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1.
本文是关于N=31至64位最佳PCM群同步码研究成果的总结报告。这些最佳码是世界上迄今为止(在该范畴内)的最新成果。文中给出了N=31~64位最佳群同步码的码组图样、误同步概率和主要特征参数。此外,还阐述了歧码问题和某些关键理论。 相似文献
2.
Although the elemental composition in all parts of the solar photosphere appears to be the same this is clearly not the case
with the solar upper atmosphere (SUA). Spectroscopic studies show that in the corona elemental composition along solar equatorial
regions is usually different from polar regions; composition in quiet Sun regions is often different from coronal hole and
active region compositions and the transition region composition is frequently different from the coronal composition along
the same line of sight. In the following two issues are discussed. The first involves abundance ratios between the high-FIP
O and Ne and the low-FIP Mg and Fe that are important for meaningful comparisons between photospheric and SUA compositions
and the second involves a review of composition and time variability of SUA plasmas at heights of 1.0≤h≤1.5R
⊙. 相似文献
3.
The fastest pulsar and the slowest nova; the oldest galaxies and the youngest stars; the weirdest life forms and the commonest
dwarfs; the highest energy particles and the lowest energy photons. These were some of the extremes of Astrophysics 2006.
We attempt also to bring you updates on things of which there is currently only one (habitable planets, the Sun, and the Universe)
and others of which there are always many, like meteors and molecules, black holes and binaries. 相似文献
4.
D.R. Japaridze M.Sh. Gigolashvili V.J. Kukhianidze 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2007,40(12):1912-1916
The differential rotation of the patterns of the large-scale solar magnetic field during solar activity cycles 20 and 21 is investigated. Compact magnetic elements with the polarity of the general solar magnetic field have larger speed of rotation than the elements with the opposite polarity. The surface of the Sun was divided by 10°-zones. In all of them the average rotation rate of the magnetic elements with negative polarity is little higher than that of the magnetic elements with positive polarity, except for 50°-zone of the south hemisphere and at the 10° latitude of the north hemisphere.
The rates of differential rotation for large-scale magnetic elements with negative and positive polarities have similar behavior for both cycles of the solar activity.
The rotation rate varies at polarity reversal of the circumpolar magnetic fields. For the cycle No 20 in 1969–1970 the threefold reversal took place in the northern hemisphere and variations of rotation rate can be noticed for magnetic elements both with positive and negative polarity for each 10°-zone in the same hemisphere. 相似文献
5.
Large amplitude MHD waves are commonly found in the solar wind. Nonlinear interactions between the MHD waves are likely to
produce finite correlation among the wave phases. For discussions of various transport processes of energetic particles, it
is fundamentally important to determine whether the wave phases are randomly distributed (as assumed in quasi-linear theories)
or they have a finite coherence. Using a method based on a surrogate data technique and a fractal analysis, we analyzed Geotail
magnetic field data (provided by S. Kokubun and T. Nagai through DARTS at the Institute of Space and Astronautical Science)
to evaluate the phase coherence among the MHD waves in the earth's foreshock region. The correlation of wave phases does exist,
indicating that the nonlinear interactions between the waves is in progress.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
6.
7.
论述利用计算机对气象卫星数字基带信号解码的两种方法。方法一是在开环条件下对基带采样跟踪与智能判决。方法二是基于最优检测原理 ,在分相码 (Manchester码 )的解码中简化了正交积分锁相环 ,采用单积分器辅助计算机智能判断 ,对基带实现最优检测 相似文献
8.
李伟红 《华北航天工业学院学报》2002,12(4):17-19
本文介绍了多线程网络编程的实现。并给出了用Visual C 6.0实现的一个多线程端口扫描程序的关键代码。 相似文献
9.
FY-2气象卫星在轨管理工程测控关键技术(上) 总被引:1,自引:2,他引:1
介绍了风云二号(FY—2)地球静止轨道自旋气象卫星工程测控的关键技术。分析了位置保持、姿态确定、星蚀和日凌的原理,给出了位置保持、姿态控制策略和地影、月影、日凌预报算法。并提出了一种检验定姿结果正确性的方法,提供了相应的工程计算参数。这些策略都已成功地用于FY—2卫星的在轨管理工程测控。 相似文献
10.
本文给出了用于ZN3火箭姿态测量太阳角计的原理和测量结果,讨论了背景抑制和标定方法,分析了误差来源。该仪器采用选取适当探测波段和比值测量方法较好地消除了地外太阳辐照和大气消光的影响,也有效地抑制了背景辐射的干扰,大大提高了测量精度。实测结果表明,火箭姿态角测量的均方根误差约为0.7°。这一方法适用于各种自旋稳定飞行器的姿态测量。 相似文献