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261.
刑事评议程序是介于庭审程序和宣告程序之间的一个重要程序,它既是庭审的自然延续,又是裁判结论形成的前提和基础.然而,欲保证刑事评议程序的正常运行,刑事评议主体之独立必须得到保证;刑事评议之客体还应被全面考虑,并对其进行细化,以确保刑事评议的针对性和有效性,防止出现"估堆"现象.本文以域外刑事评议程序为对象,从评议的主体、客体等角度进行梳理,得出规律性的认识,以期对我国关于刑事评议的立法有所裨益.  相似文献   
262.
Unpublished reports have suggested that hydroxycobalamin (B12, i.m.) prevents motion sickness. Some biomedical evidence supports this contention in that B12 influences the metabolism of histidine and choline; dietary precursors to neurotransmitters with established roles in motion sickness. Susceptibility to motion sickness was evaluated after B12 (1000 micrograms, i.m.). Subjects initially completed vestibular function and motion sickness susceptibility tests to establish normal vestibular function. The experimental motion stressor was a modified coriolis sickness susceptibility test. Subjects executed standardized head movements at successively higher RPM until a malaise III endpoint was reached. Following two baseline tests with this motion stressor, subjects received a B12 injection, a second injection two weeks later, and a final motion sickness test three weeks later. No significant differences in susceptibility were noted after B12. Hematological parameters revealed no B12 deficiency before injection. The possibility that patients with B12 deficiencies are more susceptible to motion sickness cannot be ruled out.  相似文献   
263.
根据机场水泥混凝土道面板厚度、混凝土抗弯拉强度、混凝土抗弯拉弹性模量以及地基反应模量的概率分布和变异特性建立了PCN显式计算公式。分析了道面结构参数的变异性对PCN的影响,提出了基于可靠性理论的PCN通报方法。  相似文献   
264.
In long term space flight, the mechanical forces applied to the skeleton are substantially reduced and are altered in character. This reduced skeletal loading results in a reduction in bone mass. Exercise techniques currently used in space can maintain muscle mass but the mechanical stimulus provided by this exercise does not prevent bone loss. By applying an external impulsive load for a short period each day, which is intended to mimic the heel strike transient, to the lower limb of an astronaut during a long term space flight (5 months), this study tests the hypothesis that the bone cells can be activated by an appropriate external mechanical stimulus to maintain bone mass throughout prolonged periods of weightlessness. A mechanical loading device was developed to produce a loading of the os-calcis similar to that observed during the heel strike transient. The device is activated by the astronaut to provide a transient load to the heel of one leg whilst providing an equivalent exercising load to the other leg. During the EUROMIR95 mission on the MIR space station, an astronaut used this device for a short period daily throughout the duration of the mission. Pre- and post-flight measurements of bone mineral density (BMD) of the os-calcis and femoral neck of the astronaut were made to determine the efficacy of the device in preventing loss of bone mineral during the mission. On the os-calcis which received the mechanical stimulus, BMD was maintained throughout the period of the flight, while it was reduced by up to 7% on the os-calcis which received no stimulus. Post-flight, BMD in both the stimulated and non-stimulated os-calcis reduces, the extent of this reduction however is less in the stimulated os-calcis. For the femoral neck, the mechanical stimulation does not produce a positive effect.  相似文献   
265.
    
The changing view of planets orbiting low mass stars, M stars, as potentially hospitable worlds for life and its remote detection was motivated by several factors, including the demonstration of viable atmospheres and oceans on tidally locked planets, normal incidence of dust disks, including debris disks, detection of planets with masses in the 5-20 M() range, and predictions of unusually strong spectral biosignatures. We present a critical discussion of M star properties that are relevant for the long- and short-term thermal, dynamical, geological, and environmental stability of conventional liquid water habitable zone (HZ) M star planets, and the advantages and disadvantages of M stars as targets in searches for terrestrial HZ planets using various detection techniques. Biological viability seems supported by unmatched very long-term stability conferred by tidal locking, small HZ size, an apparent short-fall of gas giant planet perturbers, immunity to large astrosphere compressions, and several other factors, assuming incidence and evolutionary rate of life benefit from lack of variability. Tectonic regulation of climate and dynamo generation of a protective magnetic field, especially for a planet in synchronous rotation, are important unresolved questions that must await improved geodynamic models, though