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841.
The behavior of small-scale irregularities of the electron density, which can exist in the near-Earth plasma at the ionospheric and magnetospheric heights is studied. They can be of both natural and artificial origin. The kinetic approach is used, and the Vlasov-Poisson system of equations is numerically solved using the method of large particles. In the plane perpendicular to the magnetic field, the evolution of a single irregularity having a circular cross-section at the initial moment is calculated. The influence of the transverse dimension of the irregularity and the value of deviation from electro-neutrality at the initial moment on the parameters characterizing the process of irregularity evolution is studied. 相似文献
842.
The combination of microelectronic acceleration transducers and an RF telemetry link can provide a reliable means of measuring shaft vibrations of electric drives. Clear advantages include the possibility of installing the instrumentation into currently existing motor systems without any need to use flexible couplings or mounts. The proposed system covers frequencies up to several kilohertz and can handle torque transients of 20 Nm with a typical uncertainty of 1%. The preliminary system is extendable to cover adaptive control of dynamic drive performance and can be customized to specific speed and torque ranges 相似文献
843.
O P Berezovska N V Rodionova E N Grigoryan V I Mitashov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1998,21(8-9):1059-1063
Intensity of osteoclastic resorption and calcium content were investigated in intact limb bones of the newts flown on board of a biosatellite Cosmos-2229 after amputation of their forelimbs and tail. Using X-ray microanalysis it was shown an increase in calcium content in the bones on 20th day after operation. Histological study revealed an activation of osteoclastic resorption on endosteal surface of long bones. The newts exposed after surgery on a biosatellite had the same level of bone mineralisation as operated ground control ones, but the increase in number of polynuclear osteoclasts was lower. 相似文献
844.
845.
Becker R.H. Clayton R.N. Galimov E.M. Lammer H. Marty B. Pepin R.O. Wieler R. 《Space Science Reviews》2003,106(1-4):377-410
Variations in the isotopic ratios of volatile elements in different reservoirs on the terrestrial planets carry information
about processes that operated on the planets since their formation. Comparisons between primordial planetary compositions,
to the extent they can be determined, may help us understand the planetary formation process. This working group report summarizes
our knowledge of terrestrial planet volatile inventories.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
846.
O A Kuznetsov K H Hasenstein 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2001,27(5):887-892
The statoliths in Chara rhizoids are denser and more diamagnetic than the cytoplasm, therefore they can be displaced inside a living cell by a sufficiently strong high gradient magnetic field (HGMF). An experimental setup for intracellular magnetophoresis of statoliths was developed. The movement of statoliths and rhizoid growth was measured by video microscopy either under the influence of gravity or a HGMF equivalent to about 2 g. The contribution of the cytoskeleton to statolith motility was assayed before and after depolymerizing microtubules with oryzalin and F-actin with latrunculin B. Application of latrunculin caused immediate cessation of growth, clumping of statoliths, and application of HGMF resulted in higher displacement of statoliths. Oryzalin had no effect on the behavior of statoliths. The data indicate that magnetophoresis is a useful tool to study the gravisensing system and rheology of the Chara rhizoid. 相似文献
847.
I.S. Veselovsky V. Bothmer P. Cargill A.V. Dmitriev K.G. Ivanov E. Romashets A.N. Zhukov O.S. Yakovchouk 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,36(12):2460-2464
Times of sustained strong northward IMF can interrupt the magnetic storm development and lead to lower levels of geomagnetic activity for many hours. During 1997–2000 we have found two events of this kind observed on November 8, 1998 and October 13, 2000. In both cases, the storms started as usual after arrival of ejecta with a southward IMF component from the Sun to the Earth, but ceased after several hours due to the onset of sustained northward IMF leading to the faster recovery process. After the passage of this so-called positive domain, the storm development started again. The heliospheric magnetic field intensity remained enhanced and nearly constant. The solar origins of the geomagnetic storm interruptions have been investigated. Tentatively they may be related to strong nonlinear Alfvйn type solitary waves excited by non-stationary coronal current variations with a characteristic time-scale of about a day. 相似文献
848.
C Rodier O Vandenabeele-Trambouze R Sternberg D Coscia P Coll C Szopa F Raulin C Vidal-Madjar M Cabane G Israel M F Grenier-Loustalot M Dobrijevic D Despois 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2001,27(2):195-199
If there is, or ever was, life in our solar system beyond the Earth, Mars is the most likely place to search for. Future space missions will have then to take into account the detection of prebiotic molecules or molecules of biological significance such as amino acids. Techniques of analysis used for returned samples have to be very sensitive and avoid any chemical or biological contamination whereas in situ techniques have to be automated, fast and low energy consuming. Several possible methods could be used for in situ amino acid analyses on Mars, but gas chromatography would likely be the most suitable. Returned samples could be analyzed by any method in routine laboratory use such as gas chromatography, already successfully performed for analyses of organic matter including amino acids from martian meteorites. The derivatization step, which volatilizes amino acids to perform both in situ and laboratory analysis by gas chromatography, is discussed here. 相似文献
849.
This paper presents a review of geoid error characteristics of three satellite gravity missions in view of the general problem
of separating scientifically interesting signals from various noise sources. The problem is reviewed from the point of view
of two proposed applications of gravity missions, one is the observation of the mean oceanic circulation whereby an improved
geoid model is used as a reference surface against the long term mean sea level observed by altimetry. In this case we consider
the presence of mesoscale variability during assimilation of derived surface currents in inverse models. The other experiment
deals with temporal changes in the gravity field observed by GRACE in which case a proposed experiment is to monitor changes
in the geoid in order to detect geophysical interesting signals such as variations in the continental hydrology and non-steric
ocean processes. For this experiment we will address the problem of geophysical signal contamination and the way it potentially
affects monthly geoid solutions of GRACE.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
850.
P.O. Petrucci J. Ferreira G. Henri L. Sauge G. Pelletier 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2909-2911
We present a unified accretion–ejection picture that explains the different spectral state of Black Hole X-ray binaries (BHXrB) from radio to X/γ-rays. In this view, the central region of BHXrB has a multi-flow configuration which consists in (1) an outer standard accretion disc, (2) an inner magnetized accretion disc driving, (3) a self-collimated electron–proton MHD jet, surrounding and (4) a relativistic electron–positron beam when adequate conditions are met. This picture provides a simple and unified explanation to the various canonical spectral states of BH X-ray binaries, by varying the transition radius rJ between the inner disc driving jets and the outer standard disc. In this framework, large rJ correspond to Quiescent and Hard states while small rJ correspond to Thermal Dominant ones. In between these two extremes, rJ can reach values that switches on the pair cascade process giving birth to a relativistic electron–positron beam. This would correspond to the bright intermediate state. 相似文献