Asymmetries in Mars' Exosphere

Observations and simulations show that Mars' atmosphere has large seasonal variations. Total atmospheric density can have an order of magnitude latitudinal variation at exobase heights. By numerical simulations we show that these latitude variations in exobase parameters induce asymmetries in the hydrogen exosphere that propagate to large distances from the planet. We show that these asymmetries in the exosphere produce asymmetries in the fluxes of energetic neutral atoms (ENAs) and soft X-rays produced by charge exchange between the solar wind and exospheric hydrogen. This could be an explanation for asymmetries that have been observed in ENA and X-ray fluxes at Mars.     

新古典经济增长理论和二元经济模型的分析与借鉴

本文主要介绍了发展经济学中新古典经济增长理论和二元经济理论，并分析了它们对我国经济发展的适用性问题。据此，对我国的经济发展提出了相关的政策建议。     

中国工业化道路的特征与选择

工业化是各国经济发展中不可逾越的阶段，通过回顾世界各国不同的工业化道路，归纳了世界主要工业化道路的特征和我国工业化道路的特点，分析了在贸易投资自由化、一体化条件下，我国的工业化进程处于两难境地的现状与原因，进而提出我国工业化应选择的产业和采取的产业政策。     

新自由主义的社会福利思想

作为当代社会一个重要的理论范式，新自由主义是在与凯恩斯主义的论战中逐步发展起来的。在政治经济领域内，它拒绝国家的干预和控制；在社会福利领域内，它反对福利思想的传播和福利国家的构建，主张通过自由市场机制和个人的自我负责来取代长期由国家提供的社会福利，借以减轻国家的负担，激发个人的进取精神。在新自由主义思想的指引下，英国和美国分别实施了社会福利改革，短期内在减少社会福利开支的同时，也导致了社会福利水平的下降，从长期看，新自由主义的社会福利政策存在着缺陷。     

Magnetosphere Imaging Instrument (MIMI) on the Cassini Mission to Saturn/Titan

The magnetospheric imaging instrument (MIMI) is a neutral and charged particle detection system on the Cassini orbiter spacecraft designed to perform both global imaging and in-situ measurements to study the overall configuration and dynamics of Saturn’s magnetosphere and its interactions with the solar wind, Saturn’s atmosphere, Titan, and the icy satellites. The processes responsible for Saturn’s aurora will be investigated; a search will be performed for substorms at Saturn; and the origins of magnetospheric hot plasmas will be determined. Further, the Jovian magnetosphere and Io torus will be imaged during Jupiter flyby. The investigative approach is twofold. (1) Perform remote sensing of the magnetospheric energetic (E > 7 keV) ion plasmas by detecting and imaging charge-exchange neutrals, created when magnetospheric ions capture electrons from ambient neutral gas. Such escaping neutrals were detected by the Voyager l spacecraft outside Saturn’s magnetosphere and can be used like photons to form images of the emitting regions, as has been demonstrated at Earth. (2) Determine through in-situ measurements the 3-D particle distribution functions including ion composition and charge states (E > 3 keV/e). The combination of in-situ measurements with global images, together with analysis and interpretation techniques that include direct “forward modeling’’ and deconvolution by tomography, is expected to yield a global assessment of magnetospheric structure and dynamics, including (a) magnetospheric ring currents and hot plasma populations, (b) magnetic field distortions, (c) electric field configuration, (d) particle injection boundaries associated with magnetic storms and substorms, and (e) the connection of the magnetosphere to ionospheric altitudes. Titan and its torus will stand out in energetic neutral images throughout the Cassini orbit, and thus serve as a continuous remote probe of ion flux variations near 20R _S (e.g., magnetopause crossings and substorm plasma injections). The Titan exosphere and its cometary interaction with magnetospheric plasmas will be imaged in detail on each flyby. The three principal sensors of MIMI consists of an ion and neutral camera (INCA), a charge–energy–mass-spectrometer (CHEMS) essentially identical to our instrument flown on the ISTP/Geotail spacecraft, and the low energy magnetospheric measurements system (LEMMS), an advanced design of one of our sensors flown on the Galileo spacecraft. The INCA head is a large geometry factor (G ∼ 2.4 cm² sr) foil time-of-flight (TOF) camera that separately registers the incident direction of either energetic neutral atoms (ENA) or ion species (≥5^∘ full width half maximum) over the range 7 keV/nuc < E < 3 MeV/nuc. CHEMS uses electrostatic deflection, TOF, and energy measurement to determine ion energy, charge state, mass, and 3-D anisotropy in the range 3 ≤ E ≤ 220 keV/e with good (∼0.05 cm² sr) sensitivity. LEMMS is a two-ended telescope that measures ions in the range 0.03 ≤ E ≤ 18 MeV and electrons 0.015 ≤ E≤ 0.884 MeV in the forward direction (G ∼ 0.02 cm² sr), while high energy electrons (0.1–5 MeV) and ions (1.6–160 MeV) are measured from the back direction (G ∼ 0.4 cm² sr). The latter are relevant to inner magnetosphere studies of diffusion processes and satellite microsignatures as well as cosmic ray albedo neutron decay (CRAND). Our analyses of Voyager energetic neutral particle and Lyman-α measurements show that INCA will provide statistically significant global magnetospheric images from a distance of ∼60 R _S every 2–3 h (every ∼10 min from ∼20 R _S). Moreover, during Titan flybys, INCA will provide images of the interaction of the Titan exosphere with the Saturn magnetosphere every 1.5 min. Time resolution for charged particle measurements can be < 0.1 s, which is more than adequate for microsignature studies. Data obtained during Venus-2 flyby and Earth swingby in June and August 1999, respectively, and Jupiter flyby in December 2000 to January 2001 show that the instrument is performing well, has made important and heretofore unobtainable measurements in interplanetary space at Jupiter, and will likely obtain high-quality data throughout each orbit of the Cassini mission at Saturn. Sample data from each of the three sensors during the August 18 Earth swingby are shown, including the first ENA image of part of the ring current obtained by an instrument specifically designed for this purpose. Similarily, measurements in cis-Jovian space include the first detailed charge state determination of Iogenic ions and several ENA images of that planet’s magnetosphere.This revised version was published online in July 2005 with a corrected cover date.     

