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Description: This program simulates Gaussian beam propagation through a Fabry-Perot interferometer
％with adjustable error angles.-Gaussian beam prop agation through a Fabry-Perot interferometer % error with adjustable angles.
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Size: 10333 |
Author: 余华清 |
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Description: THIS M-FILE USES THE TRANFER MATRIX METHOD TO EVALUATE THE COUPLED-MODE
％EQUATIONS. THE REFLECTION SPECTRUM OF THE GRATING AND THE TRANSMISSION
％SPECTRUM, DELAY AND DISPERSION OF THE FABRY-PEROT FILTER ARE SIMULATED-THIS M-FILE TRANFER USES THE MATRIX METHOD TO EVALUATE THE COUPLED - MODE EQUATIONS%. THE R EFLECTION SPECTRUM OF THE GRATING AND THE TRANS MISSION% SPECTRUM, DELAY AND DISPERSION OF THE FABRY-Ross PEROT FILTER ARE SIMULATED
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Size: 1663 |
Author: liuliu |
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Description: This program simulates Gaussian beam propagation through a Fabry-Perot interferometer
％with adjustable error angles.-Gaussian beam prop agation through a Fabry-Perot interferometer % error with adjustable angles.
Platform: |
Size: 10240 |
Author: 余华清 |
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Description: THIS M-FILE USES THE TRANFER MATRIX METHOD TO EVALUATE THE COUPLED-MODE
％EQUATIONS. THE REFLECTION SPECTRUM OF THE GRATING AND THE TRANSMISSION
％SPECTRUM, DELAY AND DISPERSION OF THE FABRY-PEROT FILTER ARE SIMULATED-THIS M-FILE TRANFER USES THE MATRIX METHOD TO EVALUATE THE COUPLED- MODE EQUATIONS%. THE R EFLECTION SPECTRUM OF THE GRATING AND THE TRANS MISSION% SPECTRUM, DELAY AND DISPERSION OF THE FABRY-Ross PEROT FILTER ARE SIMULATED
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Size: 1024 |
Author: liuliu |
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Description: 有关光电子学的许多论文，重点是法布里泊罗干涉仪和RPG-Many opto-electronics-related papers, with a focus on Fabry Perot interferometer and RPG
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Size: 4883456 |
Author: 公孙致远 |
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Description: THIS M-FILE USES THE TRANFER MATRIX METHOD TO EVALUATE THE COUPLED-MODE EQUATIONS. THE REFLECTION SPECTRUM OF THE GRATING AND THE TRANSMISSION SPECTRUM, DELAY AND DISPERSION OF THE FABRY-PEROT FILTER ARE SIMULATED
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Size: 1024 |
Author: soft |
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Description: calculate the band of Fabry-Parot Filter -A Fabry-Parot Filter consist of the cavity formed by two highly reflective mirrors placed parallel to each other , as shown in the figure 1.The input light beam to the filter enters the first mirror at right angles to its surface. The output of the filter is the light beam leaving the second mirror. This filter is called Fabry-Parot or etalon. This is a classical device that has been used widely in interferometric applications. Fabry-Parot filters have been used for WDM in several optical network test beds. There are better filters today, such as thin film resonant multi cavity filter and they can still be viewed as Fabry-Perot filter. This type of filter transmits a narrow band of wavelengths and rejects wavelengths outside of that band. An interesting feature of this type of filter is its ability to "select" a different peak wavelength as the filter is tilted
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Size: 1024 |
Author: mengbo |
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Description: This toolkit has two main purposes.
1. Decomposition and visualization of paraxial beams in Hermite-Gaussian and Laguerre-Gaussian bases. (These functions are located in the subdirectory "transverse.")
2. Propagation of such beams through optical systems including two-mirror fabry-perot cavities. (These functions are located in the subdirectory "axial."
