全文获取类型
收费全文 | 596篇 |
免费 | 183篇 |
国内免费 | 102篇 |
专业分类
航空 | 598篇 |
航天技术 | 120篇 |
综合类 | 37篇 |
航天 | 126篇 |
出版年
2024年 | 7篇 |
2023年 | 16篇 |
2022年 | 47篇 |
2021年 | 48篇 |
2020年 | 33篇 |
2019年 | 33篇 |
2018年 | 35篇 |
2017年 | 28篇 |
2016年 | 40篇 |
2015年 | 34篇 |
2014年 | 46篇 |
2013年 | 51篇 |
2012年 | 43篇 |
2011年 | 51篇 |
2010年 | 41篇 |
2009年 | 39篇 |
2008年 | 44篇 |
2007年 | 33篇 |
2006年 | 29篇 |
2005年 | 37篇 |
2004年 | 19篇 |
2003年 | 20篇 |
2002年 | 13篇 |
2001年 | 13篇 |
2000年 | 10篇 |
1999年 | 6篇 |
1998年 | 5篇 |
1997年 | 12篇 |
1996年 | 10篇 |
1995年 | 9篇 |
1994年 | 10篇 |
1993年 | 2篇 |
1992年 | 6篇 |
1991年 | 3篇 |
1990年 | 3篇 |
1989年 | 2篇 |
1988年 | 3篇 |
排序方式: 共有881条查询结果,搜索用时 15 毫秒
661.
Valadis Katsikas George Exarhos Xenophon Moussas 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
In this paper we study the shape, extend and time variations of the solar wind transition surfaces using the Lima and Priest (1993) hydrodynamic model adequately adapted for the case of the solar wind flow. The transition surfaces, namely the Slow (Sonic), the Alfvén, and the Fast Magnetosonic surface, are important boundaries around the Sun and play a crucial role in the development of the solar wind and the structure of the inner heliosphere. We determine the shape and dimension of these surfaces as a function of heliographic latitude using measurements from Ulysses spacecraft, and we also study their temporal variation using data from spacecrafts at 1 AU (OMNI database). Furthermore, we establish their dependence with the solar activity, demonstrating their shape and location for the last two solar cycles. From this we noticed that the temporal variation of all transition surfaces follows the 11-year solar cycle. Finally, from the OMNI database, we have studied the temporal variation over the past 40 years of the plasma β parameter, the kinetic to magnetic and the kinetic to thermal energy ratios, at a distance of 1 AU from the Sun. 相似文献
662.
D.M. Moeketsi L.A. McKinnell W.L. Combrinck 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
For more than a decade, ionospheric research over South Africa has been carried out using data from ionosondes geographically located at Madimbo (28.38°S, 30.88°E), Grahamstown (33.32°S, 26.50°E), and Louisvale (28.51°S, 21.24°E). The objective has been modelling the bottomside ionospheric characteristics using neural networks. The use of Global Navigation Satellite System (GNSS) data is described as a new technique to monitor the dynamics and variations of the ionosphere over South Africa, with possible future application in high frequency radio communication. For this task, the University of New Brunswick Ionospheric Modelling Technique (UNB-IMT) was applied to compute midday (10:00 UT) GNSS-derived total electron content (GTEC). GTEC values were computed using GNSS data for stations located near ionosondes for the years 2002 and 2005 near solar maximum and minimum, respectively. The GTEC was compared with the midday ionosonde-derived TEC (ITEC) measurements to validate the UNB-IMT results. It was found that the variation trends of GTEC and ITEC over all stations are in good agreement and show a pronounced seasonal variation for the period near solar maximum, with maximum values (∼80 TECU) around autumn and spring equinoxes, and minimum values (∼22 TECU) around winter and summer. Furthermore, the residual ΔTEC = GTEC − ITEC was computed. It was evident that ΔTEC, which is believed to correspond to plasmaspheric electron content, showed a pronounced seasonal variation with maximum values (∼20 TECU) around equinoxes and minimum (∼5 TECU) around winter near solar maximum. The equivalent ionospheric and total slab thicknesses were also computed and comprehensively discussed. The results verified the use of UNB-IMT as one of the tools for future ionospheric TEC research over South Africa. 相似文献
663.
IMU/磁罗盘/GPS组合导航系统设计 总被引:2,自引:0,他引:2
设计了一个IMU/GPS/磁罗盘组合导航系统和相应导航算法,针对该系统的特点设计了特殊的静基座对准算法。根据系统元器件的特殊性和以往工作经验,采用渐消记忆Kalman滤波算法对IMU和GPS信息进行组合。跑车实验表明,该系统具有精度高,工作稳定等优点,达到了设计要求。 相似文献
664.
