全文获取类型
收费全文 | 1050篇 |
免费 | 60篇 |
国内免费 | 14篇 |
专业分类
航空 | 113篇 |
航天技术 | 884篇 |
综合类 | 4篇 |
航天 | 123篇 |
出版年
2023年 | 30篇 |
2022年 | 9篇 |
2021年 | 57篇 |
2020年 | 30篇 |
2019年 | 34篇 |
2018年 | 37篇 |
2017年 | 7篇 |
2016年 | 7篇 |
2015年 | 12篇 |
2014年 | 74篇 |
2013年 | 59篇 |
2012年 | 55篇 |
2011年 | 79篇 |
2010年 | 66篇 |
2009年 | 87篇 |
2008年 | 88篇 |
2007年 | 50篇 |
2006年 | 22篇 |
2005年 | 70篇 |
2004年 | 25篇 |
2003年 | 10篇 |
2002年 | 16篇 |
2001年 | 18篇 |
2000年 | 19篇 |
1999年 | 12篇 |
1998年 | 29篇 |
1997年 | 22篇 |
1996年 | 9篇 |
1995年 | 13篇 |
1994年 | 28篇 |
1993年 | 11篇 |
1992年 | 15篇 |
1991年 | 11篇 |
1990年 | 9篇 |
1989年 | 3篇 |
1987年 | 1篇 |
排序方式: 共有1124条查询结果,搜索用时 15 毫秒
71.
High-Altitude Long-Endurance(HALE) solar-powered Unmanned Aircraft Vehicles(UAVs) can utilize solar energy as power source and maintain extremely long cruise endurance,which has attracted extensive attentions from researchers. Trajectory optimization is a promising way to achieve superior flight time because of the finite solar energy absorbed in a day. In this work,a method of trajectory optimization and guidance for HALE solar-powered aircraft based on a Reinforcement Learning(RL) framework is... 相似文献
72.
Convex optimization of asteroid landing trajectories driven by solar radiation pressure 总被引:1,自引:1,他引:0
High-area/mass ratio landers driven by Solar Radiation Pressure(SRP) have potential applications for future asteroid landing missions. This paper develops a new convex optimization-based method for planning trajectories driven by SRP. A Minimum Landing Error(MLE) control problem is formulated to enable planning SRP-controlled trajectories with different flight times. It is transformed into Second Order Cone Programming(SOCP) successfully by a series of different convexification technologies. A t... 相似文献
73.
本文用化学沉积法和电化学沉积法制备太阳能电池用半导体薄膜硫化镉(CdS),对成膜的影响因素进行了测试。结果表明,化学沉积CdS质量较好,沉积速度较慢,受pH的影响较大,且水浴容器壁上沉积有大量的CdS膜。电化学沉积CdS的电流密度在0.5~2.5 m A/cm 2 的范围内,沉积速度快,材料消耗少,但是对电流密度过于敏感,成膜参数难以控制。 相似文献
74.
75.
76.
H.S. Ahluwalia 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The descent of sunspot cycle 23 to an unprecedented minimum of long duration in 2006–2009 led to a prolonged galactic cosmic ray (GCR) recovery to the highest level observed in the instrumental era for a variety of energetic charged particle species on Earth, over a wide range of rigidities. The remarkable GCR increase measured by several ground-based, balloon-borne, and detectors on a satellite is described and discussed. It is accompanied by a decrease in solar wind velocity and interplanetary magnetic field at 1 a.u., reaching the lowest values since measurements of the solar wind began in October 1963; the solar polar field strength (μT) measured at the Wilcox Solar Observatory (WSO) is also significantly reduced compared to prior cycles since the start of the program in 1976, the polar field in the northern hemisphere reversed in June 2012 and again in February 2014, that in the southern hemisphere reversed in July 2013. If updates of WSO data confirm the second reversal in northern solar hemisphere, it would pose a serious challenge to the Dynamo Theory. The long-term change in solar behavior may have begun in 1992, perhaps earlier. The physical underpinnings of these solar changes need to be understood and their effect on GCR modulation processes clarified. The study discusses the recent phenomena in the context of GCR modulation since 1900. These happenings affected our empirical predictions for the key parameters for the next two sunspot cycles (they may be progressively less active than sunspot cycle 24) but it enhanced support for our prediction that solar activity is descending into a Dalton-like grand minimum in the middle of the twentyfirst century, reducing the frequency of the coronal mass ejections; they determine the space weather affecting the quality of life on Earth, radiation dose for hardware and human activities in space as well as the frequency of large Forbush decreases at 1 a.u. 相似文献
77.
78.
H.S. Ahluwalia C. Lopate 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
Solar modulations of galactic cosmic ray (GCR) intensity contain a wealth of information about their transport in the heliosphere. To extract this information from the data one studies the dependence of the observed modulations on the mean energy of response of detectors providing data for the analyses. There is a great deal of confusion about the detector energy response to GCR spectrum in the literature. We present a preliminary report on the computations of the mean energy of response for the Climax neutron monitor (CL/NM) and IMP 8 cosmic ray nuclear composition instrument to GCR protons for 1973–1998, covering the solar cycles 21 and 22. We find that for penetrating proton channel on IMP 8 the mean energy changes by a factor of over two whereas for the neutron monitor the change is only 21%. However, the corresponding change for the computed modulation function is a factor of about 3.5. 相似文献
79.
B. Sylwester J. Sylwester K.J.H. Phillips E. Landi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
We present the observations of He-like Ar triplet lines obtained by RESIK spectrometer aboard CORONAS-F. Interpretation of intensity ratios between triplet lines of lower Z elements is known to provide useful diagnostics of plasma conditions within the emitting source. Here, we investigate whether triplet line ratios are useful for interpretation of higher Z element spectra. A high sensitivity, low background and precise absolute calibration of RESIK allow to consider in addition also the continuum contribution. This provides a way to determine the Ar absolute abundance from the observed triplet component ratios. The method is presented and the results are shown for two selected flares. Derived values of Ar absolute abundance for these flares are found to be similar: 2.6 × 10−6 and 2.9 × 10−6. They fall in the range between presently accepted Ar photospheric and coronal abundances. 相似文献
80.
V. Truhlik D. Bilitza L. Triskova 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
A database of electron temperature (Te) measurements comprising of most of the available satellite measurements in the topside ionosphere is used for studying the solar activity variations of the electron temperature Te at different latitudes, altitudes, local times and seasons. The Te data are grouped into three levels of solar activity (low, medium, high) at four altitude ranges, for day and night, and for equinox and solstices. We find that in general Te changes with solar activity are small and comparable in magnitude with seasonal changes but much smaller than the changes with altitude, latitude, and from day to night. In all cases, except at low altitude during daytime, Te increases with increasing solar activity. But this increase is not linear as assumed in most empirical Te models but requires at least a parabolic approximation. At 550 km during daytime negative as well as positive correlation is found with solar activity. Our global data base allows to quantify the latitude range and seasonal conditions for which these correlations occur. A negative correlation with solar activity is found in the invdip latitude range from 20 to 55 degrees during equinox and from 20 degrees onward during winter. In the low latitude (20 to −20 degrees invdip) F-region there is almost no change with solar activity during solstice and a positive correlation during equinox. A positive correlation is also observed during summer from 30 degrees onward. 相似文献