全文获取类型
收费全文 | 3030篇 |
免费 | 413篇 |
国内免费 | 476篇 |
专业分类
测绘学 | 610篇 |
大气科学 | 189篇 |
地球物理 | 480篇 |
地质学 | 1275篇 |
海洋学 | 501篇 |
天文学 | 422篇 |
综合类 | 229篇 |
自然地理 | 213篇 |
出版年
2024年 | 9篇 |
2023年 | 36篇 |
2022年 | 117篇 |
2021年 | 144篇 |
2020年 | 129篇 |
2019年 | 170篇 |
2018年 | 103篇 |
2017年 | 146篇 |
2016年 | 154篇 |
2015年 | 164篇 |
2014年 | 182篇 |
2013年 | 187篇 |
2012年 | 179篇 |
2011年 | 196篇 |
2010年 | 135篇 |
2009年 | 187篇 |
2008年 | 178篇 |
2007年 | 190篇 |
2006年 | 146篇 |
2005年 | 177篇 |
2004年 | 162篇 |
2003年 | 129篇 |
2002年 | 119篇 |
2001年 | 75篇 |
2000年 | 94篇 |
1999年 | 57篇 |
1998年 | 58篇 |
1997年 | 70篇 |
1996年 | 40篇 |
1995年 | 41篇 |
1994年 | 34篇 |
1993年 | 22篇 |
1992年 | 25篇 |
1991年 | 10篇 |
1990年 | 13篇 |
1989年 | 17篇 |
1988年 | 8篇 |
1987年 | 2篇 |
1986年 | 3篇 |
1985年 | 1篇 |
1984年 | 2篇 |
1983年 | 3篇 |
1978年 | 2篇 |
1976年 | 1篇 |
1975年 | 1篇 |
1954年 | 1篇 |
排序方式: 共有3919条查询结果,搜索用时 15 毫秒
351.
352.
353.
C. R. Kaiser 《Monthly notices of the Royal Astronomical Society》2006,367(3):1083-1094
Flat radio spectra with large brightness temperatures at the core of active galactic nuclei and X-ray binaries are usually interpreted as the partially self-absorbed bases of jet flows emitting synchrotron radiation. Here we extend previous models of jets propagating at large angles to our line of sight to self-consistently include the effects of energy losses of the relativistic electrons due to the synchrotron process itself and the adiabatic expansion of the jet flow. We also take into account energy gains through self-absorption. Two model classes are presented. The ballistic jet flows, with the jet material travelling along straight trajectories, and adiabatic jets. Despite the energy losses, both scenarios can result in flat emission spectra; however, the adiabatic jets require a specific geometry. No re-acceleration process along the jet is needed for the electrons. We apply the models to observational data of the X-ray binary Cygnus X-1. Both models can be made consistent with the observations. The resulting ballistic jet is extremely narrow with a jet opening angle of only 5 arcsec. Its energy transport rate is small compared to the time-averaged jet power and therefore suggests the presence of non-radiating protons in the jet flow. The adiabatic jets require a strong departure from energy equipartition between the magnetic field and the relativistic electrons. These models also imply a jet power of two orders of magnitude higher than the Eddington limiting luminosity of a 10-M⊙ black hole. The models put strong constraints on the physical conditions in the jet flows on scales well below achievable resolution limits. 相似文献
354.
Boris Bardin 《Celestial Mechanics and Dynamical Astronomy》2002,82(2):163-177
We deal with the planar restricted circular problem of three bodies. We study trajectories in a small neighborhood of the Lagrange equilibrium point L
4 when mass ratio is close to Routh's value. In particular, we show that the case of proper degeneracy takes place and for most initial conditions trajectories are conditionally-periodic. We obtain an approximate representation of families of periodic solution emanating from the equilibrium point L
4. We also show that in the case of instability of L
4 the trajectories starting in a vicinity of L
4 remain in a finite domain forever. We give an upper bound of this domain. To carry out our investigation, we analyze the dynamics of a general Hamiltonian system with two degrees of freedom in the case of 1 : 1 resonance in detail.This revised version was published online in October 2005 with corrections to the Cover Date. 相似文献
355.
Churyumov Klim I. Luk'yanyk Igor V. Berezhnoi Alexei A. Chavushyan Vahram H. Sandoval Lourdes S. Palma Alejandro A. 《Earth, Moon, and Planets》2002,90(1-4):361-368
We present a preliminary analysis of medium resolution optical spectra of comet C/2000 WM1 (LINEAR) obtained on 22 November
2001. Theemission lines of the molecules C2, C3, CN, NH2,H2O+ and presumably CO (Asundi and triplet bands) and C2
-were identified in these spectra. By analysing the brightnessdistributions of the C2, C3, CN emission lines along theslit of the spectrograph we determined some physical parameters of theseneutrals, such as their
lifetimes and expansion velocities inthe coma. The Franck–Condon factors for the CO Asundi bands and C2
- bands were calculated using a Morse potential model. 相似文献
356.
毫秒脉冲星定时研究进展 总被引:1,自引:0,他引:1
毫秒脉冲星守时的理论和方法研究己取得重要进展,利用现有2颗毫秒脉冲星约10yr的计时观测资料分析得到的 TAI-PT,其长期稳定度为 2×10-14。采用合适的长期稳定度算法,由多颗毫秒脉冲星计时观测可以建立综合脉冲星时间尺度。它可以成为与原子时系统比较的重要手段,并对原子时长期稳定度的改进做出贡献。介绍了该领域研究的基本状况,重点对毫秒脉冲星守时的理论方法,综合脉冲星时间及与原子时的关系等进行了讨论和评述。对由双星系统内毫秒脉冲星的轨道运动定义的双星脉冲星时也做了介绍。 相似文献
357.
The nucleus, coma, and dust jets of short-period Comet 19P/Borrelly were imaged from the Deep Space 1 spacecraft during its close flyby in September 2001. A prominent jet dominated the near-nucleus coma and emanated roughly normal to the long axis of nucleus from a broad central cavity. We show it to have remained fixed in position for more than 34 hr, much longer than the 26-hr rotation period. This confirms earlier suggestions that it is co-aligned with the rotation axis. From a combination of fitting the nucleus light curve from approach images and the nucleus' orientation from stereo images at encounter, we conclude that the sense of rotation is right-handed around the main jet vector. The inferred rotation pole is approximately perpendicular to the long axis of the nucleus, consistent with a simple rotational state. Lacking an existing IAU comet-specific convention but applying a convention provisionally adopted for asteroids, we label this the north pole. This places the sub-solar latitude at ∼60° N at the time of the perihelion with the north pole in constant sunlight and thus receiving maximum average insolation. 相似文献
358.
359.
Picazzio Enos De Almeida Amaury A. Churyumov Klim I. Andrievski Sergei M. Luk'yanyk Igor V. 《Earth, Moon, and Planets》2002,90(1-4):391-400
We report on the preliminary analysis of the high-resolution spectrum of CometC/2000 WM1 (LINEAR), obtained on Dec. 1, 2001
with the Fiber fed ExtendedRange Optical Spectrograph (FEROS) installed on the 1.52-m telescope of ESO(Chile). Many emission
lines of the molecules C2, C3, CN, CH, CH+,NH2, CO, CO+, H2O+ and, presumably, C2
- were identifiedin the spectral range 400–900 nm.
Also, near-infrared photometry was performed on Dec. 2 and 3, with the infraredcamera (CamIV) attached to the 0.60-m Boller
and Chivens telescope of the Picodos Dias Observatory (LNA/MCT), Brazil. We report the preliminary and comparativeanalysis
of the I-J and J-H color indices. 相似文献
360.