665.
全流量补燃循环液氧/甲烷发动机系统分析 总被引:1,自引:0,他引:1
对全流量补燃循环液氧,甲烷发动机系统进行了分析研究。确定了初步的发动机系统方案,对发动机的系统参数、结构质量进行了分析计算。 相似文献
666.
根据民用航空发动机压比提出分段FOX(formation and oxidation)方法,估算民用航空发动机LTO(landing and takeoff)循环黑碳(BC)颗粒质量排放指数,结合航空发动机机场实际运行时间和燃油流量修正,编制了2018年国内某国际机场某周国内民航航班黑碳颗粒质量排放清单。结果表明:考虑燃油流量修正的分段FOX方法对民用航空发动机慢车、进近等低工况的黑碳颗粒质量估算精度较FOX方法提高1~2倍,爬升、起飞等高工况估算值更接近实验值。考虑民航实际运行时间和燃油流量后,2018年此国际机场国内民航进出港LTO循环黑碳颗粒质量周排放量约300 kg,其中B737、A320等中型机离港(起飞和爬升阶段为主)阶段排放贡献超70%。 相似文献
667.
668.
669.
Melinda Nagy Alexandre Lemerle Paul Charbonneau 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(4):1425-1433
The solar dipole moment at activity minimum is a good predictor of the strength of the subsequent solar cycle. Through a systematic analysis using a state-of-the-art D solar dynamo model, we found that bipolar magnetic regions (BMR) with atypical characteristics can modify the strength of the next cycle via their impact on the buildup of the dipole moment as a sunspot cycle unfolds. In addition to summarizing these results, we present further effects of such “rogue” BMRs. These have the ability to generate hemispheric asymmetry in the subsequent sunspot cycle, since they modify the polar cap flux asymmetry of the ongoing cycle. We found strong correlation between the polar cap flux asymmetry of cycle i and the total pseudo sunspot number asymmetry of cycle . Good correlation also appears in the case of the time lag of the hemispheres of cycle . 相似文献
670.
Characterization of GPS-TEC over African equatorial ionization anomaly (EIA) region during 2009–2016
Temitope Seun Oluwadare Chinh Nguyen Thai Andrew Oke-Ovie Akala Stefan Heise Mahdi Alizadeh Harald Schuh 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(1):282-301
This study characterizes total electron content (TEC) measured by Global Positioning System (GPS) over African equatorial ionization anomaly (EIA) region for 2009–2016 period during both quiet geomagnetic conditions (Kp?≤?1) and normal conditions (1?>?Kp?≤?4). GPS-TEC data from four equatorial/low-latitude stations, namely, Addis Ababa (ADIS: 9.04°N, 38.77°E, mag. lat: 0.2°N) [Ethiopia]; Yamoussoukro (YKRO: 6.87°N, 5.24°W, mag. lat: 2.6°S) [Ivory Coast]; Malindi (MAL2; 3.00°S, 40.19°E, mag. lat: 12.4°S) [Kenya] and Libreville (NKLG; 0.35°N, 9.67°W, mag. lat: 13.5°S) [Gabon] were used for this study. Interesting features like noontime TEC bite-out, winter anomaly during the ascending and maximum phases of solar cycle 24, diurnal and seasonal variations with solar activity have been observed and investigated in this study. The day-to-day variations exhibited ionospheric TEC asymmetry on an annual scale. TEC observed at equatorial stations (EIA-trough) and EIA-crest reach maximum values between ~1300–1600 LT and ~1300–1600 LT, respectively. About 76% of the high TEC values were recorded in equinoctial months while the June solstice predominantly exhibited low TEC values. Yearly, the estimated TEC values increases or decreases with solar activity, with 2014 having the highest TEC value. Solar activity dependence of TEC within the EIA zone reveals that both F10.7?cm index and EUV flux (24–36?nm) gives a stronger correlation with TEC than Sunspot Number (SSN). A slightly higher degree of dependence is on EUV flux with the mean highest correlation coefficient (R) value of 0.70, 0.83, 0.82 and 0.88 for quiet geomagnetic conditions (Kp?≤?1) at stations ADIS, MAL2, NKLG, and YKRO, respectively. The correlation results for the entire period consequently reveals that SSN and solar flux F10.7?cm index might not be an ideal index as a proxy for EUV flux as well as to measure the variability of TEC strength within the EIA zone. The estimated TEC along the EIA crest (MAL2 and NKLG) exhibited double-hump maximum, as well as post-sunset peaks (night time enhancement of TEC) between ~2100 and 2300 LT. EIA formation was prominent during evening/post-noon hours. 相似文献