全文获取类型
收费全文 | 1108篇 |
免费 | 253篇 |
国内免费 | 218篇 |
专业分类
航空 | 796篇 |
航天技术 | 340篇 |
综合类 | 119篇 |
航天 | 324篇 |
出版年
2024年 | 9篇 |
2023年 | 48篇 |
2022年 | 65篇 |
2021年 | 79篇 |
2020年 | 70篇 |
2019年 | 57篇 |
2018年 | 55篇 |
2017年 | 54篇 |
2016年 | 78篇 |
2015年 | 52篇 |
2014年 | 89篇 |
2013年 | 61篇 |
2012年 | 76篇 |
2011年 | 87篇 |
2010年 | 73篇 |
2009年 | 63篇 |
2008年 | 67篇 |
2007年 | 67篇 |
2006年 | 60篇 |
2005年 | 58篇 |
2004年 | 33篇 |
2003年 | 30篇 |
2002年 | 29篇 |
2001年 | 37篇 |
2000年 | 21篇 |
1999年 | 18篇 |
1998年 | 24篇 |
1997年 | 11篇 |
1996年 | 15篇 |
1995年 | 12篇 |
1994年 | 13篇 |
1993年 | 17篇 |
1992年 | 17篇 |
1991年 | 6篇 |
1990年 | 7篇 |
1989年 | 8篇 |
1988年 | 8篇 |
1987年 | 2篇 |
1986年 | 1篇 |
1984年 | 2篇 |
排序方式: 共有1579条查询结果,搜索用时 15 毫秒
31.
32.
N. Kylafis D. Giannios D. Psaltis 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2810-2812
We propose a jet model for the low/hard state of galactic black-hole X-ray sources which explains the energy spectra from radio to X-rays and a number of timing properties in the X-ray domain such as the time lag spectra, the hardening of the power density spectra and the narrowing of the autocorrelation function with increasing photon energy. The model assumes that (i) there is a magnetic field along the axis of the jet, (ii) the electron density in the jet drops inversely proportional to distance, (iii) the jet is “hotter” near its center than at its periphery, and (iv) the electrons in the jet follow a power-law distribution function. We have performed Monte Carlo simulations of Compton upscattering of soft photons from the accretion disk and have found power-law high-energy spectra with photon-number index in the range 1.5–2 and cutoff at a few hundred keV, power-law time lags versus Fourier frequency with index 0.8, and an increase of the rms amplitude of variability and a narrowing of the autocorrelation function with increasing photon energy as they have been observed in Cygnus X-1. The spectrum at long wavelengths (radio, infrared, optical) is modeled to come from synchrotron radiation of the energetic electrons in the jet. We find flat to inverted radio spectra that extend from the radio up to about the optical band. For magnetic field strengths of the order 105–106 G at the base of the jet, the calculated spectra agree well in slope and flux with the observations. 相似文献
33.
G. Smoot G. De Amici S.D. Friedman C. Witebski N. Mandolesi R.B. Partridge G. Sironi L. Danese G. De Zotti 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
New measurements of the Cosmic Background Radiation temperature at 12 cm, 6.3 cm, 3 cm, 0.9 cm and 0.3 cm have made in July 1982 from the White Mountain High Altitude Research Station. The results are presented and the existence of spectral distortions discussed. 相似文献
34.
同无黑子耀斑相协的微波爆发机制的探讨 总被引:1,自引:0,他引:1
1980—1984年期间,我们在云南天文台9375MHz,3653MHz和2902 HHz三个波段的射电观测资料中,查到11组微波爆发与无黑子耀斑相伴随。本文研究了这些爆发与耀斑的大气层高度,射电爆发类型以及通过落进峰值流量-时间图的位置,确认出爆发机制是活动区中作麦克斯韦分布电子的热轫致辐射。 相似文献
35.
Silvia Zane Roberto Turolla Luciano Nobili Nanda Rea 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
In this paper, we discuss our first attempts to model the broadband persistent emission of magnetars within a self-consistent, physical scenario. We present the predictions of a synthetic model that we calculated with a new Monte Carlo 3D radiative code. The basic idea is that soft thermal photons (e.g. emitted by the star surface) can experience resonant cyclotron upscattering by a population of relativistic electrons treated in the twisted magnetosphere. Our code is specifically tailored to work in the ultra-magnetized regime; polarization and QED effects are consistently accounted for, as well different configurations for the magnetosphere. We discuss the predicted spectral properties in the 0.1–1000 keV range, the polarization properties, and we present the model application to a sample of magnetars soft X-ray spectra. 相似文献
36.
Anne Hutter Felix Spanier 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
We consider a relativistically moving blob consisting of an isotropic electron distribution that Compton-scatters photons from an external isotropic radiation field. We compute the resulting beaming pattern, i.e. the distribution of the scattered photons, in the blob frame as well as in the observer’s frame by using the full Klein–Nishina cross section and the exact incident photon distribution. In the Thomson regime the comparison of our approach with Dermer (1995) results in concurrent characteristics but different absolute number of the scattered photons by a factor of fcorr = 3.09. Additionally, our calculation yields a slightly lower boost factor which varies the more from the corresponding value in Dermer (1995) the higher the spectral index p of the electron distribution gets. 相似文献
37.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(8):1951-1964
A novel method is presented to evaluate on the graphics processing unit (GPU) the force and torque on a spacecraft due to solar radiation pressure. The method employs efficient ray tracing techniques, developed in the graphics rendering discipline, to resolve spacecraft self-shadowing and reflections at faster than real-time computation speed. The primary algorithmic components of the ray tracing process which contribute to the method’s computational efficiency are described. These components include two-level bounding volume hierarchy acceleration data structures, fast ray to bounding box intersection testing using the slab intersection algorithm and fast triangle intersection testing using the Möller-Trumbore algorithm. Spacecraft material optical properties are represented as a combination of Lambertian diffuse and ideal specular reflections. Both diffuse and specular ray-surface interactions are modeled. The approach is implemented using C++ and OpenCL and executed on a consumer grade GPU. Model validation is presented comparing ray traced force and torque values to the same quantities produce by a faceted analytic model. Numerical results illustrate the impact of self-shadowing on the force and torque calculation, and demonstrate the fast computational speed that is enabled with this implementation. 相似文献
38.
39.
为解决框架类零件的高位置度孔的精密镗削加工问题,研发了ZYTC600专用镗削机床.其精度指标优于现有的通用镗床(包括进口镗床),尺寸在500mm范围内,同轴度优于2μm,垂直度优于5μm,其中的关键部件双回转轴系分度精密转台采用了一套精密调整机构,可以实现0.2s”的精密调整,通过有限元分析得到其驱动刚度可达到800N/μm,可以满足加工需求. 相似文献
40.
提高卫星信道资源利用率,探索高效可行的端站接入机制是卫星通信发展亟待解决的问题之一。当前卫星通信DVB-RCS标准基于带宽预先规划的接入机制与端站随遇接入的需求矛盾凸显,因此提出一套信道反馈优化接入机制,综合考虑各端站数据业务需求,在不改变原有协议信令特征的基础上,探索性地引入谦虚度激励方法,创造性地构造动态协商反馈模型并加以求解,达到提高端站接入数量、满足随遇接入需求、提升信道利用效率、最大化整体带宽通信业务效益的目的。通过试验验证,带宽分配反馈优化机制比传统模式提高近1倍接入率,最大端站数接入时算法耗时约只有0.67s,可为卫星信道使用提供技术参考。 相似文献