they both probably impose constraints on the planet mass. M star HZ terrestrial planets must survive a number of early trials in order to enjoy their many Gyr of stability. Their formation may be jeopardized by an insufficient initial disk supply of solids, resulting in the formation of objects too small and/or dry for habitability. The small empirical gas giant fraction for M stars reduces the risk of formation suppression or orbit disruption from either migrating or nonmigrating giant planets, but effects of perturbations from lower mass planets in these systems are uncertain. During the first approximately 1 Gyr, atmospheric retention is at peril because of intense and frequent stellar flares and sporadic energetic particle events, and impact erosion, both enhanced, the former dramatically, for M star HZ semimajor axes. Loss of atmosphere by interactions with energetic particles is likely unless the planetary magnetic moment is sufficiently large. For the smallest stellar masses a period of high planetary surface temperature, while the parent star approaches the main sequence, must be endured. The formation and retention of a thick atmosphere and a strong magnetic field as buffers for a sufficiently massive planet emerge as prerequisites for an M star planet to enter a long period of stability with its habitability intact. However, the star will then be subjected to short-term fluctuations with consequences including frequent unpredictable variation in atmospheric chemistry and surficial radiation field. After a review of evidence concerning disks and planets associated with M stars, we evaluate M stars as targets for future HZ planet search programs. Strong advantages of M stars for most approaches to HZ detection are offset by their faintness, leading to severe constraints due to accessible sample size, stellar crowding (transits), or angular size of the HZ (direct imaging). Gravitational lensing is unlikely to detect HZ M star planets because the HZ size decreases with mass faster than the Einstein ring size to which the method is sensitive. M star Earth-twin planets are predicted to exhibit surprisingly strong bands of nitrous oxide, methyl chloride, and methane, and work on signatures for other climate categories is summarized. The rest of the paper is devoted to an examination of evidence and implications of the unusual radiation and particle environments for atmospheric chemistry and surface radiation doses, and is summarized in the Synopsis. We conclude that attempts at remote sensing of biosignatures and nonbiological markers from M star planets are important, not as tests of any quantitative theories or rational arguments, but instead because they offer an inspection of the residues from a Gyr-long biochemistry experiment in the presence of extreme environmental fluctuations. A detection or repeated nondetections could provide a unique opportunity to partially answer a fundamental and recurrent question about the relation between stability and complexity, one that is not addressed by remote detection from a planet orbiting a solar-like star, and can only be studied on Earth using restricted microbial systems in serial evolution experiments or in artificial life simulations. This proposal requires a planet that has retained its atmosphere and a water supply. The discussion given here suggests that observations of M star exoplanets can decide this latter question with only slight modifications to plans already in place for direct imaging terrestrial exoplanet missions.  相似文献   
266.
针对以往雷达网抗干扰效能评估不具有直观性、脱离战场地形环境的缺点,设计了一种基于GIS的雷达网抗干扰效能评估系统,实现了可视化的雷达网抗干扰效能评估。仿真应用表明,此系统具有较高的推广和实际应用价值。  相似文献   
267.
临近空间高超声速飞行器在高空长时间飞行,受气流加热影响,飞行器表面温度显著升高,依赖地面试验和传统DSMC仿真预测的热流值明显高于飞行观测值,导致飞行器防热系统的保守设计.本文发展了一种基于壁面辐射平衡的DSMC边界模型,通过热流值反算辐射平衡壁面温度,并以此温度作为下一个时间步DSMC计算的边界条件,迭代更新至给出壁面温度的收敛值.基于该温度边界条件,开发了适用于轴对称构型的DSMC求解器,并以钝锥构型对计算模型和求解器进行了验证.重点针对激波风洞试验条件下的双锥构型,开展数值模拟研究,结果表明:该构型恒温冷壁条件得到的壁面压力分布和热流与风洞试验结果吻合,两种温度条件下的压力峰值差异约为15.4%,但是整体气动力特性差异仅约为0.33%;相对于冷壁,辐射平衡计算得到的前缘处热流峰值降低约50%,再附点处的热流峰值降低约三分之二;两种条件相结合,可以给出壁面热流的预测范围.  相似文献   
268.
利用2008-2010年6-8月共9个月的地面观测资料、高空观测资料和探空资料,分析发生强对流天气的天气形势,进行相关性分析并使用消空法筛选有利于强对流天气发生的物理量因子和指数.分析和检验结果表明:在系统性天气过程影响下K指数、沙氏指数(SI)、700hPa假相当位温(θse(700))和地面24小时变温(△T24)对广汉机场12小时强对流天气潜势预报有较好的指导作用.  相似文献   
269.
为了抑制积分运算带来的捷联惯性姿态累积误差.根据姿态角三角函数关系引入横滚、俯仰角的三个替换变量作为姿态变量,并根据系统姿念变量之间的约束方程和运动体的前向速度测量提出了基于半球谐振陀螺的捷联惯性姿态确定系统的一种扩展卡尔曼粒子滤波算法.采用基于国产半球谐振陀螺的捷联惯性测量组合进行实验与仿真,与标准卡尔曼滤波算法进行了比较.实验与仿真结果表明:该算法有效地提高了定姿性能.作为高可靠性姿态确定系统的备用算法,该算法尤其适用于长寿命的小型航天器.  相似文献   
270.
国企改制是一个复杂的社会问题,容易导致各种利益冲突。面对改制中的各种纷争政府应如何面对?在国企改制中政府应当做什么以及不应当做什么?本文结合国企改制中发生的一起案件,探究国企改制中政府行为存在的问题及应对措施,准确定位政府在国企改制中的角色,规范政府行为。  相似文献   
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