全文获取类型
收费全文 | 232篇 |
免费 | 6篇 |
国内免费 | 2篇 |
专业分类
航空 | 150篇 |
航天技术 | 50篇 |
综合类 | 7篇 |
航天 | 33篇 |
出版年
2022年 | 4篇 |
2021年 | 4篇 |
2020年 | 2篇 |
2019年 | 6篇 |
2018年 | 12篇 |
2017年 | 5篇 |
2016年 | 2篇 |
2015年 | 2篇 |
2013年 | 12篇 |
2012年 | 9篇 |
2011年 | 8篇 |
2010年 | 7篇 |
2009年 | 9篇 |
2008年 | 8篇 |
2007年 | 14篇 |
2006年 | 8篇 |
2005年 | 12篇 |
2004年 | 6篇 |
2002年 | 1篇 |
2001年 | 10篇 |
2000年 | 11篇 |
1999年 | 8篇 |
1998年 | 3篇 |
1997年 | 2篇 |
1996年 | 3篇 |
1995年 | 8篇 |
1994年 | 3篇 |
1992年 | 6篇 |
1991年 | 2篇 |
1989年 | 1篇 |
1985年 | 13篇 |
1984年 | 9篇 |
1983年 | 1篇 |
1982年 | 5篇 |
1981年 | 14篇 |
1980年 | 1篇 |
1977年 | 1篇 |
1975年 | 2篇 |
1973年 | 1篇 |
1972年 | 1篇 |
1971年 | 1篇 |
1969年 | 2篇 |
1963年 | 1篇 |
排序方式: 共有240条查询结果,搜索用时 15 毫秒
211.
J. Büchner 《Space Science Reviews》2006,122(1-4):149-160
Current sheets are essential for energy dissipation in the solar corona, in particular by enabling magnetic reconnection.
Unfortunately, sufficiently thin current sheets cannot be resolved observationally and the theory of their formation is an
unresolved issue as well. We consider two predictors of coronal current concentrations, both based on geometrical or even
topological properties of a force-free coronal magnetic field. First, there are separatrices related to magnetic nulls. Through
separatrices the magnetic connectivity changes discontinuously. Coronal magnetic nulls are, however, very rare. Second, inspired
by the concept of generalized magnetic reconnection without nulls, quasi-separatrix layers (QSL) were suggested. Through QSL
the magnetic connectivity changes continuously, though strongly. The strength of the connectivity change can be quantified
by measuring the squashing of the flux tubes which connect the magnetically conjugated photospheres.
We verify the QSL and separatrix concepts by comparing the sites of magnetic nulls and enhanced squashing with the location
of current concentrations in the corona. Due to the known difficulties of their direct observation, we simulated coronal current
sheets by numerically calculating the response of the corona to energy input from the photosphere, heating a simultaneously
observed Extreme Ultraviolet Bright Point. We did not find coronal current sheets at separatrices but at several QSL locations.
The reason is that, although the geometrical properties of force-free extrapolated magnetic fields can indeed hint at possible
current concentrations, a necessary condition for current sheet formation is the local energy input into the corona. 相似文献
212.
J. Büchner 《Space Science Reviews》2006,124(1-4):345-360
Reconnection is a major commonality of solar and magnetospheric physics. It was conjectured by Giovanelli in 1946 to explain
particle acceleration in solar flares near magnetic neutral points. Since than it has been broadly applied in space physics
including magnetospheric physics. In a special way this is due to Harry Petschek, who in 1994 published his ground breaking
solution for a 2D magnetized plasma flow in regions containing singularities of vanishing magnetic field. Petschek’s reconnection
theory was questioned in endless disputes and arguments, but his work stimulated the further investigation of this phenomenon
like no other. However, there are questions left open. We consider two of them – “anomalous” resistivity in collisionless
space plasma and the nature of reconnection in three dimensions. The CLUSTER and SOHO missions address these two aspects of
reconnection in a complementary way -- the resistivity problem in situ in the magnetosphere and the 3D aspect by remote sensing of the Sun. We demonstrate that the search for answers to both questions
leads beyond the applicability of analytical theories and that appropriate numerical approaches are necessary to investigate
the essentially nonlinear and nonlocal processes involved. Necessary are both micro-physical, kinetic Vlasov-equation based
methods of investigation as well as large scale (MHD) simulations to obtain the geometry and topology of the acting fields
and flows. 相似文献
213.
Dust is an important constituent of cometary emission; its analysis is one of the major objectives of ESA’s Rosetta mission
to comet 67P/Churyumov-Gerasimenko (C–G). Several instruments aboard Rosetta are dedicated to studying various aspects of
dust in the cometary coma, all of which require a certain level of exposure to dust to achieve their goals. At the same time,
impacts of dust particles can constitute a hazard to the spacecraft. To conciliate the demands of dust collection instruments
and spacecraft safety, it is desirable to assess the dust environment in the coma even before the arrival of Rosetta. We describe
the present status of modelling the dust coma of 67P/C–G and predict the speed and flux of dust in the coma, the dust fluence
on a spacecraft along sample trajectories, and the radiation environment in the coma. The model will need to be refined when
more details of the coma are revealed by observations. An overview of astronomical observations of 67P/C–G is given, because
model parameters are derived from this data if possible. For quantities not yet measured for 67P/C–G, we use values obtained
for other comets, e.g. concerning the optical and compositional properties of the dust grains. One of the most important and
most controversial parameters is the dust mass distribution. We summarise the mass distribution functions derived from the
in-situ measurements at comet 1P/Halley in 1986. For 67P/C–G, constraining the mass distribution is currently only possible
by the analysis of astronomical images. We find that both the dust mass distribution and the time dependence of the dust production
rate of 67P/C–G are those of a fairly typical comet. 相似文献
214.
