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A 220–280 GHz dual polarization receiver has been built for the James Clerk Maxwell Telescope. Schottky diode mixers cooled to 15K by a closed-cycle refrigerator are used to give DSB noise temperatures of 300K and 420K in the two channels. The optical design is based on gaussian-beam optics, and is frequency independent; it allows the significant higher order gaussian modes to propagate unhindered, thus offering the prospect of very high aperture efficiency. The receiver includes a number of novel optical components, including a completely symmetric dual polarization Martin-Puplett interferometer, used as the L.O. injection diplexer; a dielectric waveplate used as an in-line variable polarization splitter; and a dual-polarization in-line tunable Fabry-Perot SSB filter. Measurements of the performance of the optical system are presented.  相似文献   
3.
Present and near future limb-sounding heterodyne instruments operating at millimeter or sub-millimeter wavelengths will be capable to gather profile information on a variety of stratospheric trace gases with relatively strong spectral features such as O3, H2O, O2 (temperature), N2O, HCl, ClO, HNO3, CH3Cl, and CO. Some species however, which are of particular interest for the understanding of stratospheric ozone chemistry, have only very weak spectral signatures, either due to their very small abundances and/or spectroscopic properties. These are amongst others the radical BrO, the potential bromine reservoir HBr, HOCl as a member of the chlorine family, and the hydroperoxyl radical HO2. Often, these target species are very difficult to detect and profiles have not yet been measured by space-borne sensors at all, even considering other spectral ranges and observation techniques. A study was therefore dedicated to the investigation of the retrieval of species with spectral features close to the detection limit of a typical state-of-the-art space-borne heterodyne receiver. A survey of the millimeter- and sub-millimeter spectral range was performed in order to identify appropriate spectral bands, followed by retrieval simulations for a representative atmospheric and instrumental scenario in order to explore the relative merits of the pre-selected bands and to derive associated parameters as measurement precision, altitude range and resolution. The feasibility of retrieving profile information from limb observations at sub-millimeter wavelengths of the “weak line” species under investigation is demonstrated. Optimal dedicated bands are recommended for HBr , BrO , and HOCl . For HO2 five more or less equivalent bands between 585 and are identified.  相似文献   
4.
为了测量 HL-2M 装置中的电子温度剖面分布,研制了一套扫频电子回旋辐射(SECE)系统。该系统 能够测量装置中心纵场大小在 1.4~2.2T 时的等离子体电子温度。采用扫频外差接收的方式,径向空间分辨达到 2.5cm,时间分辨达到 1ms。接收机前端的准光学系统采用两级金属反射镜的配置,系统能够接收的最小极向光 斑的直径为 1.5cm(波数 kθ<4.2rad·cm-1)。系统的频带范围覆盖 33~110GHz,采用 VCO 作为本振源,双边带混频 输出中频信号。后端首次采用高性能对数检波器解调中频,能直接对-70dBm 的微弱信号进行检测,输入-输出工 作区间的动态范围达到 45dB 以上。在实验期间,成功测量到了等离子体中电子逃逸以及回旋辐射产生的信号。  相似文献   
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光纤水听器是水声研究领域的关键技术,在实际应用中具有显著优势,广泛应用于AUV导航定位、资源勘探、海水警戒等场景.光纤水听器将声信号转化为光信号传播,在接收信号时就需要对光信号进行解调提取出声压信号.总结了几种常用的信号解调算法及关键技术,包括PGC解调法、3×3耦合器解调法和外差解调法;介绍了各种解调算法的基本原理和...  相似文献   
6.
非对称空间外差光谱技术是一种新型的超高分辨率遥感探测技术,要求后期的数据处理技术也具有相应的超高准确度.从数字信号处理的角度,提出了一种自适应的频率跟踪处理方法,根据信号的空间频率来插值补偿信号的相位偏移,并且递归迭代出最接近真实值的相位信息.经仿真实验对比验证表明,在噪声干扰强度不大的条件下,相较于传统傅里叶变换方法,本文算法对信号频率和相位提取的准确度提高了约100倍以上,能够有效降低非对称空间外差光谱技术的系统误差.  相似文献   
7.
1.06 μm相干激光雷达动目标多普勒信号探测   总被引:2,自引:1,他引:1  
介绍了一套1.06 μm脉冲式相干激光雷达测速演示系统.采用单块非平面环形激光器作为种子,注入到单纵模运转的Q开关高重复频率Nd∶YAG激光器为发射源,实现稳定的单频输出.通过外差式相干探测的方法,利用转速0~60 Hz可调、直径为10 cm的转盘为运动目标,回波信号被带宽为3.5 GHz的高速光电探测器响应后,经采样率为2.5 GS/s的A/D采样,输送到基于LabVIEW信号处理系统中,从而测量不同转速下的多普勒频移,各测速点的多普勒频移测量结果相对误差在3%以内.针对测量中存在的误差从激光器输出线宽和测速系统准确度两方面进行了误差分析,并提出了改进措施.演示系统的良好重复性证实了这种相干激光雷达系统的可行性.  相似文献   
8.
If the incident angle of a light beam on the boundary surface between the thin metal film of a surface plasmon resonance (SPR) apparatus and a test medium is equal to or very near the resonant angle, then the phase difference between the p- and s-polarizations of the reflected light is related to the associated physical parameter. The phase difference can be measured accurately with heterodyne interferometry. If the relationship between the phase difference and the associated physical parameter is specified, then the associated physical parameter can be estimated from the phase difference data. This method has the benefits of both common-path interferometry and heterodyne interferometry, such as simple structure, high stability, high resolution, easy operation, and rapid real-time measurement.  相似文献   
9.
A powerful method for the phase retardation measurement of a reflective liquid crystal cell is presented. The proposed method is based on the heterodyne interferometer theory for probing cell parameters. Due to common-path optical arrangement, a fast measurement with high accuracy and sensitivity was possible. Both theoretical analysis and experimental procedures are presented. The experimental results agree well with that obtained theoretically.  相似文献   
10.
A novel heterodyne detection scheme for light-induced transient grating technique is presented. The heterodyne detection is achieved coherently mixing the picosecond pulses of diffracted and scattered light. A phase difference between these pulses is controlled by moving a holographic beam splitter along its grating vector. This approach is employed to study a competition of coexisting electronic and thermal optical nonlinearities in CVD grown diamond films in sub-nanosecond time domain and to determine carrier parameters.  相似文献   
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