全文获取类型
收费全文 | 311篇 |
免费 | 66篇 |
国内免费 | 27篇 |
专业分类
航空 | 122篇 |
航天技术 | 154篇 |
综合类 | 10篇 |
航天 | 118篇 |
出版年
2024年 | 2篇 |
2023年 | 4篇 |
2022年 | 8篇 |
2021年 | 9篇 |
2020年 | 11篇 |
2019年 | 5篇 |
2018年 | 9篇 |
2017年 | 12篇 |
2016年 | 11篇 |
2015年 | 10篇 |
2014年 | 18篇 |
2013年 | 10篇 |
2012年 | 12篇 |
2011年 | 16篇 |
2010年 | 21篇 |
2009年 | 24篇 |
2008年 | 21篇 |
2007年 | 24篇 |
2006年 | 10篇 |
2005年 | 15篇 |
2004年 | 23篇 |
2003年 | 13篇 |
2002年 | 9篇 |
2001年 | 16篇 |
2000年 | 10篇 |
1999年 | 6篇 |
1998年 | 10篇 |
1997年 | 7篇 |
1996年 | 11篇 |
1995年 | 12篇 |
1994年 | 6篇 |
1993年 | 4篇 |
1992年 | 8篇 |
1991年 | 6篇 |
1990年 | 3篇 |
1989年 | 4篇 |
1984年 | 4篇 |
排序方式: 共有404条查询结果,搜索用时 187 毫秒
91.
92.
J.R. Fernandez C.J. Mertens D. Bilitza X. Xu J.M. Russell III M.G. Mlynczak 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
We present a new technique for improving ionospheric models of nighttime E-region electron densities under geomagnetic storm conditions using TIMED/SABER measurements of broadband 4.3 μm limb radiance. The response of E-region electron densities to geomagnetic activity is characterized by SABER-derived NO+(v) 4.3 μm Volume Emission Rates (VER). A storm-time E-region electron density correction factor is defined as the ratio of storm-enhanced NO+(v) VER to a quiet-time climatological average NO+(v) VER, which will be fit to a geomagnetic activity index in a future work. The purpose of this paper is to demonstrate the feasibility of our technique in two ways. One, we compare storm-to-quiet ratios of SABER-derived NO+(v) VER with storm-to-quiet ratios of electron densities measured by Incoherent Scatter Radar. Two, we demonstrate that NO+(v) VER can be parameterized by widely available geomagnetic activity indices. The storm-time correction derived from NO+(v) VER is applicable at high-latitudes. 相似文献
93.
O.G. Morales-Olivares R.A. Caballero-Lopez 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
Our understanding of galactic cosmic ray (GCR) modulation has advanced greatly in the last three decades. However, we still need an appropriate knowledge of the GCR intensity gradient. Numerical simulations of the transport particle equation allow interpretation of cosmic ray intensities in the heliosphere. We use the numerical solution of the GCR transport equation during solar maximum epoch to compute the radial and latitudinal gradients. Our analysis indicates that adiabatic energy loss plays an important role in the radial distribution of GCR in the inner heliosphere, while in the outer region the diffusion and convection are the relevant processes. The latitudinal gradient is small. 相似文献
94.
V.P. Chuprova S.K. GerasimovaV.G. Grigoryev P.A. KrivoshapkinG.F. Krymsky V.P. MamrukovaV.M. Migunov A.N. PrikhodkoG.V. Shafer G.V. Skripin Ye.Ye. SorokinS.A. Starodubtsev V.E. Timofeev 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Some unknown historical facts of cosmic ray studies in the north-east of the former Soviet Union related to the Yakutsk scientific group are reported for the benefit of the international scientific community. It focuses on the founders of Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy of Siberian Branch of Russian Academy of Sciences. A chronology of measurements of cosmic ray intensity variations since 1949 in Yakutia (Sakha Republic; NE Siberia) is given. In particular, for the first time the data of the first solar cosmic ray event registered at Yakutsk (GLE04), with a small ionization chamber S-2 (volume: 20 L) are presented. Moreover, the data of the large ionization chamber ASK-1 (volume: 950 L) for the 1953–2003 period useful for specialists in the field of cosmic ray variations are also shown. 相似文献
95.
