全文获取类型
收费全文 | 6935篇 |
免费 | 302篇 |
国内免费 | 387篇 |
专业分类
航空 | 3780篇 |
航天技术 | 2266篇 |
综合类 | 450篇 |
航天 | 1128篇 |
出版年
2021年 | 53篇 |
2019年 | 43篇 |
2018年 | 77篇 |
2017年 | 45篇 |
2016年 | 66篇 |
2015年 | 66篇 |
2014年 | 156篇 |
2013年 | 206篇 |
2012年 | 181篇 |
2011年 | 278篇 |
2010年 | 259篇 |
2009年 | 259篇 |
2008年 | 385篇 |
2007年 | 256篇 |
2006年 | 186篇 |
2005年 | 211篇 |
2004年 | 194篇 |
2003年 | 244篇 |
2002年 | 152篇 |
2001年 | 233篇 |
2000年 | 177篇 |
1999年 | 222篇 |
1998年 | 276篇 |
1997年 | 207篇 |
1996年 | 222篇 |
1995年 | 245篇 |
1994年 | 243篇 |
1993年 | 184篇 |
1992年 | 207篇 |
1991年 | 121篇 |
1990年 | 107篇 |
1989年 | 171篇 |
1988年 | 69篇 |
1987年 | 84篇 |
1986年 | 81篇 |
1985年 | 170篇 |
1984年 | 138篇 |
1983年 | 116篇 |
1982年 | 134篇 |
1981年 | 150篇 |
1980年 | 66篇 |
1979年 | 64篇 |
1978年 | 50篇 |
1977年 | 38篇 |
1975年 | 54篇 |
1974年 | 44篇 |
1973年 | 40篇 |
1972年 | 48篇 |
1971年 | 43篇 |
1969年 | 39篇 |
排序方式: 共有7624条查询结果,搜索用时 15 毫秒
131.
Chao-Song Huang J.C. Foster K. Yumoto J.L. Chau O. Veliz 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,36(12):2407-2412
It is well known that the solar wind can significantly affect high-latitude ionospheric dynamics. However, the effects of the solar wind on the middle- and low-latitude ionosphere are much less studied. In this paper, we report observations that large perturbations in the middle- and low-latitude ionosphere are well correlated with solar wind variations. In one event, a significant (20–30%) decrease of the midlatitude ionospheric electron density over a large latitudinal range was related to a sudden drop in the solar wind pressure and a northward turning of the interplanetary magnetic field, and the density decrease became larger at lower latitudes. In another event, periodic perturbations in the dayside equatorial ionospheric E × B drift and electrojet were closely associated with variations in the interplanetary electric field. Since the solar wind is always changing with time, it can be a very important and common source of ionospheric perturbations at middle- and low-latitudes. The relationship between solar wind variations and significant ionospheric perturbations has important applications in space weather. 相似文献
132.
L. Balmaceda A. Dal Lago G. Stenborg C. Francile W.D. Gonzalez R. Schwenn 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2003,32(12):2625-2630
In this work we have tracked coronal mass ejections observed with the ground based Mirror Coronagraph for Argentina (MICA) and the Large Angle and Spectroscopic Coronagraph (LASCO) C2 and C3 on board of the Solar and Heliospheric Observatory (SOHO). The MICA telescope is located at El Leoncito (31.8 S, 69.3 W), San Juan (Argentina), since 1997 as part of a bilateral scientific project between Germany and Argentina. SOHO is a project of international cooperation between ESA and NASA. Together these instruments are able to observe the solar corona ranging from 1.05 to 32 solar radii. MICA images the Fe XIV emission line corona and LASCO coronagraphs observe the Thomson scattered white light corona. We have selected events for which there are observations from the three coronagraphs. Using the composite data we were able to obtain height-time diagrams for the corresponding dynamical coronal features traveling outwards in order to determine some of their kinematical properties, i.e., plane of sky velocity and acceleration. 相似文献
133.
本文根据粘性流体力学原理和转子动力学理论,分析了椭圆齿轮流量计的缝隙漏流和转子受力状况,建立了能预测介质粘性对流量计误差特性和压力损失影响的理论模型。数值计算表明,理论值与实验数据基本吻合。 相似文献
134.
南极长城站电离层变化的数值模拟 总被引:1,自引:0,他引:1
南极长城站夏季电离层日变化具有Weddell海异常现象.本文利用一个一维时变理论模式,对长城站夏季电离层f0F2和hm日变化进行了数值模拟.我们讨论了中性风和顶部输运通量对f0F2和hm的影响,认为模拟计算得到的f0F2值比实测值要大的一个主要原因是国际参考电离层给出的上边界值偏大.文章最后介绍了一个获得实际的f0F2和hm的方法. 相似文献
135.
