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991.
关于域F上的向量空间V的一个性质的证明 总被引:1,自引:1,他引:0
李恒沛 《北京航空航天大学学报》1994,20(3):322-323
利用扩张域论述方法,证明域F上的向量空间V的一个基本性质,即在F上,V关于F的基底的元数等于维数(V:F)。 相似文献
992.
R. F. Wimmer-Schweingruber 《Space Science Reviews》2006,123(1-3):471-480
This workshop summary tries to distill the key difficulties and questions in the art of (I)CME physics and strategies to address
them. (I)CMEs are multi-dimensional, multi-parameter, and multi-scale phenomena related to the solar dynamo, corona, and heliosphere.
This workshop illustrates the immense progress made in describing and modeling these spectacular energetic solar events, but
also shows clear shortcomings in our understanding of them. 相似文献
993.
Cassini Plasma Spectrometer Investigation 总被引:1,自引:0,他引:1
《Space Science Reviews》2004,114(1-4):1-112
The Cassini Plasma Spectrometer (CAPS) will make comprehensive three-dimensional mass-resolved measurements of the full variety of plasma phenomena found in Saturn’s magnetosphere. Our fundamental scientific goals are to understand the nature of saturnian plasmas primarily their sources of ionization, and the means by which they are accelerated, transported, and lost. In so doing the CAPS investigation will contribute to understanding Saturn’s magnetosphere and its complex interactions with Titan, the icy satellites and rings, Saturn’s ionosphere and aurora, and the solar wind. Our design approach meets these goals by emphasizing two complementary types of measurements: high-time resolution velocity distributions of electrons and all major ion species; and lower-time resolution, high-mass resolution spectra of all ion species. The CAPS instrument is made up of three sensors: the Electron Spectrometer (ELS), the Ion Beam Spectrometer (IBS), and the Ion Mass Spectrometer (IMS). The ELS measures the velocity distribution of electrons from 0.6 eV to 28,250 keV, a range that permits coverage of thermal electrons found at Titan and near the ring plane as well as more energetic trapped electrons and auroral particles. The IBS measures ion velocity distributions with very high angular and energy resolution from 1 eV to 49,800 keV. It is specially designed to measure sharply defined ion beams expected in the solar wind at 9.5 AU, highly directional rammed ion fluxes encountered in Titan’s ionosphere, and anticipated field-aligned auroral fluxes. The IMS is designed to measure the composition of hot, diffuse magnetospheric plasmas and low-concentration ion species 1 eV to 50,280 eV with an atomic resolution M/ΔM ∼70 and, for certain molecules, (such asN
2
+ and CO+), effective resolution as high as ∼2500. The three sensors are mounted on a motor-driven actuator that rotates the entire instrument over approximately one-half of the sky every 3 min.This revised version was published online in July 2005 with a corrected cover date. 相似文献
994.
对所有形如的方程的集合E(D),引入线性变换群G(D),从而将E(D)进行等价分类,并由此提出解空间显易结构唯一性概念,指出Bernoulli类方程具第一显易结构,但其显易结构不唯一,而任何非Bernoulli类方程着具显易结构,则其显易结构必唯一. 相似文献
995.
The forecast of the terrestrial ring current as a major contributor to the stormtime Dst index and a predictor of geomagnetic storms is of central interest to ‘space weather’ programs. We thus discuss the dynamical
coupling of the solar wind to the Earth's magnetosphere during several geomagnetic storms using our ring current-atmosphere
interactions model and coordinated space-borne data sets. Our model calculates the temporal and spatial evolution of H+, O+, and He+ ion distribution functions considering time-dependent inflow from the magnetotail, adiabatic drifts, and outflow from the
dayside magnetopause. Losses due to charge exchange, Coulomb collisions, and scattering by EMIC waves are included as well.
As initial and boundary conditions we use complementary data sets from spacecraft located at key regions in the inner magnetosphere,
Polar and the geosynchronous LANL satellites. We present recent model simulations of the stormtime ring current energization
due to the enhanced large-scale convection electric field, which show the transition from an asymmetric to a symmetric ring
current during the storm and challenge the standard theories of (a) substorm-driven, and (b) symmetric ring current. Near
minimum Dst there is a factor of ∼ 10 variation in the intensity of the dominant ring current ion specie with magnetic local time, its
energy density reaching maximum in the premidnight to postmidnight region. We find that the O+ content of the ring current increases after interplanetary shocks and reaches largest values near Dst minimum; ∼ 60% of the total ring current energy was carried by O+ during the main phase of the 15 July 2000 storm. The effects of magnetospheric convection and losses due to collisions and
wave-particle interactions on the global ring current energy balance are calculated during different storm phases and intercompared.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
996.
Wei Fengsi Feng Xueshang Guo Jian-shan Fan Quanlin Wu Jian 《Space Science Reviews》2003,107(1-2):327-334
Recent progress in space weather research are briefly presented here from three aspects: establishment or improvement in observation
systems, such as extra-soft X-ray detector and γ-ray detector onboard the spacecraft ‘Shen Zhou 2’, new solar radio broad-band
spectrometer, magnetometer-chain, ionosonde and digisonde–chain, laser-lidar system and VHF radar; partial topic progresses
included in CMEs, multi-streamer structures, evolution of interplanetary magnetic field B
z component, regional properties of traveling ionospheric disturbances, a fully-nonlinear global dynamical model for the middle
and upper atmosphere, and a combined prediction method for geomagnetic disturbances; and space weather activity, such as ‘Meridian
Project’ — a national major scientific project, ‘International Space Weather Meridian Circle Program’ — a suggestion of internationalization
of ‘Meridian Project’, ‘Space Weather Research Plan’ — a major research plan from National Natural Science Foundation of China
(NNSFC) and other space weather activities.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
997.
本文利用不动点类的代数化,决定复迭空间的基本群的正规子群H的构成因素及其性质,研究不动点类与H不动点类的关系。 相似文献
998.
Recent research in geographic information systems hasbeen concerned with the construction of algebras tomake inferences about spatial relations by embeddingspatial relations within a space in which decisionsabout compositions are derived geometrically. Wepursue an alternative approach by studying spatialrelations and their inferences in a concrete spatialscenario, a room space that contains such manipulableobjects as a box, a ball, a table, a sheet of paper,and a pen. We derive from the observed spatialproperties an algebra related to the fundamentalspatial concepts of containers and surfaces and showthat this container-surface algebra holds allproperties of Tarski's relation algebra, except forthe associativity. The crispness of the compositionscan be refined by considering the relative size of theobjects) and their roles (i.e., whether it isexplicitly known that the objects are containers orsurfaces). 相似文献
999.