A Baüerle R H Anken R Hilbig N Baumhauer H Rahmann 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(7):1598-1601
Humans taking part in parabolic aircraft flights (PAFs) may suffer from space motion sickness (SMS, a kinetosis). Since it has been repeatedly shown earlier that some fish of a given batch also reveal a kinetotic behavior during PAFs (especially so-called spinning movements and looping responses) and due to the homology of the vestibular apparatus among all vertebrates, fish can be used as model systems to investigate the origin of susceptibility to motion sickness. Therefore, we examined the utricular maculae (they are responsible for the internalization of gravity in teleosteans) of fish swimming kinetotically at microgravity in comparison with animals from the same batch who swam normally. On the histological level, it was found that the total number of both sensory and supporting cells of the utricular maculae did not differ between kinetotic animals as compared to normally swimming fish. Cell density (sensory and supporting cells/100 micrometers2), however, was reduced in kinetotic animals (p<0.0001), which seemed to be due to malformed epithelial cells (increase in cell size) of the kinetotic specimens. Susceptibility to kinetoses may therefore originate in malformed sensory epithelia. 相似文献
215.
Theodor Meyer's 1908 doctoral dissertation, with Ludwig Prandtl (1875–1953) as his advisor, introduced much of what has now become basic gas dynamics: not only the Prandtl–Meyer expansion but also the oblique-shock-wave theory as well. It is arguably the most influential dissertation in all of fluid dynamics. Yet no biography or even a photograph of Meyer has been available in the intervening century. This biography provides some insight into his character and covers his education, dissertation, World War I combat service and long career as an engineer and a teacher of math and physics. 相似文献
216.
A. Langmeier M. Sztajno J. Trümper 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1985,5(3):121-123
We present the results of a search for millisecond rotational pulsations in the X-ray emission of five low-mass X-ray binaries: MXB1728-34, 4U1702-42, 4U1705-44, 4U1755-33 and GX17+2. The data were obtained by the EXOSAT Medium Energy Experiment Argon Counters (1–20 keV) with a time resolution of 7.8125 milliseconds. We searched for periods in the range from 16 msec to 8 sec. Upper limits of 1.5 – 5% were found at a 3 sigma level. 相似文献
217.
B. Ehmann L. Balázs É. Fülöp R. Hargitai P. Kabai B. Péley T. Pólya A. Vargha J. László 《Acta Astronautica》2011,68(9-10):1560-1566
This paper is about a pilot application of narrative psychological content analysis in the psychological status monitoring of Crew 71 of a space analog simulation environment, the Mars Desert Research Station (MDRS). Both the method and its theoretical framework, Scientific Narrative Psychology, are original developments by Hungarian psychologists [5] (László, 2008). The software was NooJ, a multilingual linguistic development environment [11] (Silberztein, 2008). Three measures were conceptualized and assessed: emotional status, team spirit and subjective physical comfort. The results showed the patterns of these three measures on a daily basis at group level, and allowed for detecting individual differences as well. The method is adaptable to languages involved in space psychology, e.g. Russian, French and German in addition to English. 相似文献
218.
Observations of dust in the solar system and in the diffuse interstellar medium are summarized. New measurements of interstellar dust in the heliosphere extend our knowledge about micron-sized and bigger particles in the local interstellar medium. Interplanetary grains extend from submicron- to meter-sized meteoroids. The main destructive effect in the solar system are mutual collisions which provide an effective source for smaller particles. In the diffuse interstellar medium sputtering is believed to be the dominant destructive effect on submicron-sized grains. However, an effective supply mechanism for these grains is presently unknown. The dominant transport mechanisms in the solar system is the Poynting-Robertson effect which sweeps meteoroids bigger than about one micron in size towards the sun. Smaller particles are driven out of the solar system by radiation pressure and electromagnetic interaction with the interplanetary magnetic field. In the diffuse interstellar medium coupling of charged interstellar grains to large-scale magnetic fields seem to dominate frictional coupling of dust to the interstellar gas. 相似文献
219.
D. Offermann H.G. Brückelmann K.M. Torkar H. Widdel 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1981,1(12):123-126
Model mechanisms to explain the D-region winter anomaly have so far not really been successful, considering the many different aspects of this atmospheric/ionospheric phenomenon. A new model is therefore proposed relating the winter anomaly essentially to atmospheric temperature and wind variations. The new mechanism is checked by a set of data obtained during the Western European Winter Anomaly Campaign 1975/76, and additionally by a second set of data taken in earlier years. 相似文献
220.
R. Herrmann P. Rudolph H. Krüger G. Schneider R. Röstel R. Kuhl A.S. Okhotin V.T. Khryapov E.V. Markov I.P. Kazakov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1981,1(5):163-166
Two sublimation experiments with PbTe were performed at 850°C and 750°C under microgravity conditions during the “Salyut-6”-“Soyuz-31” mission in 1978. The sublimation took place on the (100)-face of a PbTe crystal. The condensate grown at 850°C shows in the upper part the formation of a pyramidal habit. The bulk consists of parallel growth colums with [100]-boundary faces. The charge carrier concentration of the electrons (N=1,5·1019 cm?3) is higher than the homogeniety limit for 800°C should permit. This is in contrast to the result obtained on the PbTe crystal of the parallel experiment on the earth. At 750°C a laminated condensate is grown with a low growth rate. The microphotograph of the substrate shows the beginning whisker formation according to the VLS-mechanism. 相似文献