scholarly journals Proposed Method For Improving The Performance Of Wireless Optical Link FSO Using The Center Of Balance With a Laser Fog Sensor

Author(s):  
Mazen Abdullatif ◽  
Mohammed Haji Ali ◽  
Rami Khal

In this research, the problem of the optical link in different fog cases was solved through the use of the proposed center balance with the RF link, where this center adjusts the power of the laser transmitter according to the damping of the optical link, where the length of the transmitted signal is increased which leads to overcome dispersion. Measurements are carried out by three fog laser sensors located at the beginning, middle and end of the optical link. These sensors generate voltage proportional to the amount of fog and then send these values ​​using radio waves RF to the equilibrium center, which calculates the average damping value and adjusts the power value of the laser transmitter according to the damping coefficient value. Simulated using OPTISYSTE programming environment and MATLAB environment, MIE dispersion was adopted in wireless optical link and transmitted signal wavelength 1550nm where quality coefficient was improved from 3.6% to 44.45% in moderate, light and very light fog

2019 ◽  
Vol 20 (1-2) ◽  
pp. 109-112
Author(s):  
Jarosław Moczarski

Paper discussed the problem of rolling stock elements identification and recognition of loads. For evaluation of the object shape and position, in the tests are used laser sensors such as mid-range distance sensors, automation light grids and 2D laser measurement sensors. For the creation of digital models of the studied objects and their subsequent identification there was developed a computer application working in Matlab programming environment. Typologization of models of rolling stock elements accelerate calculations and increase the effectiveness of the conducted identification.


2021 ◽  
Vol 11 (5) ◽  
pp. 2329
Author(s):  
Jaeseong Choi ◽  
Jung Hwan Ahn ◽  
Hwa Young Kim

A pilot-operated solenoid valve is used to control ultra-high pressure vessels. However, it is difficult to understand its dynamic behavior because the valve operates under ultra-high pressure conditions and the driving unit moves in a multi-step fashion in a tight hidden space. This study aims to identify the system coefficient, especially the damping coefficient, required to analyze the dynamic behavior of a solenoid driving unit. Experiments to measure the dynamic behavior of the driving unit are conducted using two laser sensors and one accelerator. The damping coefficient is estimated using Matlab Simulink, by varying the damping coefficient to match the experimental results. The obtained system coefficients are modeled as equations of motion. It is verified that the valve motion consists of two sequential movements—Phase 1 by pilot plunger and Phase 2 by main plunger, pilot plunger, and the valve initiation time is as fast as 9.9 ms. The damping coefficient of each phase is estimated 0.001 N ∙ s/mm for Phase 1, 0.004 N ∙ s/mm for Phase 2.


1994 ◽  
Vol 144 ◽  
pp. 21-28 ◽  
Author(s):  
G. B. Gelfreikh

AbstractA review of methods of measuring magnetic fields in the solar corona using spectral-polarization observations at microwaves with high spatial resolution is presented. The methods are based on the theory of thermal bremsstrahlung, thermal cyclotron emission, propagation of radio waves in quasi-transverse magnetic field and Faraday rotation of the plane of polarization. The most explicit program of measurements of magnetic fields in the atmosphere of solar active regions has been carried out using radio observations performed on the large reflector radio telescope of the Russian Academy of Sciences — RATAN-600. This proved possible due to good wavelength coverage, multichannel spectrographs observations and high sensitivity to polarization of the instrument. Besides direct measurements of the strength of the magnetic fields in some cases the peculiar parameters of radio sources, such as very steep spectra and high brightness temperatures provide some information on a very complicated local structure of the coronal magnetic field. Of special interest are the results found from combined RATAN-600 and large antennas of aperture synthesis (VLA and WSRT), the latter giving more detailed information on twodimensional structure of radio sources. The bulk of the data obtained allows us to investigate themagnetospheresof the solar active regions as the space in the solar corona where the structures and physical processes are controlled both by the photospheric/underphotospheric currents and surrounding “quiet” corona.


1933 ◽  
Vol 148 (5) ◽  
pp. 272-273 ◽  
Author(s):  
J. H. Davis
Keyword(s):  

2019 ◽  
pp. 55-58
Author(s):  
A. S. Putina

The article discusses the problems of organizing group work in education, in particular, group work in the Scratch visual programming environment, where it is possible to use tools that help in teamwork — Backpack, Remix, Scratch Studio. An example of creating a project by a group of students is given.


Author(s):  
Bagus Septyanto ◽  
Dian Nurdiana ◽  
Sitti Ahmiatri Saptari

In general, surface positioning using a global satellite navigation system (GNSS). Many satellites transmit radio signals to the surface of the earth and it was detected by receiver sensors into a function of position and time. Radio waves really bad when spreading in water. So, the underwater positioning uses acoustic wave. One type of underwater positioning is USBL. USBL is a positioning system based on measuring the distance and angle. Based on distance and angle, the position of the target in cartesian coordinates can be calculated. In practice, the effect of ship movement is one of the factors that determine the accuracy of the USBL system. Ship movements like a pitch, roll, and orientation that are not defined by the receiver could changes the position of the target in X, Y and Z coordinates. USBL calibration is performed to detect an error angle. USBL calibration is done by two methods. In USBL calibration Single Position obtained orientation correction value is 1.13 ̊ and a scale factor is 0.99025. For USBL Quadrant calibration, pitch correction values is -1.05, Roll -0.02 ̊, Orientation 6.82 ̊ and scale factor 0.9934 are obtained. The quadrant calibration results deccrease the level of error position to 0.276 - 0.289m at a depth of 89m and 0.432m - 0.644m at a depth of 76m


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