共查询到20条相似文献,搜索用时 15 毫秒
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Broadband probe-fed notched plate antenna 总被引:1,自引:0,他引:1
A probe-fed notched plate antenna for improving the impedance bandwidth is experimentally presented. The notched square plate is suspended above the ground plane. The spacing between the plate and ground plane is ~7% of the operating wavelength. The plate antenna is diagonally fed by a coaxial probe. Measured results show that the notches at the plate function as the reactive loading and, as a result, the enhanced impedance bandwidth reaches the order of 20% without any parasitic elements. The effects of geometric parameters of the plate antenna on the bandwidth are discussed. The radiation patterns and the achieved gains are also examined experimentally 相似文献
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An antenna consisting of the modified rhombic dielectric plate with double tapers in theH -plane excited by the open end of a transverse electric (TE_{10} ) rectangular waveguide is proposed, and some antenna geometrical factors and radiation properties are given experimentally. It is found that these types of antennas have relatively narrow beamwidth and suppressed sidelobe in theH -plane, fairly flat main lobe in theE -plane, and medium performances of about 11.5 dB gain and 1.25 voltage standing-wave ratio (VSWR). It is also found that the radiation performances are virtually independent of frequency over a ten percent bandwidth about 10 GHz. 相似文献
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Based on scalar diffraction optics theory, a new type of mm-wave antenna(diffraction antenna) phase-correcting Fresnel zone plate with continuous structure is described in this paper. It has the advantages of thinner thickness, lighter weight and design flexibility. The design theory and space shadow are discussed in details, and the measured results are presented. The results show that the properties of this kind of antenna is closed to paraboloid reflector. 相似文献
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A novel planar antenna in which radiating slots are arrayed on one side of a square parallel plate waveguide and coupling slots occupy the other side is proposed. The antenna is excited via the coupling slots by a rectangular waveguide. In order to suppress unwanted reflections and to assure the purity of the transverse electromagnetic traveling-wave mode in the parallel plate waveguide, all the slots are arrayed in pairs. An X -band model antenna was fabricated, and uniform aperture illumination was demonstrated with 48% antenna efficiency. These results demonstrate the feasibility of antennas of this type 相似文献
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Coles W.A. Frehlich R.G. Kojima M. 《Proceedings of the IEEE. Institute of Electrical and Electronics Engineers》1994,82(5):697-704
Describes the design and construction of an 8000 m2 74-MHz phased array dedicated to measurement of the solar-wind velocity using the interplanetary scintillation (IPS) technique, and a simple and novel autocalibration system that measures and connects phase and amplitude errors to a level of 1° and 0.2 dB rms. In the IPS technique, intensity fluctuations of compact radio sources caused by plasma turbulence in the solar wind are observed with multiple antennas. The time lag between the antennas is estimated using a cross-correlation analysis. The primary requirement of such a system is sensitivity so that one may observe a large number of compact sources. A secondary requirement is high beam efficiency so that one may observe near the Sun. The scan angle was limited to allow the largest possible array element and thus the simplest feed system. The feed was designed to have independent phase and amplitude control of each element. Although this is not strictly necessary it permits the use of the feed as a phase switched interferometer with which any element can be correlated against any other group of elements. This provides a simple and accurate calibration of the entire array. The antenna was completely prefabricated, the site preparation was minimal, and the installation was quick and accurate. The system is remotely operated. The control information, system diagnostics, and data are transmitted over a leased telephone line. The entire system is powered by storage batteries charged by solar cells. In addition to IFS it has been used extensively for pulsar observations which have similar requirements 相似文献
