基于BP神经网络的GNSS-R海面风速反演

针对GNSS-R进行海面风速反演过程中时频域相关物理量较多，数据耦合性强等问题，提出了基于反向传播（BP）神经网络反演海面风速的方法。建立反演过程中相关观测量与风速的对应关系，选取多观测量作为输入，对输入数据进行处理，设置神经元与激励函数，使用BP神经网络自适应调整拟合参数，将风速作为神经网络输出端的特征量提取。反演结果，风速≤ 20 m/s时，反演均方根误差RMSE=1.21 m/s，风速>20 m/s时反演均方根误差RMSE=2.54 m/s，反演结果优于使用时延相关曲线前沿斜率（LES）和时延多普勒相关功率均值（DDMA）方法得到的反演结果，且迭代次数较少，复杂度较低，证明该方法可以应用于GNSS-R海面风速反演。     

航电系统并行检测过程与检测设备解耦方法

航电系统在使用或升级改造过程中进行可靠性检测是必不可少的。特别是在当前批量航电系统大量投入使用的背景下，迫切需要能高效、快速、准确地对系统进行可靠性检测。由于航电系统安全性要求高，内置检测软件受限，需要外置检测设备通过航电系统指定接口进行检测，检测过程也不允许出现任何泄露等行为。检测设备与具体航电系统耦合，检测过程与具体检测设备耦合，难以实现批量航电系统并行检测。为此，通过引入逻辑检测设备，给出了一种航电系统并行检测分层框架，解决检测设备与被测系统耦合的问题，同时也保证了检测的安全性。通过逻辑检测设备、检测跳转机和被测主机上检测行为的描述，给出了一种面向通用航电系统并行检测的检测设备协同机制，解决检测过程与检测设备耦合的问题，从而支持多个航电系统并行检测。最后，实现了一个通用航电系统并行检测系统，并通过实际应用和实验对比验证所提方法的有效性。     

Study of the 27-day variations of the galactic cosmic ray intensity and anisotropy

We demonstrate that the general features of the radial and azimuthal components of the anisotropy of galactic cosmic rays can be studied by the harmonic analysis method using data from an individual neutron monitor with cut off rigidity <5 GV. In particular, we study the characteristics of the 27-day (solar rotation period) variations of the galactic cosmic ray intensity and anisotropy, solar wind velocity, interplanetary magnetic field strength and sunspot number. The amplitudes of the 27-day variations of the galactic cosmic ray anisotropy are greater, and the phases more clearly established, in A > 0 polarity periods than in A < 0 polarity periods at times of minimum solar activity. The phases of the 27-day variations of the galactic cosmic rays intensity and anisotropy are opposite with respect to the similar changes of the solar wind velocity in A > 0 polarity periods. No significant dependence of the amplitude of the 27-day variation of the galactic cosmic ray anisotropy on the tilt angle of the heliospheric neutral sheet is found. Daily epicyclegrams obtained by Chree’s method show that the 27-day variations of the galactic cosmic ray anisotropy during A > 0 polarity periods follow elliptical paths with the major axes oriented approximately along the interplanetary magnetic field. The paths are more irregular during A < 0 polarity periods.     

高职语文课程的生存现状及问题分析

受功利主义教育价值观影响，高职语文日益被边缘化。各高校在高职语文课程目标着眼点上认识还很不一致；教材中心现象突出；教学实践模式化，缺乏创新和发展。     

夹具质量对标准测力仪的影响

分析了用试验机进行力学性能检定过程中，夹具的质量对标准测力仪造成的影响，并通过分析原因，给出消除或减小这种影响的方法。     

非营利组织参与农村公共产品供给的制约因素研究

在农村公共产品供给多元化的格局下,鼓励非营利组织参与农村公共产品的供给是一种多赢。但现实语境下,非营利组织参与农村公共产品的供给,还存在着组织自身缺陷、经济实力不足、与非营利组织相关的农村公共产品准入机制还不完善,法制还不健全,供给缺少科学合理的决策和激励机制等因素的制约。本文认为,政府组织有必要监管并引导好非营利组织健康稳定发展,并给予必要的帮助与支持,完善相关法律制度建设,建立科学合理的农村公共产品决策和管理制度等,以化解这些制约因素,改善新时期农村公共产品的有效供给。     

Intermediate-term periodicities in relativistic solar electron fluences during solar cycles 22 and 23

In this paper, we have investigated the intermediate-term periodicities of the relativistic (E > 10 MeV) solar electron flares measured by IMP-8 satellite of NASA for the time period of 1986–2001. This period of investigation includes the entire solar cycle 22; ascending, maximum and a part of descending phase of the current solar cycle 23. To determine accurately the occurrence rate of electron flux, we have employed three different spectral decomposition techniques, viz. fast Fourier transformation (FFT); maximum entropy method (MEM) and Lomb–Scargle periodogram analysis method. For solar cycle 22, in the low frequency range, power spectrum analysis exhibits statistically significant periodicities at ∼706, ∼504 and ∼392 days. In the intermediate frequency range, we have found a series of significant periodicities ∼294, ∼221, ∼153, ∼86, ∼73 and ∼66 days. For short term, periodicities of ∼21–23, ∼31 and ∼37 days were found in power spectrum. When solar cycle 23 is considered the significant periodicities are ∼20, ∼23, ∼29, ∼39, ∼54, ∼63, ∼118, ∼133 and ∼154 days. These results provide evidence that the best known Rieger period (∼153 days), appeared in the high energetic electron flux data for cycle 22 and also likely during maxima of cycle 23. The existence of these periodicities has been discussed in the light of earlier results.     

Seasonal variations of GPS derived TEC at three different latitudes of the southern hemisphere during geomagnetic storms

Data from the archive of the International GNSS Services (IGS) were used to study the seasonal variations of Total Electron Content (TEC) over three stations located at different latitudes in the southern hemisphere during the geomagnetic storms of 11 January, 6 April, 8 June, and 13 October 2000, representing storms that occurred in summer, autumn equinox, winter and spring equinox, respectively. The percentage TEC deviation with respect to reference values differs substantially from season to season. A strong seasonal anomaly and clear equinoctial asymmetry in TEC response to the storms were observed. Weak and short-lived positive TEC deviations as well as strong and long-lasting negative trends were observed in summer storm during the main and recovery phases respectively over the high and low latitudes whereas in winter storm, the highest positive TEC deviations was recorded during the main phase over the entire latitudes. TEC enhancement dominated all the stations during the autumn (March) equinox storm while TEC depletion was majorly observed during the spring (September) equinox. All these variations find their explanations in the thermospheric composition change and circulation. Future work with direct or modeled measurement of atomic Oxygen to molecular Nitrogen ratio (O/N₂), large number of storms and other possible factors such as variations in storm’s intensity and local time dependence of the storm onset is expected to validate the observations in this study.     

我国货币需求函数的影响因素——基于1992—2012年的数据

依据货币需求理论，采用1992～2012年的数据进行整理和计量分析，构建合理的货币需求模型，分析货币需求量与国内生产总值、利率、汇率、外汇储备等变量之间的因果关系，并对变量进行格兰杰因果关系检验，发现狭义货币量、广义货币量与各因素的因果关系并不完全一致。根据实证研究结果，解释了各变量对货币需求量的影响并对货币政策的实施提出建议。     

航空电子企业中数据挖掘技术的应用

以Oracle数据库为源头在微软SQL Server Analysis Services平台上通过建立数据挖掘模型并在航空电子企业中得到实践与应用。