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Size: 52224 |
Author: mitko |
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Description: 计算Fabry Perot谐振腔引起的损耗以及对波长的选择作用，考虑入射光角度。-Fabry Perot resonator caused by calculating the loss as well as wavelength selection effect, given the angle of incident light.
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Size: 1488896 |
Author: Korjonyang |
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Description: 光纤光栅法布里—珀罗腔（FBG F-P）的matlab仿真程序。利用光纤光栅的矩阵传输特性。-Fiber Bragg Grating Fabry- Perot cavity (FBG FP) of matlab simulation program. Optical fiber grating transmission characteristics of the matrix.
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Size: 1024 |
Author: 赵一 |
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Description: Matlab code for fabry perot
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Size: 1024 |
Author: fethallah |
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Description: 本文介绍了用来测量对流层温度垂直分布的基于高光谱分辨率雷达技术的瑞利-米激光雷达系统（激光是对人眼安全的355nm波长的紫外线）。在该系统中，用两个法布里-珀罗标准具滤波器对影响大气温度的两个瑞利信号进行过滤。这些滤波器放在瑞利散射频谱的同一侧，并带有双端口光学输出通道。这种配置对米氏散射能获得较高的抑制比以及合理的瑞利散射透光率。米氏信号用第三个位于激光频率中间位置的法布里-珀罗标准具滤波器进行检测。这三个滤波器的参数是经过数值计算优化了的。实验结果表明，对于这两个瑞利通道都能实现-45dB的米散射抑制和大于1 的瑞利透光率。文中还介绍了一种用于校正气溶胶散射实验中所测得的温度（受到气溶胶和云的影响）的方法。初步试验和仿真证明，该设备中的双通道标准具和米散射校正在实际应用中有较高的性能。-A Rayleigh–Mie-scattering lidar system at an eye-safe 355nm ultraviolet wavelength that is based on a
high-spectral-resolution lidar technique is demonstrated for measuring the vertical temperature profile
of the troposphere. Two Rayleigh signals, which determine the atmospheric temperature, are filtered
with two Fabry–Perot etalon filters. The filters are located on the same side of the wings of the Rayleighscattering
spectrum and are optically constructed with a dual-pass optical layout. This configuration
achieves a high rejection rate for Mie scattering and reasonable transmission for Rayleigh scattering. The
Mie signal is detected with a third Fabry–Perot etalon filter, which is centered at the laser frequency. The
filter parameters were optimized by numerical calculation。
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Size: 381952 |
Author: shasha |
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Description: HWM是一个水平上热层中性风的经验模型。它是基于AE-E和DE 2卫星数据获得的。矢量球谐是用来描述一组有限的经向和纬向风分量。第一个版本发布于1987年（HWM87）的模型被用于超过220公里的大风。风的数据列入非相干散射雷达和陆基法布里 - 珀罗光学干涉仪，HWM90向下延伸到100公里，并使用MF/流星数据HWM93延伸到地面。HWM90受太阳活动周期的变化较小，而且并不总是很清楚地划定是当前的数据。该模型描述了从上热层为主的昼夜变化半日变化，低热和过渡从夏季到冬季，冬季到夏季流量低于流量140公里以上的过渡。在一些地方海拔在风中向上延伸至300公里。该模型软件提供指定的纬度，经度，时间，和Ap指数的经向和纬向风。-Brief Description:
The HWM is an empirical model of the horizontal neutral wind in the upper thermosphere. It is based on wind data obtained from the AE-E and DE 2 satellites. A limited set of vector spherical harmonics is used to describe the zonal and meridional wind components. The first edition of the model released in 1987 (HWM87) was intended for winds above 220 km. With the inclusion of wind data from ground-based incoherent scatter radar and Fabry-Perot optical interferometers, HWM90 was extended down to 100 km and using MF/Meteor data HWM93 was extended down to the ground. Solar cycle variations are included (since HWM90), but they are found to be small and not always very clearly delineated be the current data. Variations with magnetic activity (Ap) are included. Mid- and low-latitude data are reproduced quite well by the model. The polar vortices are present, but not to full detail. The model describes the transition from predominately diurnal variations in the upper therm
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Size: 20480 |
Author: Liu Jin |
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Description: fit data for fabry perot interferometer
