全文获取类型
收费全文 | 498篇 |
免费 | 53篇 |
国内免费 | 125篇 |
专业分类
航空 | 235篇 |
航天技术 | 199篇 |
综合类 | 22篇 |
航天 | 220篇 |
出版年
2024年 | 2篇 |
2023年 | 12篇 |
2022年 | 9篇 |
2021年 | 44篇 |
2020年 | 36篇 |
2019年 | 14篇 |
2018年 | 23篇 |
2017年 | 16篇 |
2016年 | 24篇 |
2015年 | 25篇 |
2014年 | 47篇 |
2013年 | 31篇 |
2012年 | 33篇 |
2011年 | 36篇 |
2010年 | 28篇 |
2009年 | 15篇 |
2008年 | 18篇 |
2007年 | 30篇 |
2006年 | 65篇 |
2005年 | 30篇 |
2004年 | 9篇 |
2003年 | 22篇 |
2002年 | 13篇 |
2001年 | 2篇 |
2000年 | 7篇 |
1999年 | 24篇 |
1998年 | 14篇 |
1997年 | 5篇 |
1996年 | 10篇 |
1995年 | 13篇 |
1994年 | 11篇 |
1993年 | 2篇 |
1992年 | 2篇 |
1991年 | 2篇 |
1990年 | 1篇 |
1989年 | 1篇 |
排序方式: 共有676条查询结果,搜索用时 437 毫秒
131.
本文例举观测实例说明,在宁静太阳风中或重现太阳风的低速流区,有可能形成行星际亚阿尔文波速流。这种流出现在阿尔文波速异常增强区,并与特定的磁场位形相联系。 相似文献
132.
太阳电子事件粒子源区的位置 总被引:1,自引:0,他引:1
对ISEE-3的引个太阳电子事件资料,进行了系统地分析。通过Saha平衡模型分别计算了高Fe事件和贫Fe事件源区的平衡温度大小,指出两类事件粒子源区不相重合,高Fe事件的粒子源区位于高色球层,贫Fe事件粒子源区在色球层-日冕之间的过渡区。对高Fe事件和贫Fe事件的形成作了初步的设想。 相似文献
133.
太阳能帆板的功率衰减特性分析,对地外天体表面探测器的功率平衡、电源系统健康管理以及长寿命在轨管理有重要意义。通过对月面巡视器在轨运行第2到11月昼的电流遥测进行研究,提出了一种基于有限遥测的太阳能帆板功率衰减特性分析方法。首先利用一种滞环的方法对大量的电流遥测进行数据处理;然后进行日月距离和太阳入射角的归一化,通过数据拟合计算,得出落月第一年太阳能帆板功率衰减约为2.5%,并利用巡视器历次月昼唤醒时刻的太阳入射角变化情况验证了该方法的有效性,对地外天体的太阳能帆板功率衰减特性计算提供一定参考。 相似文献
134.
GEO卫星热控涂层αS 退化空间综合环境模拟试验 总被引:1,自引:1,他引:1
文章用综合低能辐照试验模拟15年地球同步轨道环境对热控材料S781白漆、SR107-ZK白漆、镀银FEP、OSR片的太阳吸收率退化趋势。有机白漆有严重退化,而OSR和 镀银FEP材料退化较少。通过与飞行试验结果比较,证明了本次模拟试验的有效性。通过利用退化趋势的试验数据,应用最小二乘法获得退化数学模型。二次指数退化模型与4种材料退化曲线符合较好。更长试验时间结果可以通过数学模型外推的方法获得。经试验验证,用8年试验数据外推15年数据误差不超过1%。 相似文献
135.
136.
针对采用可变速控制力矩陀螺(VSCMG)进行柔性太阳翼振动抑制问题,提出一种基于求解非光滑 H∞ 综合问题的最优参数正位置反馈(PPF)控制方法。首先,建立考虑VSCMG和柔性太阳翼耦合的振动模型,得到了线性化的约束陀螺柔性板动力学模型,基于同位控制思想推导了以角度陀螺为测量装置的约束陀螺柔性板全阶状态空间模型。针对被控对象特性,确定最优PPF控制器的结构构型和待优化参数。进而,通过对约束陀螺柔性板全阶状态空间模型进行降阶、修正和加权处理,将PPF控制器参数优化问题转化为在PPF控制器构型约束条件下的非光滑H∞综合问题,并应用一阶下降算法进行寻优求解,实现最优PPF控制器的设计。该方法能够实现对各阶陀螺模态的独立控制,在保证快速性和鲁棒性的前提下,实现最优PPF参数的稳定高效求解。仿真结果表明,所提出的最优PPF控制方法能够快速、鲁棒地实现航天器柔性太阳翼的主动振动抑制。 相似文献
137.
