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271.
M. Pietrella L. Perrone G. Fontana V. Romano A. Malagnini G. Tutone B. Zolesi Lj.R. Cander A. Belehaki I. Tsagouri S.S. Kouris F. Vallianatos J. Makris M. Angling 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
After a first oblique-incidence ionospheric sounding campaign over Central Europe performed during the period 2003–2004 over the radio links between Inskip (UK, 53.5°N, 2.5°W) and Rome (Italy, 41.8°N, 12.5°E) and between Inskip and Chania (Crete, 35.7°N, 24.0°E), new and more extensive analysis of systematic MUF measurements from January 2005 to December 2006 have been performed. MUF measurements collected during moderately disturbed days (17 ? Ap ? 32), disturbed days (32 < Ap ? 50) and very disturbed days (Ap > 50), have been used to test the long term prediction models (ASAPS, ICEPAC and SIRM&LKW), and the now casting models (SIRMUP&LKW and ISWIRM&LKW). The performances of the different prediction methods in terms of r.m.s are shown for selected range of geomagnetic activity and for each season. 相似文献
272.
R.R. Rosa M. Karlický T.B. Veronese N.L. Vijaykumar H.S. Sawant A.I. Borgazzi M.S. Dantas E.B.M. Barbosa R.A. Sych O. Mendes 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
We analyze the weak component of the localized temporal pattern variability of 3 GHz solar burst observed by the Ondrejov radiospectrograph. A complex, short and weak impulsive sample from the time series was analyzed by applying a method based on the gradient pattern analysis and discrete wavelet decomposition. By analyzing canonical temporal variability patterns we show that the new method can reliably characterize the phenomenological dynamical process of short time series (N ? 103 measurements) as the radio burst addressed here. In the narrowest sense, by estimating the mutual information distance in the gradient spectra, we show that the fluctuation pattern of the short and weak 3 GHz impulsive solar burst, with energetic amplitudes <350 SFU, is closer to the intermittent and strong MHD turbulent variability pattern. 相似文献
273.
L. van Driel-Gesztelyi C.P. Goff P. Démoulin J.L. Culhane S.A. Matthews L.K. Harra C.H. Mandrini K.-L. Klein H. Kurokawa 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
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. 相似文献
274.
275.
为了模拟无线电引信中的Chirp信号,设计了一种基于DDS的无线电引信Chirp信号生成系统的方案。该方案采用PC输出波形控制参数,用DSP进行数字信号处理并控制DDS芯片的总体结构。对PC与DSP芯片的通信接口、DSP芯片与DDS芯片的接口以及软件处理流程进行了详细设计。 相似文献
276.
277.
电磁散射场和雷达散射截面积的计算 总被引:2,自引:1,他引:1
薛晓春 《北京航空航天大学学报》1998,24(2):193-196
计算了绕二维物体的时域电磁散射场的空间分布和雷达散射截面积 (RCS).通常的电磁场计算是频域的,采用高频计算方法,而流场计算是时域的.由于以研究流场--电磁场优化设计计算为目的,需要统一采用时域计算,因此重点采用矢通量分裂法这种时域方法计算了RCS ,通过将特征值分裂为正负两部分,抑制了各自的误差.此外,采用LaxWendroff方法作为对照.两种方法的结果一致. 相似文献
278.
电离层对单频卫星导航系统伪距差分定位的影响 总被引:1,自引:0,他引:1
用计算机仿真方法 ,给出了单频卫星导航系统伪距差分后 ,定位误差受电离层影响的一些结果。伪距差分定位能够校正电离层时延误差 ,但校正精度随用户与基准站到同一颗卫星倾斜因子的不同而不同。为此 ,提出了一种改进的伪距差分方法。仿真结果表明 ,改进后有明显效果 相似文献
279.
280.
介绍了超短波电台自动检测系统与故障诊断系统的功能,并根据功能要求进行了硬件电路的设计,采取面向信号的ATLAS语言进行软件设计和建立在专家知识输入故障推理模型.该系统经使用证明,检测结果精确,检测效率较高. 相似文献