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Size: 1024 |
Author: ASHRIF |
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Description: HWM是一个水平上热层中性风的经验模型。它是基于AE-E和DE 2卫星数据获得的。矢量球谐是用来描述一组有限的经向和纬向风分量。第一个版本发布于1987年（HWM87）的模型被用于超过220公里的大风。风的数据列入非相干散射雷达和陆基法布里 - 珀罗光学干涉仪，HWM90向下延伸到100公里，并使用MF/流星数据HWM93延伸到地面。HWM90受太阳活动周期的变化较小，而且并不总是很清楚地划定是当前的数据。该模型描述了从上热层为主的昼夜变化半日变化，低热和过渡从夏季到冬季，冬季到夏季流量低于流量140公里以上的过渡。在一些地方海拔在风中向上延伸至300公里。该模型软件提供指定的纬度，经度，时间，和Ap指数的经向和纬向风。-The HWM is an empirical model of the horizontal neutral wind in the upper thermosphere. It is based on wind data obtained from the AE-E and DE 2 satellites. A limited set of vector spherical harmonics is used to describe the zonal and meridional wind components. The first edition of the model released in 1987 (HWM87) was intended for winds above 220 km. With the inclusion of wind data from ground-based incoherent scatter radar and Fabry-Perot optical interferometers, HWM90 was extended down to 100 km and using MF/Meteor data HWM93 was extended down to the ground. Solar cycle variations are included (since HWM90), but they are found to be small and not always very clearly delineated be the current data. Variations with magnetic activity (Ap) are included. Mid- and low-latitude data are reproduced quite well by the model. The polar vortices are present, but not to full detail. The model describes the transition from predominately diurnal variations in the upper therm
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Size: 19456 |
Author: jlp |
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Description: 光器件所用F-P腔的matlab模拟资料-FP cavity optical devices used in the matlab simulation data
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Size: 236544 |
Author: 卢卫东 |
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Description: THIS M-FILE USES THE TRANFER MATRIX METHOD TO EVALUATE THE COUPLED-MODE
EQUATIONS. THE REFLECTION SPECTRUM OF THE GRATING AND THE TRANSMISSION
SPECTRUM, DELAY AND DISPERSION OF THE FABRY-PEROT FILTER ARE SIMULATED
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Size: 1024 |
Author: yuan |
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Description: OSCAR is an optical FFT code used to calculate the steady state optical
eld circulating in Fabry Perot cavities. The code can integrate non-sperical
mirrors and any arbitrary input elds. Recent applications for OSCAR have
been: calculation of thermal lensing e ect and calculation of di raction loss
and cavity eigen modes for mesa beams. One great advantage of OSCAR is
the simplicity and
exibility of the code, everyone with only minimal knowl-
edge of Matlab can easily modi ed OSCAR code to suit spec c purposes.
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Size: 3879936 |
Author: habib |
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Description: OSCAR is an optical FFT code used to calculate the steady state optical field circulating in Fabry Perot cavities. The code can integrate non-sperical mirrors and any arbitrary input fields. Recent applications for OSCAR have
been: calculation of thermal lensing effect and calculation of diffraction loss and cavity eigen modes for mesa beams. One great advantage of OSCAR is the simplicity and exibility of the code, everyone with only minimal knowl- edge of Matlab can easily modifed OSCAR code to suit specfic purposes.
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Size: 2003968 |
Author: habib |
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Description: 高斯光束在F-P干涉仪中的传输模拟(Simulates Gaussian beam propagation through a Fabry-Perot
interferometer with adjustable error angles.)
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Size: 9216 |
Author: liuliuyunpeng
|
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