全文获取类型
收费全文 | 3725篇 |
免费 | 44篇 |
国内免费 | 28篇 |
专业分类
航空 | 1782篇 |
航天技术 | 1321篇 |
综合类 | 71篇 |
航天 | 623篇 |
出版年
2021年 | 35篇 |
2018年 | 51篇 |
2017年 | 61篇 |
2016年 | 34篇 |
2015年 | 35篇 |
2014年 | 74篇 |
2013年 | 100篇 |
2012年 | 85篇 |
2011年 | 164篇 |
2010年 | 115篇 |
2009年 | 141篇 |
2008年 | 209篇 |
2007年 | 117篇 |
2006年 | 111篇 |
2005年 | 119篇 |
2004年 | 83篇 |
2003年 | 119篇 |
2002年 | 91篇 |
2001年 | 111篇 |
2000年 | 89篇 |
1999年 | 103篇 |
1998年 | 109篇 |
1997年 | 101篇 |
1996年 | 89篇 |
1995年 | 104篇 |
1994年 | 107篇 |
1993年 | 64篇 |
1992年 | 75篇 |
1991年 | 39篇 |
1990年 | 44篇 |
1989年 | 74篇 |
1988年 | 39篇 |
1987年 | 32篇 |
1986年 | 34篇 |
1985年 | 113篇 |
1984年 | 79篇 |
1983年 | 79篇 |
1982年 | 59篇 |
1981年 | 103篇 |
1980年 | 25篇 |
1979年 | 27篇 |
1978年 | 33篇 |
1977年 | 25篇 |
1976年 | 23篇 |
1975年 | 39篇 |
1974年 | 20篇 |
1972年 | 33篇 |
1971年 | 25篇 |
1969年 | 22篇 |
1967年 | 23篇 |
排序方式: 共有3797条查询结果,搜索用时 390 毫秒
591.
A special measurement technique allows to determine the stationary and dynamic temperature profiles, acting on a material sample during a Bridgman crystal growth process. It turns out that the thermal field of the furnaces at the place of the sample is modified by a number of device-related factors and by regular correlations. The investigations refer to the execution of experiments in the field of materials sciences in space in furnaces on board Salyut-stations. 相似文献
592.
C.R. Philbrick M.E. Garnder P. Lämmerzhal 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1983,3(1):95-98
Measurements of the density and composition of the thermosphere between 150 and 500 km, which were obtained by the S3-1 satellite, have been compared with the Jacchia and MSIS models. The measurements of the densities of O, N2, N and Ar show some differences from the current models which should be considered during the preparation of the next CIRA model. The Ar measurements are particularly useful in examining the response of the neutral atmosphere to geomagnetic heating. These results are useful in establishing the appropriate lower boundary conditions for modeling of the thermosphere. 相似文献
593.
The Infrared Space Observatory (ISO), a fully approved and funded project of ESA, will operate at wavelengths from 3–200 microns. The satellite essentially consists of a large cryostat containing about 2300 litres of superfluid helium to maintain the telescope (primary mirror diameter of 60 cm) and the scientific instruments at temperatures between 2K and 8K. A pointing accuracy of a few arc seconds is provided by a three-axis-stabilisation system. ISO's instrument complement consists of four instruments, namely: an imaging photo-polarimeter (3–200 microns), a camera (3–17 microns), a short wavelength spectrometer (3–45 microns) and a long wavelength spectrometer (45–180 microns). ISO's scheduled launch date is May 1993 and it will be operational for at least 18 months. In keeping with ISO's role as an observatory, two-thirds of its observing time will be made available to the general astronomical community via several Calls for Observing Proposals. 相似文献
594.
A number of modern spectral estimators are shown to have a common generic formulation. These include minimum variance, MUSIC, and maximum entropy. A new maximum entropy spectral estimator is derived using constraints on the modal powers or the expected-square projections of the data onto the eigenvectors of the data covariance matrix. The formulation incorporates uncertainty in the modal power constraints and the signal-versus-noise subspace separation. The resulting estimators have forms which incorporate all other modern estimators, including maximum entropy and minimum norm. The new estimators allow further development when a priori information is used in the constraints. Comparison of one version of the estimator with the minimum norm verifies the greater probability of resolution of the minimum norm but indicates in some instances the value of the incorporated uncertainties. Another version uses complex constraints and reduces to conventional maximum entropy or minimum norm under certain conditions 相似文献
595.
T.H. Vonder Haar G.G. Campbell E.A. Smith A. Arking K. Coulson J. Hickey F. House A. Ingersoll H. Jacobowitz L. Smith L. Stowe 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1981,1(4):285-297
Two special measurements of the energy exchange between earth and space were made in connection with the FGGE. A global monitoring program using wide-field-of-view and scanner detectors from NASA's NIMBUS-7 satellite successfully returned measurements during the entire FGGE. This experiment system also used a black cavity detector to measure the total energy output of the sun to very high precision. A second set of high frequency time and space estimates of the radiation budget were determined from selected geostationary satellite data. Preliminary results from both radiation budget data sets and the solar “constant” measurements will be presented. 相似文献
596.
E L Powers 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1983,3(8):73-78
Several factors modifying radiation sensitivity in dry bacterial spores are described and discussed. Vacuum inducing the loss of critical structural water, very low dose rates of radiation from which the cell may recover, radiations of high linear energy transfer, and the action of temperature over long periods of time on previously irradiated cells are recognized from extensive laboratory work as important in determining survival of spores exposed to low radiation doses at low temperatures for long periods of time. Some extensions of laboratory work are proposed. 相似文献
597.
L. Sehnal 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1983,3(1):91-94
The atmospheric drag and lift effects are studied on the orbital data of the satellite 1974-70A. The values of the thermal accomodation coefficient and of the drag coefficient are determined. 相似文献
598.
L. Dezső G. Csepura O. Gerlei Á. Kovács I. Nagy 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,4(7):57-60
Using full-disc white light photoheliograms, we have studied umbrae motion and variations in sunspot areas in a large activity complex over 4 solar rotations. On the basis of the observational data we illustrate with typical examples to what extent rapid spot motions are associated with flare occurrences. 相似文献
599.
600.
G.H. Schwehm R.H. Giese F. Giovane D.W. Schuerman J.L. Weinberg 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1981,1(8):121-125
The 1985 International Solar Polar Mission will provide the first opportunity to perform measurements from out of the ecliptic and from above the solar poles. Included in this mission is the Zodiacal Light/Background Starlight Experiment of the Ruhr-University Bochum, FRG (in collaboration with the State University of New York at Albany). The experiment is based on the use of a multicolor, sky-scanning photopolarimeter, which will be carried on the NASA S/C.The scientific objectives of the experiment are to investigate the intensity, polarization, and color of the diffuse sky brightness and determine the spatial distribution and physical properties of the interplanetary dust, including a possible interstellar component, as a function of S/C position in and out of the ecliptic.The instrument will allow simultaneous measurements in two separate wavelength bands. Measurements will be performed at 180, 220, 240, 280, 320, 350, 360, 440, 540, 640, 800 nm, including the state of polarization. Two different fields-of-view (1 sq deg and 5.6 sq deg) can be selected.The use of a microprocessor system in the instrument electronics will provide flexibility in measurement sequences and programs, on-board data processing and data quality control. 相似文献