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101.
102.
提出一种采用数字处理的时延测试方法,用于对导航卫星导航信号发射通道分数码片时延的精确测量。该方法是通过高速A/D(模/数)转换器,对导航卫星下行的BPSK(二进制相移键控)信号和卫星导航秒脉冲进行双通道采样,读取采样数据并进行数据处理。根据秒脉冲信号触发门限上升沿确定时延测量起点,对BPSK采样数据进行平方律检波,获取码片换相点,计算换相点和秒脉冲之间的分数码片时延,并进行滤波器时延校准,从而得到导航卫星发射链路的分数码片时延,该方法不需要进行伪随机信号的捕获和跟踪,测量精度主要取决于采样器采样率。通过在测试中使用一根校准电缆对该方法进行验证,验证结果表明,采用本文提出测试方法的测量误差优于0.3ns。 相似文献
103.
对极小展弦比背鳍进行了风洞实验和CFD分析。研究表明:亚声速大迎角下背鳍涡破裂影响不严重,且涡破裂迎角较大;正侧滑通常使背鳍法向力增加,负侧滑使法向力降低;CFD分析证实了大负侧滑条件下翼片法向力会变成负值,从而引起十字翼在倾斜条件下滚转力矩发生突变。 相似文献
104.
105.
Statistical study of radio drifting pulsation structures with associated CMEs and other observations
Chengming Tan Y.H. Yan Y.Y. Liu Q.J. Fu S.J. Wang H.R. Ji Z.J. Chen H.R. Jing 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(6):969-975
Solar radio burst, especially the fine structures (FSs) and the drifting pulsation structures (DPSs), may be used as an important diagnostics tool to draw the evolution map of the flare loop in the initial phase of solar flares. In this work, 52 radio events were found accompanying with DPSs. They were all observed with the Solar Radio Spectrometers (0.625–7.6 GHz) of China during 1998–2004. Combining the radio observations with LASCO-C2, Goes-8 SXR, Hα, EUV and Trace observations, we analyzed all these events and obtained some statistic conclusions: First, 88% DPSs take place at the initial phase of the radio burst, and their rich spectrum characteristics are helpful to understand the events further. Second, 83% DPSs are associated with CMEs or ejection events, and all the events are accompanied by Goes SXR flare. Third, for CMEs and DPSs, which take the first step, there is no significant predominance of either of them. The relationship between the DPSs and CMEs is still not clear in this study because of the lack of spatial resolution in the centimeter–decimeter band. However, the EIT or Trace ejection happened during the onset/end time of DPSs. They are signatures of the initial phase of CMEs. Two events will be illustrated to explain this. 相似文献
106.
K. Shibasaki T. Takano S. Enome H. Nakajima M. Nishio Y. Hanaoka C. Torii H. Sekiguchi T. Bushimata S. Kawashima N. Shinohara H. Koshiishi Y. Shiomi 《Space Science Reviews》1994,68(1-4):217-224
The early phases of three flares, observed by the Nobeyama Radio Heliograph, are studied. Nonthermal and thermal radio sources are identified by comparison with soft X-ray images taken by the Soft X-ray Telescope onboard the Yohkoh satellite. Two of the flares are mainly of nonthermal origin and their location coincides with one of the footpoints of soft X-ray loops. Another flare has both thermal and nonthermal components which start to brighten simultaneously. This suggests that particle acceleration and plasma compression develop simultaneously. 相似文献
107.
A. J. Kliore J. D. Anderson J. W. Armstrong S. W. Asmar C. L. Hamilton N. J. Rappaport H. D. Wahlquist R. Ambrosini F. M. Flasar R. G. French L. Iess E. A. Marouf A. F. Nagy 《Space Science Reviews》2004,115(1-4):1-70
Cassini radio science investigations will be conducted both during the cruise (gravitational wave and conjunction experiments) and the Saturnian tour of the mission (atmospheric and ionospheric occultations, ring occultations, determinations of masses and gravity fields). New technologies in the construction of the instrument, which consists of a portion on-board the spacecraft and another portion on the ground, including the use of the Ka-band signal in addition to that of the S- and X-bands, open opportunities for important discoveries in each of the above scientific areas, due to increased accuracy, resolution, sensitivity, and dynamic range.This revised version was published online in July 2005 with a corrected cover date. 相似文献
108.
109.
根据传统机翼气动外形设计的方案,结合CAD与CFD软件,本文提出了一套机翼气动外形设计流程,包括翼型选择、机翼平面参数确定、建立三维机翼外形模型、流场网格划分和典型飞行条件下的气动计算等多个部分。依据该流程,完成了一个满足设计指标的无人机大展弦比机翼外形的设计,充分说明了该机翼气动外形设计流程的技术可行性。 相似文献
110.
I.A. Nesterov V.E. Kunitsyn 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
We discuss the specific features of the spatiotemporal radio tomography of ionospheric electron density based on the data from high orbiting global navigational satellite system (GNSS). The main peculiarities are four-dimensionality of the problem and essential incompleteness of input data. The approach suggested for the solution of this problem is based on the search for the solution with minimal Sobolev’s norm (the most smooth solution), which provides, in particular, smooth extension of the solution to the area where no input data is available. Methods and algorithms for the solution of the problem are developed, and the resolution of the proposed technique is estimated. Examples of global and regional radio tomographic imaging based on GNSS data are presented. The obtained results are compared with the data of ionosondes and with the results of radio tomography based on the radio transmissions from low-orbiting satellites. 相似文献