation, scale and control points for a coordinate system. Neither existing data nor future data are likely to provide significant information on the .001 angle between the axis of angular momentum and axis of rotation. Existing data have provided data to about .01 accuracy on the pole position and to possibly a meter on the origin of the system and for control points. The longitude origin is essentially arbitrary. While these accuracies permit acquisition of useful data on tides and polar motion through dynamio analyses, they are inadequate for determination of crustal motion or significant improvement in polar motion. The limitations arise from gravity, drag and radiation forces on the satellites as well as from instrument errors. Improvements in laser equipment and the launch of the dense LAGEOS satellite in an orbit high enough to suppress significant gravity and drag errors will permit determination of crustal motion and more accurate, higher frequency, polar motion. However, the reference frame for the results is likely to be an average reference frame defined by the observing stations, resulting in significant corrections to be determined for effects of changes in station configuration and data losses.

Models of Thermodynamic Properties of Prominences

1979 ◽  
Vol 44 ◽  
pp. 349-355
Author(s):  
R.W. Milkey
Keyword(s):  
Thermodynamic Properties ◽  
Mass Transport ◽  
Emission Spectrum ◽  
Thermodynamic Parameters ◽  
Working Group ◽  
Physical Processes ◽  
Theoretical Concepts ◽  
Group 3 ◽  
Observational Techniques

The focus of discussion in Working Group 3 was on the Thermodynamic Properties as determined spectroscopically, including the observational techniques and the theoretical modeling of physical processes responsible for the emission spectrum. Recent advances in observational techniques and theoretical concepts make this discussion particularly timely. It is wise to remember that the determination of thermodynamic parameters is not an end in itself and that these are interesting chiefly for what they can tell us about the energetics and mass transport in prominences.

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