New flare model using recent measurements of the solar ultraviolet irradiance

The solar photon output from the Sun, which was once thought to be constant, varies considerably over time scales from seconds during solar flares to years due to the solar cycle. This is especially true in the wavelengths shorter than 190 nm. These variations cause significant deviations in the Earth and space environment on similar time scales, which then affects many things including satellite drag, radio communications, atmospheric densities and composition of particular atoms, molecules, and ions of Earth and other planets, as well as the accuracy in the Global Positioning System (GPS). The Flare Irradiance Spectral Model (FISM) is an empirical model that estimates the solar irradiance at wavelengths from 0.1 to 190 nm at 1 nm resolution with a time cadence of 60 s. This is a high enough temporal resolution to model variations due to solar flares, for which few accurate measurements at these wavelengths exist. This model also captures variations on the longer time scales of solar rotation (days) and solar cycle (years). Daily average proxies used are the 0–4 nm irradiance, the Mg II c/w, F10.7, as well as the 1 nm bins centered at 30.5 nm, 121.5 (Lyman Alpha), and 36.5 nm. The GOES 0.1–0.8 nm irradiance is used as the flare proxy. The FISM algorithms are given, and results and comparisons are shown that demonstrate the FISM estimations agree within the stated uncertainties to the various measurements of the solar Vacuum Ultraviolet (VUV) irradiance.     

Geomagnetic effects on mid-latitude railways: A statistical study of anomalies in the operation of signaling and train control equipment on the East-Siberian Railway

Intense geomagnetically induced currents (GIC) can hamper rail traffic by disturbing signaling and train control systems. GIC threats have been a concern for technological systems at high-latitude locations due to geomagnetic disturbances driven by substorm expansion electrojet or convection electrojet intensifications. However, other geomagnetic storm processes such as storm sudden commencement (SSC) and geomagnetic pulsations can also cause GIC concerns for technological systems. We present in this paper the first evidence based on statistical data for links between geomagnetic disturbances and faulty operations (anomalies) in the functioning of railway automatics and telemetry. We analyze anomalies of automatic signaling and train control equipment which occurred in 2004 on the East-Siberian Railway (corrected geomagnetic latitude _m = 46–51°N and longitude λ_m = 168–187°E). Our results reveal a seasonal effect in the number of anomalies per train similar to the one observed in geomagnetic activity (Kp, Ap, Dst indices). We also found an increase by a factor of 3 in the total duration of daily anomalies during intense geomagnetic storms (local geomagnetic index specific to Siberian Observatory A_max > 30), with a significant correlation between the daily sum of durations of anomalies with geomagnetic activity. Special attention was paid to failures not related to recognized technical malfunctions. We found that the probability of these failures occurring in geomagnetically disturbed periods was 5–7 times higher than the average anomaly occurrence.     

Dark matter search with the CALET detector on-board ISS

The CALorimetric Electron Telescope, CALET, mission is proposed for the observation of high-energy electrons and gamma-rays at the Exposed Facility of the Japanese Experiment Module on the International Space Station. The CALET has a capability to observe the electrons (without separation between e⁺ and e⁻) in 1 GeV–10 TeV and the gamma-rays in 20 MeV–several TeV with a high-energy resolution of 2% at 100 GeV, a good angular resolution of 0.06 degree at 100 GeV, and a high proton-rejection power of nearly 10⁶. The CALET has a geometrical factor of 1 m²sr, and the observation period is expected for more than three years. The very precise measurement of electrons enables us to detect a distinctive feature in the energy spectrum caused from WIMP dark matter in the Galactic halo. The excellent energy resolution of CALET, which is much better than GLAST or air Cherenkov telescopes over 10 GeV, enables us to detect gamma-ray lines in the sub-TeV region from WIMP dark matter annihilations. The CALET has, therefore, a unique capability to search for WIMP dark matter by the hybrid observations of electrons and gamma-rays.     

空间碎片超高速撞击动力学建模与数值仿真技术

阐明了空间碎片超高速撞击数值仿真技术研究的目的、意义和国内外发展状况 ;重点论述了空间碎片超高速撞击数值仿真技术的主要研究内容、技术指标和具体实施途径 ,从而为研究的深入开展提供了技术依据和指导原则     

中国载人航天工程的外部设计

在“神舟号”载人飞船工程实现了中国人往返于天地间的目的之后 ,中国应审慎地选择发展载人航天的目标。文章从中国社会对载人航天的需求出发 ,讨论了以开发利用空间微重力物质环境为目标的空间站和以发展天基航天为目标的天基航天站的外部工程系统的环境条件 ,认为中国在运载火箭、发射和回收场、测控站网方面已有较好基础 ,基本具备条件 ,运人运输器已有“神舟号”载人飞船 ,运物运输器的研制也不困难 ,但在为保障航天员在空间生活、工作的航天员系统方面和为实现载人航天工程功能和显现价值的有效载荷系统方面欠缺较多 ,需要一个研究、试验、培训和开发、演示的发展阶段     

利用频谱分析确定空间目标太阳翼定向模式

分析对比了空间目标与可控飞行器轨道确定的不同,论述了太阳翼定向模式的不同对轨道运动特性的影响。通过地面站的测距与测角数据,推算出测量数据的地心距频谱。假定一种太阳翼定向模式,利用测量数据进行轨道确定,利用定轨数据计算地心距频谱并与测量数据的频谱比对,由此可确定太阳翼定向模式。利用数值仿真对近地太阳同步轨道和地球静止轨道两种情况进行了验证,仿真结果表明该思路和方法是有效的。     

返回舱和着陆系统设计的新理念

文章描述了美俄合作提出的一种低成本和低风险的载人返回舱概念。方案采用已有的硬件 和技术,由美国负责电子设备和软件,充分利用俄罗斯在返回舱方面的技术和低成本。提出的这种返回舱 概念是把联盟-TM按比例增大到可以容纳8位乘员,而且着陆系统增加了气囊,对伤病航天员的着陆具有 更好的缓冲作用。     

FY—1C卫星空间粒子成分监测器及其探测结果

简要介绍了FY－1C星空间粒子成分监测器的任务目标、工作原理、创新特色及在轨探测结果。空间粒子成分监测器用于卫星轨道空间的带电粒子辐射监测，为卫星的在轨安全和抗辐射加固设计服务。监测器在世界上实现用1套传感器完成对高能电子、质子、α粒子至铁离子的全成分监测，使我国首次获得了870km高太阳同步轨道全空间的各种重离子分布、质子能谱分布和电子通量分布，捕捉到大量的地磁暴和太阳质子事件，获得了批重要的探测成果。     

GPS用于航天器交会对接的方案与模糊度OTF解算研究

设计了GPS相对导航在航天器交会对接中应用的两种方案 ;认为在交会对接相对导航的过程中 ,可以进行载波相位模糊度的OTF解算 ,以直接利用高精度的载波相位观测量 ,提高交会对接测量的精度。通过实算 ,对结论进行了验证。     

载人航天器真空热试验技术探讨

文章介绍了载人航天器真空环境下热平衡试验的必要性,热真空试验的特点、试验目的和试验项目,以及美国载人航天的热真空试验技术,特别是载人航天活动对热真空试验的特殊要求等。