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101.
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A novel architecture for computing the fast Fourier transform ( FFT ) on programmable devices is presented.To improve the system operation speed , a hybrid parallel FFT algorithm is used.Results indicate that the use of an 8×8parallel structure for realizing the 64-point FFT leads to a 8times higher processing speed compared with its counterparts employing other series of techniques. 相似文献
104.
S.S. Nikte A.K. Sharma D.P. Nade M.V. Rokade R.N. Ghodpage P.T. Patil R.V. Bhonsle 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
A dual dipole antenna has been installed at low latitude station Kolhapur (Geographic 16.8°N, 74.25°E), Maharashtra, India for the study of cosmic radio noise absorption using Solid State Riometer (which operates at 30 MHz) during pre phase of 24th solar maxima. The aim for this type of study over Kolhapur was to know the response of lower (D region) ionosphere over low latitude by cosmic radio noise absorption using riometer technique during quite period as well as sudden ionospheric disturbances (SID). The observations are being taken for 3 years. Two different sites (∼40 km away from each other) were used for the installation of riometer equipment assuming minimum local noise. It is found that solar noise to cosmic radio noise hence resulting in signal saturation. The night time signal is relatively free of interference but sometimes local noise is responsible for spike-like signatures. Hence it is concluded that Kolhapur (a low latitude station) is not suitable for the study of cosmic radio noise absorption on 30 MHz with riometer and dual dipole antenna. Proper choice for operating frequency of riometer and antenna gain is suggested for low latitude use of this technique for ionospheric deviative and nondeviative absorption studies. 相似文献
105.
L.I. Dorman I.V. Dorman 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
A short history of the beginning of cosmic ray (CR) astrophysics is considered: from the hypothesis on CR origin as a result of Supernova explosions in the Metagalaxy, to a model of solar origin of CR, galactic origin based on the stochastic mechanism of charged particle acceleration in interstellar space, to extragalactic and hierarchical models of CR origin, as well as galactic CR origin taking into account radio-astronomical data. We consider also the first balloon results on the chemical contents of primary CR (especially of the contents Li, Be, B), important for any model of CR origin. Investigations of the injection problem, CR drift and diffusion acceleration by shock waves, and CR generation in Supernova remnants were also important steps in the beginning of CR astrophysics. 相似文献
106.
F.X. Esnault N. Rossetto D. Holleville J. Delporte N. Dimarcq 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
HORACE (HOrloge à Refroidissement d’Atomes en Cellule = clock based on atoms cooled from vapour cell) is a compact cold caesium atom clock developed in SYRTE at Paris Observatory. This clock can operate both on ground and in microgravity environment. Design of HORACE is based on isotropic light cooling, allowing performing the whole clock sequence (cooling, atomic preparation, Ramsey interrogation and detection) at the same place. Compared to more conventional cold atom clocks such as atomic fountains, the use of isotropic light cooling simplifies both the optical part of the setup and the detection sequence, and leads to a drastic size reduction of the physics package. Very good short-term performances have been demonstrated at SYRTE since relative frequency instability of 2.2 × 10−13 τ−1/2 has been obtained. Optimization of the long term stability is still under progress and current results show relative frequency instability around 3 × 10−15 in 104 s of integration. With these performances, HORACE appears as a good candidate both for Galileo’s ground segment clock and for onboard Galileo clock. 相似文献
107.
针对密集读写器环境下的无线射频识别(RFID,Radio Frequency Identification)多读写器冲突情况,提出了一种基于随机时隙并通过中央计算机协调的读写器防冲突方法.首先,中央计算机发送每轮起始命令和时隙指令,读写器根据当前利用率随机选择时隙.选择当前时隙的读写器若没有接收到忙信号则发送信标并侦听,若无邻近读写器发送信标则开始读写标签,否则该轮回停止工作.若时隙末存在没有接收到忙信号的读写器则在额外时隙发送二次信标.与现有的分布式防冲突方法相比,该方法具有较好的吞吐量和公平性. 相似文献
108.
M. Abada-Simon A. Lecacheux T. S. Bastian J. A. Bookbinder G. A. Dulk 《Space Science Reviews》1994,68(1-4):291-292
We report the first millimetric detections of the magnetic cataclysmic variable AE Aquarii, accompanied by contemporaneous microwave observations. These data show that the time-averaged spectrum is well fit by a power-law which extends to mm wavelengths. We suggest that the spectrum is consistent with that expected from a superposition of flare-like events. 相似文献
109.
一个设计不好的无线电发射机, 工作时产生的谐波十分严重, 而接收设备又对电磁干扰非常敏感。本文介绍了发射机谐波的抑制方法和接收机抗干扰技术体制, 实现自适应通信, 确保通信质量。 相似文献
110.
软件无线电中FSK信号解调的一种快速算法 总被引:4,自引:0,他引:4
訾学博 《沈阳航空工业学院学报》2003,20(2):55-57
本文介绍了采用差分检波解调算法实现软件无线电中移频键控信号(FSK)快速解调方祛,并通过数字信号处理技术验证了该解调方祛。 相似文献