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A compact patch antenna suitable for mounting above a conducting plate for WLAN operation in the 2.4 GHz band is presented. It is demonstrated that, by introducing a supporting metal plate connected to the antenna ground below, the proposed antenna in free space can easily be mounted at the corner of a conducting plate of various dimensions without rapidly deteriorating the antenna bandwidth. With a compact size of 20times20times6 mm, the antenna can be placed very close to a conducting plate of side length varied from 20 to 200 mm for application in a PC peripheral device 相似文献
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Enlund M.A. Sadrai M.L. Derneryd A. Engstrom U. Johansson M. Svensson B. 《Electronics letters》2005,41(11):626-627
Simulation and measurement results for a parallel plate waveguide antenna designed for a point-to-multipoint communication system at millimetre-wave frequencies is presented. The antenna consists of a waveguide feed, an H-plane horn, an enclosed parabolic reflector, a rectangular waveguide containing irises, and corrugated baffles. Half power beamwidths between 4.9/spl deg/-6.0/spl deg/ in elevation and 58/spl deg/-79/spl deg/ in azimuth are achieved for a bandwidth of 13%. The gain varies between 19 and 20 dBi for the frequency range between 21 and 25 GHz. The manufactured antenna is very compact with a size of 200/spl times/147/spl times/50 mm. 相似文献
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J. C. Chen P. H. Stanton H. F. Reilly Jr. 《Journal of Infrared, Millimeter and Terahertz Waves》1993,14(12):2401-2422
The first Ka-Band Deep Space Network downlink demonstration was recently carried out by the Ka-Band Link Experiment (KABLE) in association with the Mars Observer spacecraft. In order to support the mission, a dichroic plate was required in the DSS-13 beam waveguide antenna to allow simultaneous X- and Ka-Band dual-frequency operation. AnX/Ka/KABLE dichroic plate was designed to transmit a future Ka-Band downlink (31.8–32.3 GHz), future Ka-Band uplink (34.2–34.7 GHz), and KABLE downlink frequency (33.6–33.8 GHz), while reflecting X-band (7.1–8.6 GHz). A computer program was developed for the analysis of a dichroic plate with rectangular apertures using the mode-matching method. The plate was then fabricated and tested. The reflection, group delay, and noise temperature in the antenna system due to the dichroic plate were measured. The experimental results show good agreement with theoretical predictions. 相似文献
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设计了一种小型化双频天线。通过在单极子天线上引入寄生耦合的方法,即在单极子顶部引入耦合加载板,既保证了单极子天线的辐射全向性又减小了电小天线的分布电容,从而使该天线具有宽频带、低剖面特性。采用仿真软件Ansoft HFSS进行仿真和优化,优化结果表明:该天线工作频率为824~960MHz/1 710~2 690MHz(驻波比小于等于2)。根据仿真模型制作了一款天线,实测驻波带宽可达811~1 050MHz/1 580~2 660MHz,且在水平面内辐射全向方向图。该天线在限制尺寸的情况下有效地展宽了带宽。 相似文献
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针对宽波束天线在车载雷达中的应用,突破角雷达方位面3 dB波束宽度的限制,实现微带阵列天线在水平面的宽波束覆盖,设计了一款1×10串馈微带双层结构天线。线阵单元采用道尔夫-切比雪夫(Dolf-Chebyshev)综合法电流分布来达到降低天线俯仰面副瓣的效果,在串馈阵列上方加载寄生贴片和介质基板拓展天线方位面的3 dB波束宽度。分析了双层天线展宽波束的原理,加工并实测了双层宽波束天线,其方位面的3 dB波束宽度为134.6°,增益达到10.6 dB,副瓣电平为-19.8 dB,可以满足车载角雷达天线需求。 相似文献
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为利用微波传输法对大脑活动进行探测,提出了一款应用于大脑活动探测的宽带天线.该天线单元为微带单极子天线,由开槽矩形宽缝、三角形贴片极子和反射板构成,采用微带线馈电,直接与人体头组织介质匹配,经过仿真优化,该天线-10 dB回波损耗带宽覆盖了工作频率范围2.3~8 GHz.并仿真分析了大脑内的电磁能量传输特性及电场分布,结果显示介质匹配天线相比普通天线在头颅内具有更好的穿透能力,在大脑皮层和深部脑区仍存在较强的电场强度.最后对此宽带天线进行了加工测试,实测数据与仿真结果基本吻合.该天线单元尺寸小、结构简单、易加工,能够很好地满足微波传输法探测大脑活动技术中头部共形天线阵列的设计要求. 相似文献
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提出了一种具有陷波特性的新型超宽带Vivaldi天线。采用双Y巴伦实现了微带-槽线过渡,利用多阶阻抗变换器解决了宽带阻抗匹配问题。通过在微带线上添加狭缝,实现了对WLAN应用频段(5.125~5.825 GHz)的隔离,使该天线具有陷波特性。在仿真设计的基础上制作了实验模型,并对其进行了测量。实测结果表明:在超宽带UWB(Ultra Wide-Band)应用频带(3.1~10.6 GHz)范围内,除隔离频带(5.1~6.0 GHz)以外,该天线的驻波比VSWR≤2,辐射方向图定向性较好,且交叉极化较低,从而证明了该天线设计的实用性。 相似文献
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提出了一种L波段的新型天线,能形成全向的水平面方向图,顶空波束宽度可达90°~120°。用高频仿真软件HFSS对天线的电特性进行仿真计算,实验测试结果与仿真结果吻合较好。该天线可应用于电子对抗系统中。 相似文献
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介绍了一种适用于极化捷变天线的可重构射频网络.该射频网络由一个两路可重构Wilkinson功率分配器和两个45°/135°可重构移相器构成,通过控制PIN二极管的偏置电压,可实现两种单路(1:0和0:1)传输模式和三种两路(1:1,1:j和j:1)传输模式,即五种不同的工作模式切换.实测结果表明:该可重构射频网络在单路传输模式(相对带宽6.7%)下的插入损耗小于1.5 dB,输入端口的回波损耗大于12.1 dB;在两路传输模式(相对带宽4.3%)下的输出端口间隔离度大于23.6 dB,相位差为3.5~5.4°(1:1模式)和92.6~97.4°(1:j和j:1模式),相位误差小于7.4°. 相似文献