地磁Ap指数滞后太阳周循环分析

把1932-2006年地磁Ap指数12个月流动均值分解成为(Ap)R和(Ap)I.其中(Ap)R为太阳黑子数R的线性函数,与太阳黑子数R相位相同,可能对应于日冕物质抛射(CME)等地磁控制因素. (Ap)I分量与太阳黑子数R相位相差约180°,该分量可能对应于极冕洞变化(从太阳峰年开始,由日面极区逐渐向赤道延伸).以地磁Ap指数与太阳黑子数R滞后非常严重的第20太阳周为例,证实了(Ap)I分量与极冕洞向赤道延伸循环变化相对应.因此极冕洞循环变化可能是导致地磁扰动指数与太阳周循环相位不一致,出现滞后现象的一个十分重要原因.      

惯导平台式重力测量技术实现及应用

详细阐述了解析方位双轴惯导平台式重力测量的工作原理,并通过基于方位余弦积的惯导力学编排解决了极区工作问题。在常规平台式重力测量数据处理方法的基础上,针对高动态环境提出了基于Kalman滤波的运动扰动修正方法。在此基础上研制了ZL11-1A型国产惯导平台式海洋重力仪。通过与国外主流重力仪产品海上同船作业比对,结果表明,该型重力仪在高海况下测量精度依然优于1mGal,满足重力测量作业要求。     

太阳电池阵极月轨道在轨热分析

以极月轨道上太阳电池阵作为研究对象,详细分析了该轨道上电池阵所得各外热流的确定方法.以此为基础,对太阳电池阵进行在轨温度数值模拟,得到月球轨道上电池阵所得外热流以及温度的周期分布.计算结果与地球卫星的相应数据进行比较,明确了月球轨道上电池阵所得外热流以及温度的周期分布特点,为月球卫星上太阳电池阵以及整个卫星的设计提供了有利的数据参考.      

A steady-state model for the D- to F-region of the polar cap

For obvious reasons the ionosphere of the polar cap, surrounded by the auroral zone, is only poorly investigated. Even ionosonde data are very scant from geomagnetic latitudes beyond 70°. Since 1997 the European incoherent scatter radar facility EISCAT has an additional installation on Svalbard and has been providing electron density data nearly continuously ever since. These measurements which mainly cover the E- and F-regions are supplemented by rocket data from Heiss Island at a comparable magnetic latitude; these data are more sporadic, but cover lower altitudes and densities. A provisional, steady-state, neural network-based model is presented which uses the data of both sites.     

夏热冬冷地区居住建筑节能设计分析

推动建筑向节能、绿色、智能化方向发展,是国际建筑界实践可持续发展理念的大趋势,也是中国经济社会发展面临的重要任务。我国居住建筑节能,从八十年代初起步,从全国总体情况看,节能标准在北方地区推行较早,近一两年来,我省尤其是南昌市的节能标准执行力度正在不断加大。本文通过对冬冷夏热地区一栋宿舍建筑实例进行节能设计分析,得出冬冷夏热地区"宿舍"建筑节能设计外维护结构的一般设计标准。     

高温铝合金电磁超声检测回波特性及因素分析

针对高温铝合金在线检测条件下,温度对铝合金电磁超声检测回波特性的影响规律尚不明确、高温检测时缺陷定量/定位补偿困难这一难题,以螺旋线圈电磁超声换能器（EMAT）为例,建立了高温铝合金EMAT检测过程的场路耦合有限元模型;研究了温度对EMAT激励/接收换能效率、EMAT激励/接收电路的功率分配特性、超声传播过程中的扩散/介质衰减特性、回波幅值和超声声速等因素的影响规律;研制了耐高温EMAT探头,对20~500℃高温铝合金试样进行了检测实验,并测定了高温铝合金的超声介质衰减系数和超声声速。在仿真和实验相结合的基础上,分析了高温检测时超声回波幅值变化特性及其影响因素。结果表明：对于铝合金这类非铁磁性金属材料,导致高温时超声回波幅值下降的主要原因是超声介质衰减系数随着温度的升高而增大,其次为高温时EMAT激励/接收电路的功率分配特性的改变。在激励EMAT在试样表面形成的洛伦兹力不变的条件下,其所激励的超声波回波幅值具有随着温度的增加而增加的特点,可以有效减缓超声回波幅值下降的趋势。     

Are small-scale field-aligned currents and magnetosheath-like particle precipitation signatures of the same low-altitude cusp?

We examined some 75 observations from the low-altitude Earth orbiting DMSP, Ørsted and CHAMP satellites which were taken in the region of the nominal cusp. Our objective was to determine whether the actually observed cusp locations as inferred from magnetosheath-like particle precipitation (“particle cusp”) and intense small-scale magnetic field variations (“current cusp”), respectively, were identical and were consistent with the statistically expected latitude of the cusp derived from a huge number of charged particle spectrograms (“statistical cusp”).     

The hydroxyl radical as an indicator of SEP fluxes in the high-latitude terrestrial atmosphere

The low background values at nighttime of the mesospheric hydroxyl (OH) radical make it easier to single out the atmospheric response to the external solar forcing in Polar Regions. Because of the short lifetime of HO_x, it is possible to follow the trails of Solar Energetic Particle (SEP) events in the terrestrial atmosphere, as shown by Storini and Damiani (2008). The sensitivity of this indicator makes discernible not only extreme particle events with a flux peak of several thousand pfu [1 pfu = 1 particle/(cm² s sr)] at energies >10 MeV, but also those with lower flux up to about 300 pfu. Using data from the Microwave Limb Sounder (MLS) on board the EOS AURA satellite, we examined the correlation of OH abundance vs. solar proton flux for almost all the identified SEP events spanning from November 2004 to December 2006 (later on no more SEP events occurred during Solar Cycle no. 23). The channels at energies greater than 5 MeV and 10 MeV showed the best correlation values (r ∼ 0.90–0.95) at altitudes around 65–75 km whereas, as expected, the most energetic channels were most highly correlated at lower altitudes. Therefore, it is reasonably possible to estimate the solar proton flux from values of mesospheric OH (and viceversa) and it could be useful in studying periods with gaps in the records of solar particles.     

在地球极区无奇异的再入飞行器质心运动方程

传统的再入飞行器质心运动方程用经度和纬度描述地理位置，在南北极极点处奇异，在南北极区病态。本文提出利用位置矢量的三个方向余弦，称为“三余弦数”或“三元数”，代替经纬度，推导出无奇异再入质心运动方程。再入飞行器临近极点和到达极点的算例显示，使用三元数的无奇异再入方程完全避免了传统方程有关极点的奇异性。同时，无奇异方程所选状态变量与传统方程可进行很简便的转换。     

格序群的极子群在凸l－子群格中生成的闭子格

设Ｇ是一个格序群，Ｐ（Ｇ）是Ｇ的极子群集合，Ｃ（Ｇ）是Ｇ的凸ｌ－子群集合，Ω（Ｇ）是Ｐ（Ｇ）在Ｃ（Ｇ）中生成的闭子格，本文通过对Ω（Ｇ）的研究得到了一系列重要结果，对有限值格序群给予了一系列新的刻画，证明了ｇ是基元当且仅当ｇ－是ｇ的唯一的Ω－值等结论，实际上对Ｐ．Ｃｏｎｒａｄ提出的问题＂Ｄｅｓｃｒｉｂｅｔｈｅｅｌｅｍｅｎｔｓｉｎ＂进行了富有意义的探索。