地市级政府规模影响因素的实证研究——以河南省为例

政府规模是我国推进行政体制改革、简政放权进程中值得关注的一个重大课题,文章以＂利维坦假说＂和＂瓦格纳法则＂为理论基础,利用河南省1990~2012年的地市级面板数据,通过构建静态面板数据模型和动态面板数据模型,从一个更微观的视角考察了地方政府规模的影响因素。研究发现,财政分权推动了地方政府规模的扩大,＂利维坦假说＂并不成立;而经济发展水平、城镇化率与地方政府规模也呈正相关关系,即＂瓦格纳法则＂是成立的;此外,我们还发现人口规模、产业结构和开放程度也是影响地方政府规模的重要因素。     

自适应遥测信道速率的分包遥测调度方案

在卫星分包遥测静态分配适应单一遥测信道的方案基础上,提出了一种改进型动态自适应遥测信道速率的遥测分包方法,将包传输的控制参数由绝对参数优化为相对参数,从而满足不同信道速率、不同包源速率下的包传输适应性.该方法通过将遥测包周期计数与遥测包静态分配的传输周期的比值作为遥测包传输等待迫切比例系数,用相对的传输迫切比例系数值对全部遥测包进行排序,从大到小组入遥测信道下传.通过这种遥测包调度策略解决了遥测信道速率变换对包传输控制的影响.此外通过调节遥测包传输比例系数也能很好地解决遥测包数据率变化对信道传输的适应能力的影响,如数据率增加时整体降低包传输频率、数据率减少时整体加快包传输频率.     

基于中性层偏移的Z型材滚弯成形回弹预测

以提高大截面Z型材四轴滚弯成形精度为目的,通过综合考虑材料属性、几何特征和成形半径等因素对回弹的影响,建立了引入中性层偏移的大截面Z型材弯曲回弹解析模型,研究了7075-O和7475-O铝合金Z型材在不同滚弯成形半径下的回弹规律,并进行滚弯成形实验验证。结果表明,与忽略中性层偏移影响的型材回弹预测经验模型相比,基于中性层偏移的回弹预测模型能够准确预测大截面Z型材的回弹量,在相同的曲率半径下,预测回弹变形的最大相对误差从11.681%减小到3.347%。     

中性盐雾预腐蚀对AF1410高强钢疲劳寿命的影响

采用失重法和XRD法研究了AF1410钢在中性盐雾环境中的耐蚀性能,并对中性盐雾预腐蚀不同时间后的试样进行疲劳性能测试,研究了不同预腐蚀时间对材料疲劳寿命的影响。结果表明:AF1410钢发生了严重的全面腐蚀,腐蚀产物主要由FeO(OH)和Fe3O4组成,并得到其腐蚀失重曲线;疲劳断口形貌分析表明,随预腐蚀时间的延长,腐蚀损伤程度增加,在疲劳加载过程中易形成较多的疲劳裂纹扩展源而导致疲劳断裂失效;最终获得中性盐雾预腐蚀AF1410钢结构疲劳寿命特性以及预腐蚀对疲劳寿命的影响系数C(t)曲线。     

分布式容错系统的低冗余重构策略及拓扑结构研究

分布式系统需要采用合理的拓扑结构，才能在低冗余的条件下的实现容错，从而获得高的性能价格比。本文从分析的可靠性与重构策略的关系以及重构策略与系统拓扑系统入手，找出解决这一课题的一种途径，最后介绍了一个低余度高可靠实时重构的分布式容错系统的实现。