伪码引信瞄准式压制性干扰及硬件实现

伪随机码调相引信在舰空导弹和地空导弹中有广泛的应用,因此有必要对此类引信的干扰进行研究。提出了一种瞄准式压制性干扰方案。该方案中,干扰机先接收引信的辐射信号,然后对准引信工作频率,发射一个可与引信工作带宽相比拟的窄带噪声或类似噪声的干扰信号去干扰引信,使引信自身的相关接收失效,从而达到干扰引信工作的目的。给出了此方案的部分实现电路的工作原理和硬件实现,主要包括伪码调相信号的解调、解调后的码元整形和识别、低频噪声源的产生、干扰波形的调制发射等关键部件。根据各部分电路的试验结果认为,提出的干扰机设计原理正确,干扰方案有效可行。     

Pulsar radio emission

25 years after their discovery, pulsars still pose fundamental problems, in particular when the whole range of their periodsP is considered: 1.56 ms P0.09 s. This communication reviews my understanding of the pulsar magnetosphere, windzone, and (coherent) radio emission. New are details of the preferred magnetic structure, wind generation, and amplification of the emitted (pseudo) curvature radiation, the inferred brightness of which exceeds that of all other terrestrial and astrophysical sources by many orders of magnitude.     

Global monitoring of tropospheric water vapor with GPS radio occultation aboard CHAMP

The global positioning system radio occultation (GPS RO) technique provides a powerful tool for atmospheric sounding which requires no calibration, is not affected by clouds, aerosols or precipitation, and provides an almost uniform global coverage. The paper deals with application of GPS RO measurements from CHAllenging Minisatellite Payload (CHAMP) for the retrieval of tropospheric water vapor profiles. CHAMP RO data are available since 2001 with up to 200 high resolution atmospheric profiles per day. We introduce a new direct method for water vapor retrieval from GPS RO data. Additionally, a 1Dvar algorithm is used for this purpose. The so derived CHAMP water vapor profiles are validated with radiosonde data on a global scale. Here, both methods come to statistically comparable results revealing a negative bias of less than 0.1 g/kg and a standard deviation of less than 1 g/kg specific humidity in the mid troposphere. Potentials of CHAMP RO retrievals for monitoring the mean tropospheric water vapor distribution on a global scale are presented.     

基于乘波体的高超音速运载器气动布局设计

采用基于无粘锥形流的反设计方法以Ma=6为设计点设计具有高升阻比的乘波体外形;取基准圆锥激波角为12°,并利用上表面的膨胀降压作用,这一外形优化有效提高了乘波体的升阻特性,在考虑粘性影响的情况下Ma=6时的升阻比可从3.356?3提高到4.598?1;将具有高升低阻效能的乘波体作为机身初步设计单级入轨运载器布局,通过数值模拟的方法进行研究,结果表明布局在大速度范围内的升阻比得到了令人满意的结果,同时具备静稳定性.     

快变分量观测与基本分量特性

本文对太阳２２周峰年期云南天文台日冕射电频谱仪观测到的６０个快速事件作了分析。从中获得了尖峰辐射、增强噪暴、快速起伏、类尖峰、叠加脉冲五种快变型别，对它们的亮温度、叠加特性、特征时间、辐射源尺度、偏振特性以及辐射机制六个方面作了分析研究后，对射电爆发、缓变分量和宁静太阳的辐射特征参量也作了研究，从而得出基本分量特性。     

大功率无线电波与低电离层的相互作用

地面入射的大功率无线电波能加热电离层等离子体，引起电离层电子温度和密度的扰动，实现电离层的地面人工变态．本文中，着重考虑电波和电离层相互作用过程中的自吸收，构造一个自治的相互作用模型，在一定功率和频率的加热电波作用下，利用该模型计算了白天低电离层电子温度和由温度的变化而引起的电子密度的变化．计算结果表明，在白天低电离层，电波的自吸收在90km以下比较显著，而最大温度变化在70km高度上，大约增加了2倍．在α复合的假设下，电子密度变化幅度随高度的增加而减少，在70km处，大约增加55％、120km处则为4％左右．     

一种软件科斯塔斯环的模型建立与实现

文章通过双线性变换法建立了科斯塔斯环的Z域模型，分析了Z域模型下环路各项性能指标和环路参数之间的关系，系统总结了设计步骤和参数的选择方法。试验仿真结果证明捕获与跟踪性能符合理论分析。最后给出了科斯塔斯环在FPGA中的硬件实现结构。     

Multi-scale reconnections in a complex CME

A series of three flares of GOES class M, M and C, and a CME were observed on 20 January 2004 occurring in close succession in NOAA 10540. Types II, III, and N radio bursts were associated. We use the combined observations from TRACE, EIT, Hα images from Kwasan Observatory, MDI magnetograms, GOES, and radio observations from Culgoora and Wind/ WAVES to understand the complex development of this event. We reach three main conclusions. First, we link the first two impulsive flares to tether-cutting reconnections and the launch of the CME. This complex observation shows that impulsive quadrupolar flares can be eruptive. Second, we relate the last of the flares, an LDE, to the relaxation phase following forced reconnections between the erupting flux rope and neighbouring magnetic field lines, when reconnection reverses and restores some of the pre-eruption magnetic connectivities. Finally, we show that reconnection with the magnetic structure of a previous CME launched about 8 h earlier injects electrons into open field lines having a local dip and apex (located at about six solar radii height). This is observed as an N-burst at decametre radio wavelengths. The dipped shape of these field lines is due to large-scale magnetic reconnection between expanding magnetic loops and open field lines of a neighbouring streamer. This particular situation explains why this is the first N-burst ever observed at long radio wavelengths.     

EUV and Radio Observations of an Equatorial Coronal Hole

An equatorial coronal hole has been observed on 18 and 19 October 1996 with SOHO-CDS and with the Nancąy Radioheliograph (RH). The CDS EUV line intensities are used to determine the coronal hole Differential Emission Measure (DEM); in turn this is used to compute the radio brightness temperature T_b at the observed frequencies, leaving the coronal electron temperature and density as free parameters. EUV line intensities, calculated from the derived models, show a good agreement with EUV observations. This revised version was published online in June 2006 with corrections to the Cover Date.     

射频识别卡读写模块的设计

射频识别卡读写模块是射频卡读写器的核心.根据ISO14443协议,运用现代通信与信号处理的方法,采用最新的RISC指令单片机,设计了射频识别卡的读写模块.该模块没有使用专用的硬件ASIC和功率放大管,纯粹采用软件实现了硬件ASIC的功能.同时它性能稳定、价格低廉,对卡的读写距离在0~10cm.