Comparing the improved Di Giovanni/Radicella model with sounding-based electron density profiles and with the IRI model 总被引:1,自引:0,他引:1
W. Singer J. Weiss J. Bremer 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1994,14(12):83-86
The Di Giovanni/Radicella model (DGR) /1/ determines a bottom side electron densty profile alone from the set of routinely scaled ionogram parameters foE, foF1, foF2 and M(3000)F2 and the total electron content; the smoothed sunspot number R12 appears in the calculation. Present designations are DGR2/2/ and DRR3 /3/ [see Appendix]; they are valid in the northern hemisphere. DGR is compared with electron density profiles derived from ionograms obtained at Juliusruh (54.6°N, 13.4°E), and with the (URSI-based) IRI90 at different conditiones. Experimental total electron content (TEC) data are compared to both models. At the considered station, the profiles obtained by both models are reasonably in agreement amongst themselves and with the experimental data.
The TEC derived from the DGR3 model is in good agreement with experimental TEC, whereas, at high solar activity, IRI90 gives too high TEC values, especially during daytime. 相似文献
136.
简要介绍了海洋一号卫星星载GPS接收机的定位原理、流程和应用,探讨了一种在轨定位结果的确认和互验方法.借助于卫星工具包软件(STK),利用NASA网站公布的HY-1卫星两行根数(TLE)进行卫星轨道推算,生成星下点位置,并与相应时刻星载GPS接收机实测数据得到的星下点位置进行比较,由此得到两种方法定位结果之间的偏差,用实际在轨数据验证了两者的位置符合程度. 相似文献
137.
本文叙述了高空科学气球上一种自行研制的宇宙尘收集器以及气球吊篮系统。利用该系统进行了五次高空字宙尘粒的收集飞行,简述了对所收集的尘粒进行系统研究的结果。 相似文献
138.
本文将应力场分为基本应力场和修正应力场两个部分。基本应力场的应力σ_x用勒让德级数展开,级数的前两项系数用截面法确定;其他应力τ_(xy),σ_y由平衡方程和侧表面边界条件确定;再用余能原理确定其余各项系数。由于该级数收敛很快,故可得到封闭解并能给出该解的应用范围,为精确满足自由端的静力边界条件,又引入一个从自由端到固定端迅速衰减的修正应力场,该应力场的应力在自由端等于已知外力与基本应力解之差。其确定方法与基本应力场相同,它也有一个封闭解。将以上两应力场相加卽可得到满足全部边界条件的解。 相似文献
139.
140.
D O Klymchuk E L Kordyum T V Vorobyova D K Chapman C S Brown 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2003,31(10):2283-2288
Changes in the vacuolation in root apex cells of soybean (Glycine max L. [Merr.]) seedlings grown in microgravity were investigated. Spaceflight and ground control seedlings were grown in the absence or presence of KMnO4 (to remove ethylene) for 6 days. After landing, in order to study of cell ultrastructure and subcellular free calcium ion distribution, seedling root apices were fixed in 2.5% (w/v) glutaraldehyde in 0.1 M cacodylate buffer and 2% (w/v) glutaraldehyde, 2.5% (w/v) formaldehyde, 2% (w/v) potassium antimonate K[Sb(OH)6] in 0.1 M K2HPO4 buffer with an osmolarity (calculated theoretically) of 0.45 and 1.26 osmol. The concentrations of ethylene in all spaceflight canisters were significantly higher than in the ground control canisters. Seedling growth was reduced in the spaceflight-exposed plants. Additionally, the spaceflight-exposed plants exhibited progressive vacuolation in the root apex cells, particularly in the columella cells, to a greater degree than the ground controls. Plasmolysis was observed in columella cells of spaceflight roots fixed in solutions with relatively high osmolarity (1.26 osmol). The appearance of plasmolysis permitted the evaluation of the water status of cells. The water potential of the spaceflight cells was higher than the surrounding fixative solution. A decrease in osmotic potential and/or an increase in turgor potential may have induced increases in cell water potential. However, the plasmolysed (i.e. non-turgid) cells implied that increases in water potential were accompanied with a decrease in osmotic potential. In such cells changes in vacuolation may have been involved to maintain turgor pressure or may have been a result of intensification of other vacuolar functions like digestion and storage. 相似文献