Project-Based Learning (PBL) is an effective way to develop students' engineering practice skills. In order to cultivate the engineering personnel to meet the needs of society through school-enterprise cooperation, School of Optics and Photonics, Beijing Institute of Technology constructed a school-enterprise cooperation platform by utilizing the in-school resources, in which the in-school instructor is the leader and enterprise tutor is the link. Applying the PBL concept, the training mode for cultivating the engineering practical ability of professional degree master has been designed and investigated. The initial trial teaching and platform operation attempt was jointly carried out by School of Optics and Photonics with Beijing Advanced Innovation Center for Intelligent Robots and Systems (BAICIRS) of Beijing Institute of Technology, which verified the feasibility of the teaching model and provided the future teaching research direction and platform construction. There are important reference values for conclusions.
High-performance UAV has been popular and in great need in recent years. The paper introduces a new method in debugging Quadrotor UAVs. Based on the infrared thermal technology and heat transfer theory, a UAV is under debugging above a hot-wire grid which is composed of 14 heated nichrome wires. And the air flow propelled by the rotating rotors has an influence on the temperature distribution of the hot-wire grid. An infrared thermal imager below observes the distribution and gets thermal images of the hot-wire grid. With the assistance of mathematic model and some experiments, the paper discusses the relationship between thermal images and the speed of rotors. By means of getting debugged UAVs into test, the standard information and thermal images can be acquired. The paper demonstrates that comparing to the standard thermal images, a UAV being debugging in the same test can draw some critical data directly or after interpolation. The results are shown in the paper and the advantages are discussed.
Based on the complex movement of satellite platform, we take the impacts on spectral imaging by pitch, roll and yaw
into account. Then point spread matrix calculation principle is put forward, which takes transform the POS data into
point spread matrix. According to this theory, we proposed the concept of pseudo cross-correlation to set up the model of
spectral imaging degradation based on the pseudo cross-correlation, which combines the point spread matrix and original
spectral data by the concept of pseudo cross-correlation. And in this method, the process of spectral imaging degradation
is formed, which improve the existing problem of spectral imaging degradation based on the complex movement of
satellite platform. The simulation results show that this kind of degradation theory is suitable for solving the problem of
spectral imaging degradation based on the complex satellite platform movement completely.
Based on the spectrum rebuilding technology of spatially modulated imaging spectrometer, a real-time data gathering and
spectrum rebuilding system of all reflection Fourier Transform imaging spectrometer is built on FPGA. It integrates
interferogram sampling, spectrum rebuilding, data restoring, VGA display and data transmission on a single chip of
FPGA and can make them accomplished in real-time. This paper presents the key technology and the spectral calibration
study of this system. Using a mercury lamp as the calibration source, the calibration experiments have been carried on
this FPGA-based system. After analysis the experimental results, a function of pixel number-wave number has been established, and the wave number resolution has been got, which is same to the resolution got by a computer-based system.
In this paper, the researches and experiments on the feasibility of a common aperture active imaging system using a
polarization beam splitter have been presented. The system includes a CCD imaging unit, a semiconductor laser unit, a
polarization beam splitter, a linear polarizer, a quarter-wave plate, a telescope objective, a designed laser collimating
lens and mechanical assembling structures. According to the analysis with Jones matrix, the system gains remarkably
high utilization ratio of luminous energy. Also, the system can reach an illuminating distance of 3km, a laser divergence
angle of 0.504° and a degree of uniformity of 83% theoretically. The experiments have been conducted to obtain images
of objects at 300m and 3km. From the results, clear illuminated objects can be identified and no impacts of back
scattering of atmosphere turbulence have been detected. However, to make this kind of systems more effective, higher
demands on the extinction ratio, reflectivity and transmissivity of the polarized components and the uniformity of the
illuminating spot should be met.
Since the absorption of ultraviolet radiation in the atmosphere is strong, it is difficult to image solar UV
radiation using ground-based telescopes. While, the moon which has no atmosphere and has stability
geological structure and low magnetic field, observing the sun on the moon is more suitable than observing
the sun on the earth. This paper describes the design of lunar-based solar telescope which can image the sun
in three wavelength: long-wave IR (8-12μm), visible (400-900nm) and UV(100-400nm). The telescope is
mainly composed of two parts: reflective telescope and splitting system. This design effectively avoids the
material restrictions of IR and UV imaging optical systems. The rationality of the optical system design of
the common aperture multi-wavelength telescope was proved by comparing the results with the images get
by single wavelength solar telescopes all over the world. Compared the images took under different weather,
the importance of the proposition of lunar-based devise is proved. Combined the splitters and the spectral
response range of detectors, the UV, visible and IR can be split and imaged by different detectors.
This paper describes a design of sun-tracking warning demonstration system in solar blind UV. After analyzing of the
system structure and guide line of the sun-tracking warning system in solar blind UV, the key techniques of the
sun-tracking UV warning system are discussed and designed, including the optical system, UV filter module, optical
modulation system, UV detectors and its sun-tracking servo. A total reflect Cassegrain UV optical system with simple
structure, reliable performance and high-quality imaging ability is designed and manufactured. In order to enhance the
received SNR and process the signal easily, an optical UV filter and an optical modulation reticle are used to filter and
modulate the target's direct signals to alternating signal. Functional experiments show that sun-tracking warning system
needs better UV filter module whose total stopband rejection should be higher than 10-10.
The definition and classifications of the UV communication are described in the paper. The UV channel
consists of three sections: propagation loss section, scattering section and background-noise section. The
principle of selecting the wave band of UV communication is analyzed. The LOS and NLOS (a) transmission
models are presented, and the two configurations are well proved by outdoor experiments. The experiment
results also show that the communication distance of LOS can go up to 5kms, and NLOS(a) can reach 2kms
with the UV detectors at present.
On the basis of the principle of single quarter wave plate method, a model of automatic whole-field measuring optical
glass stress is presented, which is called "4+1steps phase shifting method" including the model for the isoclinic
parameter and the stress birefringence. According to this model, an automatic whole-field measuring system is
established. The correctness of the model was testified by numeric emulation experiments under the preset conditions of
isoclinic angle and stress birefringence. Practical measurement obtained a result coincident with the actual distribution of
the isoclinic angle and the birefringence. The automatic whole-field measuring model and system can achieve the whole
process intelligently and automatically, and dispose the disadvantages of tradition method about interpreting the stress
level by subjective judging birefringence of some selected spots.
A LOS solar blind UV communication channel model is presented in the paper, which consists of three sections: propagation loss section, scattering transmission section and background noise section. LOS transmission loss model of UV channel is deduced by Lambert law and noise power calculation is also analyzed. Base on them, a practicable calculation method of signal to noise ratio (SNR) is presented, which is a bridge between system parameters and system performances such as BER and limit communication distance in analysis of UV communication. Transmission loss and SNR of LOS are measured in outdoor experiments. The experiment shows that SNR calculation data agree with the experimental results quite well. The calculation also shows that the limit communication distance of LOS can achieve 7kms with the UV sensor at present.
KEYWORDS: Image transmission, Image compression, Signal to noise ratio, Mobile communications, Telecommunications, Signal processing, Error control coding, Interference (communication), Data modeling, Chlorine
A new trellis decoding method of block codes based on the GAC structure is applied to Rayleigh fading channels in this paper. Performance of this decoding technique with hard- decision and soft-decision is studied respectively. Researches are also carried out to introduce this maximum- likelihood decoding method to narrow-banded mobile image transmission systems.
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