John Vallerga 《Space Science Reviews》1996,78(1-2):277-288
Because of the strong absorption of extreme ultraviolet radiation by hydrogen and helium, almost every observation with the Extreme Ultraviolet Explorer (EUVE) satellite is affected by the diffuse clouds of neutral gas in the local interstellar medium (LISM). This paper reviews some of the highlights of the EUVE results on the distribution and physical state of the LISM and the implications of these results with respect to the interface of the LISM and the heliosphere. The distribution of sources found with the EUVE all-sky surveys shows an enhancement in absorption toward the galactic center. Individual spectra toward nearby continuum sources provide evidence of a greater ionization of helium than hydrogen in the Local Cloud with an mean ratio of H I/He I of 14.7. The spectral distribution of the EUV stellar radiation field has been measured, which provides a lower limit to local H II and He II densities, but this radiation field alone cannot explain the local helium ionization. A combination of EUVE measurements of H I, He I, and He II columns plus the measurement of the local He I density with interplanetary probes can place constraints on the local values of the H I density outside the heliosphere to lie between 0.15 and 0.34 cm–3 while the H II density ranges between 0.0 and 0.14 cm–3. The thermal pressure (P/k = nT) of the Local Cloud is derived to be between 1700 and 2300 cm–3 K, a factor of 2 to 3 above previous estimates. 相似文献
138.
Non-linear evolution of reconnection is too slow to explain-by itself-fast phenomena such as internal disruptions in tokamaks or flares in the solar atmosphere. It has been proposed that the change in topology could lead to field line stochastization, and hence to highly increased transport. An important objection to this idea is that the increase of transport coefficients should smoothly follow the amplitude of the perturbation, while the observations show a catastrophic transition. We have shown 1) that the shape of the structures (and not only their size or amplitude) evolve during non-linear evolution 2) that the stochastic threshold can be strongly influenced by the detailed shape. Therefore, sharp transitions can appear during the evolution, due to the combination of these two effects. We will first consider an idealized situation, namely the two-waves problem in slab geometry, for which we will study the effect of the separatrix shape on the stochastic threshold. In the second part, we will present an application to the internal disruption in tokamaks, with anm=1 perturbation in a toroidal magnetic configuration. In the last part, we will discuss possible applications of the studies on shape effects to the behaviour of trapped particles in structures of the solar atmosphere. 相似文献
139.
D. J. Wu 《Space Science Reviews》2005,121(1-4):333-342
Nonthermal electrons play a major role during solar flares since not only they contain a large amount of the released energy
but also they provide important information of the flaring physics through their nonthermal radiation in radio and hard X-ray
bands. In a recent work Wu (Phys. Plasmas
10 (2003) 1364) proposed that dissipative solitary kinetic Alfvén wave (DSKAW) with a local shock-like structure could provide an efficient acceleration mechanism for energetic electrons in a
low-β plasma. In the present paper dynamical characteristics of the DSKAW acceleration mechanism in solar coronal plasmas
are studied and its application to the acceleration of flaring electrons is discussed. 相似文献
140.
Roger A. Kopp 《Space Science Reviews》1994,70(1-2):309-316
The working group on coronal streamers convened on the first day of the 2nd SOHO Workshop, which took place in Marciana Marina, Isola d'Elba, 27 September –1 October 1993. Recent progress in streamer observational techniques and theoretical modeling was reported. The contribution of streamers to the mass and energy supply for the solar wind was discussed. Moreover, the importance of thin electric current sheets for determining both the gross dynamical properties of streamers and the fine-scale filamentary structure within streamers, was strongly emphasized. Potential advances to our understanding of these areas of coronal physics that could be made by the contingent of instruments aboard SOHO were pointed out. 相似文献