V.G. Grigoryev S.A. StarodubsevP.A. Krivoshapkin A.N. PrikhodkoA.G. Yegorov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(6):943-946
The method has been developed to calculate galactic cosmic ray anisotropy parameters by using on-line data of the neutron monitor 24-NM-64 and muon telescope at the Yakutsk station. The preliminary analysis shows that characteristic changes in the anisotropy parameters caused by the first spherical harmonics of cosmic ray angular distribution are observed 1–2 days before the onset of the most part of large-scale geophysical disturbances on the Earth. There is reason to believe that the attraction of data of geophysical observations of other kinds will allow to develop the forecast methods for the arrival of large-scale interplanetary disturbances at the Earth. 相似文献
96.
A.H. Maghrabi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Radiometric measurements of the thermal radiation originating from the moon’s surface were obtained using an infrared detector operating at wavelengths between 8 and 14 μm. The measurements cover a full moon cycle. The variation of the moon’s temperature with the lunar phase angle was established. The lunar temperatures were 391 ± 2.0 K for the full moon, 240 ± 3.5 K for the first quarter, and 236 ± 3 K for the last quarter. For the rest of the phase angles, the lunar temperature varied between 170 and 380 K. Our results are comparable with those obtained previously at these phase angles. For the new moon phase, the obtained temperature was between 120 and 133 K. With the exception of the new moon phase, our measurements at all the phase angles were consistent with those obtained using Earth-based data and those obtained by the Diviner experiment and the Clementine spacecraft. At the new phase, our measurements were comparable with those obtained from the ground but were significantly higher than those obtained by the Diviner and Clementine data. We attribute this inconsistency to either the calibration curve of our detector, which does not perform well at very low temperatures, or to infrared emission from the atmosphere. A simple linear model to predict the lunar temperature as a function of the phase angle was proposed. The experimental errors that affect the measured temperatures are discussed. 相似文献
97.
A. Maghrabi K. Kudela A. Aldosari M. Almutairi M. Altilasi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(5):1672-1681
In this study downward longwave (LW) atmospheric radiation data for the period of 2014–2020 were used to search for short-term periodicities using fast Fourier transform (FFT). Several local peaks in the power spectrum density were found and established. The time series exhibits a series of significant peaks (exceeding the 95% confidence limit), such as at 273 days, 227 days, 200 days, 178 days, 157 days, 110 days, 120 days, 87 days, 73 days, 53–56 days, 35–30 days, 25–27 days, 21 days, 13 days, and 9–10 days.Moreover, cosmic ray data from KACST muon detector and the Oulu neutron monitor, as well as the data for the solar radio flux at 10.7 cm (F10.7 cm), Dst index, and solar wind speed for the same period as the LW data, were used to look for common cyclic variations and periodicities matching those found in the LW radiation. This was done to investigate the possible effect of the solar activity parameters on LW radiation. Several common periodicities were observed in the spectra of all the variables considered, such as 227 days, 154–157 days, 25–27 days, and 21 days. Some of the periodicities found in the LW radiation spectrum can be attributed to the modulation of the cosmic ray intensity by solar activity. Others are attributed to the disturbances in the interplanetary magnetic field. Based on the spectral results, we suggest that the solar signals may directly or indirectly affect the variations of the downward longwave radiation, which in turn may affect climate change. 相似文献
98.
99.
介绍了红外无损检测技术的检测原理和对粘接结构产品的试验应用。试验结果表明,红外无损检测技术可以有效的对玻璃钢泡沫夹层、软木粘接、碳纤维蒙皮蜂窝夹层等粘接结构进行产品质量检测,具备广阔的应用前景。 相似文献
100.