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151.
J. Šafránková Z. Němeček L. Přech A. Koval I. Čermák M. Beránek G. Zastenker N. Shevyrev L. Chesalin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(1):153-159
The monitoring of solar wind parameters is a key problem of the space weather program. We are presenting a new solution of plasma parameter determination suitable for small and fast solar wind monitors. The first version will be launched during the SPECTR-R project into a highly elongated orbit with apogee ∼350,000 km. The method is based on simultaneous measurements of the total ion flux and ion integral energy spectrum by six identical Faraday cups. Three of them are dedicated to determination of the ion flow direction, the other three (equipped with control grids supplied by a retarding potential) are used for determination of the density, temperature, and speed of the plasma flow. The version under development is primarily designed for the measurements in the solar wind and tail magnetosheath, thus for velocities range from 270 to 750 km/s, temperatures from 1 to 30 eV, and densities up to 200 cm−3. However, the instrument design can be simply modified for measurements in other regions with a substantial portion of low-energy plasma as a subsolar magnetosheath, cusp or low-latitude boundary layer. Testing of the engineering model shows that the proposed method can provide reliable plasma parameters with a high time resolution (up to 8 Hz). The paper presents not only the method and its technical realization but it documents all advantages and peculiarities of the suggested approach. 相似文献
152.
Christopher J. Mertens Michael F. Moyers Steven A. Walker John Tweed 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
Recent developments in NASA’s deterministic High charge (Z) and Energy TRaNsport (HZETRN) code have included lateral broadening of primary ion beams due to small-angle multiple Coulomb scattering, and coupling of the ion-nuclear scattering interactions with energy loss and straggling. This new version of HZETRN is based on Green function methods, called GRNTRN, and is suitable for modeling transport with both space environment and laboratory boundary conditions. Multiple scattering processes are a necessary extension to GRNTRN in order to accurately model ion beam experiments, to simulate the physical and biological-effective radiation dose, and to develop new methods and strategies for light-ion radiation therapy. In this paper we compare GRNTRN simulations of proton lateral broadening distributions with beam measurements taken at Loma Linda University Proton Therapy Facility. The simulated and measured lateral broadening distributions are compared for a 250 MeV proton beam on aluminum, polyethylene, polystyrene, bone substitute, iron, and lead target materials. The GRNTRN results are also compared to simulations from the Monte Carlo MCNPX code for the same projectile-target combinations described above. 相似文献
153.
Christopher B. Dreyer Kris Zacny John P.H. Steele James R. Schwendeman Gale Paulsen Robert C. Andersen John Skok 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
In this paper we present a conceptual design of a spaceborne instrument for the in situ production of rock thin sections on planetary surfaces. The in situ Automated Rock Thin Section Instrument (IS-ARTS) conceptual design demonstrates that the in situ production of thin sections on a planetary body is a plausible new instrument capability for future planetary exploration. Thin section analysis would reduce much ambiguity in the geological history of a sampled site that is present with instruments currently flown. The technical challenge of producing a thin section device compatible with the spacecraft environment is formidable and has been thought too technically difficult to be practical. Terrestrial thin section preparation requires a skilled petrographist, several preparation instruments that individually exceed typical spacecraft mass and power limits, and consumable materials that are not easily compatible with spaceflight. In two companion papers we present research and development work used to constrain the capabilities of IS-ARTS in the technical space compatible with the spacecraft environment. For the design configuration shown we conclude that a device can be constructed that is capable of 50 sample preparations over a 2 year lifespan with mass, power, and volume constraints compatible with current landed Mars mission configurations. The technical requirements of IS-ARTS (mass, power and number of samples produced) depend strongly on the sample mechanical properties, sample processing rate, the sample size and number of samples to be produced. 相似文献
154.
Christopher B. Dreyer James R. Schwendeman John P.H. Steele Thomas E. Carrell Andrew Niedringhaus John Skok 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
We have developed a rock cutting mechanism for in situ planetary exploration based on abrasive diamond impregnated wire. Performance characteristics of the rock cutter, including cutting rate on several rock types, cutting surface lifetime, and cut rock surface finish are presented. The rock cutter was developed as part of a broader effort to develop an in situ automated rock thin section (IS-ARTS) instrument. The objective of IS-ARTS was to develop an instrument capable of producing petrographic rock thin sections on a planetary science spacecraft. The rock cutting mechanism may also be useful to other planetary science missions with in situ instruments in which sub-sampling and rock surface preparation are necessary. 相似文献
155.
156.
157.
M. Baguhl E. Grün D. P. Hamilton G. Linkert R. Riemann P. Staubach H. A. Zook 《Space Science Reviews》1995,72(1-2):471-476
Interstellar dust detected by the dust sensor onboard Ulysses was first identified after the Jupiter flyby when the spacecraft's trajectory changed dramatically (Grün et al., 1994). Here we report on two years of Ulysses post-Jupiter data covering the range of ecliptic latitudes from 0° to –54° and distances from 5.4 to 3.2 AU. We find that, over this time period, the flux of interstellar dust particles with a mean mass of 3·10–13 g stays nearly constant at about 1·10–4, m–2 s–1 ( sr)–1, with both ecliptic latitude and heliocentric distance.Also presented are 20 months of measurements from the identical dust sensor onboard the Galileo spacecraft which moved along an in-ecliptic orbit from 1.0 to 4.2 AU. From the impact direction and speeds of the measured dust particles we conclude that Galileo almost certainly sensed interstellar dust outside 2.8 AU; interstellar particles may also account for part of the flux seen between 1 and 2.8 AU. 相似文献
158.
为了满足动态燃烧试验对燃烧过程中燃烧放热量、温度、压力多参数动态测量的要求,研制了一套燃烧动态测试系统。首先从理论上分析了碳氢燃料燃烧时的化学反应过程与物理现象,采用光电传感技术,实现了对动态燃烧过程放热量的非接触式测量;其次运用动态理论详细研究了热电偶的动态特性,完善了用双丝频谱补偿法测量动态温度的方法;最后选择了合理的动态压力的测量方案。同时介绍了该系统的结构及工作特点、系统的动态联调结果等。试验表明了测试该系统具有所测参数多、工作性能稳定、动态响应快等特点,可广泛应用于动态与稳态燃烧试验研究或工业过程监控测量中 相似文献
159.
张秋禹%谢钢%罗正平%李郁忠 《宇航材料工艺》2001,31(3):23-25
以少量环氧类低聚体作增容剂,考察了其对聚碳酸酯/半芳族热致液晶聚合物(PC/TLCPA1)体系的增容改性作用。DSC及SEM测试结果表明,少量增容剂的加入明显改善了原位复合体系的相容性。力学性能测定结果表明,当增容剂加入到含有20%LCAPA1的复合体系后,复合体系的拉伸强度和弯曲强度均有一定程度的提高。 相似文献
160.
郑文辉 《郑州航空工业管理学院学报(管理科学版)》2001,19(3):22-25
通过分析作业成本法应用的生产条件,阐述了作业成本法作为成本计算方法和作业管理方法的运用范围,并对我国推广运用成本法,将企业从传统管理会计推向增值管理会计,提出了若干建议。 相似文献