低密度大气中降落伞开伞动载的研究

文章根据建立的降落伞充气过程中轴向和径向动量方程，研究了低密度大气中降落伞的开伞动载。通过计算并与高密度大气中开伞动载的比较，得出了低密度大气中开伞动载的特点。     

"神舟三号"大气成分探测器探测结果--2002年4月磁暴期间大气成分的异常变化

"神州三号"(SZ-3)大气成分探测器搭载在SZ-3留轨舱上于2002年3月26日发射入轨,正遇2002年4月发生的连续两次地磁扰动事件,SZ-3大气成分探测器测得了轨道舱运行高度上(330-350 km附近)大气成分的响应变化和异常现象.探测数据表明,在地磁扰动期间,不仅发生了大气中主要成分O和N2的数密度值增变的响应变化,而且在进入地磁扰动峰期开始后6h左右在较高纬度处出现了N2的异常增变和O的异常降变.4-5h后,这种异常增变峰和降变谷由纬度42°N左右逐渐推移向纬度较低地区,直至消失.     

太阳黑子数及Ap指数周期变化特征的小波分析

应用Morlet小波变换方法从多个变化尺度上对1932—2000年的太阳黑子数及Ap指数的变化特征进行分析．(1)太阳黑子数存在准11年、准32年的周期变化特征及Ap指数存在准32年、准11年、准6个月、准27天和准13．9天的周期变化特征；(2)太阳黑子数及Ap指数有着相似的准11年周期变化，但Ap指数极值的出现要比太阳黑子数极值出现滞后1—2年；(3)Ap指数准27天的周期变化在太阳黑子活动高、低年不同，在太阳活动低年，Ap指数有着较稳定的准27天周期变化，但在太阳活动高年，27天的周期变化几乎消失，这种周期变化的消失和出现时间可在Morlet小波变换图中体现出来。     

可靠性试验中通风冷却剖面的探讨

结合国家军用标准和飞机环控系统的特点对机载电子设备实际使用中的通风冷却条件进行了研究,结合产品的寿命剖面、任务剖面,针对不同任务的环境条件、飞行高度和飞行马赫数等条件,对产品在可靠性试验中通风冷却应力的施加进行了探索性研究,对现行标准中存在的问题进行了对比研究,阐述了在可靠性试验过程中如何模拟其实际使用中的通风冷却条件,制定出合理、可行的通风冷却试验剖面(包括通风气体流量、温度、湿度和洁净度等参数的确定方法).以具体产品为例,通过对产品实际使用中的通风情况进行研究,得出了其可靠性试验中与温度剖面相对应的通风冷却剖面(包括通风气体的参数以及施加的时间).     

三个素数猜想的证明

采用新的构造方法,把不规则分布的素数进行分类,即把单个素数a都同时表示成等距的区间[a,a＋h]（a为任意素数）,在[a,a＋h]中的元素为自然数,将[a,a＋h]中对应位置有相同情况,或都是素数,或都不是素数的为同一等价类,其中每个[a,a＋h]中至少有一个素数a,h取不同自然数时,分类方法不同,显然[a,a＋h]的等价类的个数在h有限时是有限的,小于2h/2。     

Estimation of probability of occurrence of F1 layer or L condition using tables and electron density profile models

An algorithm is proposed for evaluation of the probability of occurrence of an F1 layer or L condition, based on tables. Observations independent of the tables database are used for comparison between the estimated probability of occurrence, the formulation used at present in IRI, and the occurrence actually observed. The importance of the inclusion of L condition in the electron density profile model is shown.     

多元高温合金固溶极限预测

综合考虑了溶质元素与基体元素的原子半径、电负性以及外层电子数的立方根对溶质元素固溶度的影响，推导出二元合金的固溶度定量方程，提出了多元高温合金固溶极限曲线的预测新方法，并将其应用于计算镍基和钴基三元合金相图的γ／（γ＋σ）相界和γ（γ＋μ）相界。结果表明，计算的固溶极限曲线与已知相图的固溶极限曲线较吻合，与Ｍｄ值法计算的相界比较，该方法具有较高的精度。     

Longitudinal behaviors of the IRI-B parameters of the equatorial electron density profiles retrieved from FORMOSAT-3/COSMIC radio occultation measurements

The electron density profiles in the bottomside F₂-layer ionosphere are described by the thickness parameter B0 and the shape parameter B1 in the International Reference Ionosphere (IRI) model. We collected the ionospheric electron density (N_e) profiles from the FORMOSAT-3/COSMIC (F3/C) radio occultation measurements from DoY (day number of year) 194, 2006 to DoY 293, 2008 to investigate the daytime behaviors of IRI-B parameters (B0 and B1) in the equatorial regions. Our fittings confirm that the IRI bottomside profile function can well describe the averaged profiles in the bottomside ionosphere. Analysis of the equatorial electron density profile datasets provides unprecedented detail of the behaviors of B0 and B1 parameters in equatorial regions at low solar activity. The longitudinal averaged B1 has values comparable with IRI-2007 while it shows little seasonal variation. In contrast, the observed B0 presents semiannual variation with maxima in solstice months and minima in equinox months, which is not reproduced by IRI-2007. Moreover, there are complicated longitudinal variations of B0 with patterns varying with seasons. Peaks are distinct in the wave-like longitudinal structure of B0 in equinox months. An outstanding feature is that a stable peak appears around 100°E in four seasons. The significant longitudinal variation of B0 provides challenges for further improving the presentations of the bottomside ionosphere in IRI.     

Near real-time assimilation in IRI of auroral peak E-region density and equatorward boundary

The paper describes the method and initial results of assimilating the auroral peak E-region density (NmE) and the auroral equatorward boundary (EB) into the International Reference Ionosphere (IRI). The NmE and EB are obtained using a FUV based auroral model or FUV measurements in near real-time. Initial results show that the auroral NmE is often significantly larger than the NmE due to the solar EUV. This indicates the importance of including the contribution of precipitating electrons in IRI. The global equatorial boundary helps to improve the specification of the sub-auroral ionosphere trough in IRI. An IDL software package has been developed to interactively display the IRI parameters with assimilated NmE and EB. It can serve as an operational tool for space weather monitoring.     

Study of the 28 October 2003 and 20 January 2005 solar flares by means of 2.223 MeV gamma-emission line

By the data on intensity-time profiles of the neutron capture line of 2.223 MeV we have studied some characteristics of two solar flares, 28 October 2003 and 20 January 2005 (INTEGRAL and CORONAS-F observations, respectively). The SINP code was applied making allowance for the main processes of neutron interactions and deceleration in the solar plasma, character of neutron source, losses of neutrons and density model of the solar atmosphere. Comparison of the computed time profiles of 2.223 MeV line with observed ones for the flare of 28 October 2003 confirms the results obtained earlier for three other flares. Namely, the effect of density enhancement (EDE) in the sub-flare region, as well as the variations (hardening) of accelerated particle spectrum in the course of the event have been confirmed. The usual modeling procedure by the SINP code, however, seems to be inapplicable to the event of 20 January 2005. Possible causes of density enhancements during some flares and peculiarities of the 20 January 2005 flare are discussed.