全文获取类型
收费全文 | 5689篇 |
免费 | 1076篇 |
国内免费 | 1561篇 |
专业分类
测绘学 | 868篇 |
大气科学 | 2729篇 |
地球物理 | 1006篇 |
地质学 | 1033篇 |
海洋学 | 614篇 |
天文学 | 1121篇 |
综合类 | 436篇 |
自然地理 | 519篇 |
出版年
2024年 | 39篇 |
2023年 | 85篇 |
2022年 | 163篇 |
2021年 | 227篇 |
2020年 | 235篇 |
2019年 | 271篇 |
2018年 | 183篇 |
2017年 | 249篇 |
2016年 | 209篇 |
2015年 | 308篇 |
2014年 | 348篇 |
2013年 | 344篇 |
2012年 | 373篇 |
2011年 | 350篇 |
2010年 | 278篇 |
2009年 | 425篇 |
2008年 | 386篇 |
2007年 | 466篇 |
2006年 | 389篇 |
2005年 | 386篇 |
2004年 | 323篇 |
2003年 | 288篇 |
2002年 | 235篇 |
2001年 | 230篇 |
2000年 | 222篇 |
1999年 | 187篇 |
1998年 | 207篇 |
1997年 | 143篇 |
1996年 | 129篇 |
1995年 | 126篇 |
1994年 | 128篇 |
1993年 | 93篇 |
1992年 | 64篇 |
1991年 | 69篇 |
1990年 | 41篇 |
1989年 | 28篇 |
1988年 | 31篇 |
1987年 | 20篇 |
1986年 | 9篇 |
1985年 | 9篇 |
1984年 | 8篇 |
1983年 | 3篇 |
1982年 | 1篇 |
1981年 | 2篇 |
1980年 | 8篇 |
1979年 | 1篇 |
1978年 | 2篇 |
1977年 | 2篇 |
1954年 | 3篇 |
排序方式: 共有8326条查询结果,搜索用时 15 毫秒
91.
92.
93.
浅谈基于ERDAS IMAGINE软件的几何精纠正方法 总被引:1,自引:0,他引:1
随着遥感技术日新月异的发展,它在各个领域的应用已经越来越广泛。目前市场上遥感软件的种类很多,比较具有代表性的软件为美国ERDAS公司开发的遥感图像处理系统。遥感图像的几何精纠正是遥感图像分类、专题制图的基础,也是遥感应用研究的基础。本文正是基于ERDAS IMAGINE软件浅谈遥感影像的几何精纠正方法。 相似文献
94.
95.
以国家重大产业技术开发专项“西部煤炭资源高精度三维地震勘探技术”项目的由来、意义和总体研究目标为引,概括的介绍了项目依托工程中各个专项技术研究完成情况,并对非均匀介质成像技术、高精度三维地震静校正技术、高密度采集技术、特观技术、岩性反演技术、属性体解释技术等六项重大关键技术取得的突破性进展进行了重点说明。指出随着我国煤炭生产重点的逐步西移,应加强诸如叠前、叠后深度偏移技术的研究,以解决复杂山区三维地震面元内地震反射波散射问题,提高其三维地震勘探精度,为西部煤炭工业做出新贡献! 相似文献
96.
Observations of whistlers during quiet times made at low-latitude ground station Nainital (geomag. lat. 19 1 N) are used to deduce plasmasphere-ionosphere coupling fluxes. The whistler data from 3 magnetically quiet days are presented that show a smooth decrease in dispersion with time. This decrease in dispersion is interpreted in terms of a corresponding decrease in electron content of tubes of ionization. The electron densities, electron tube contents (1016 el/m2-tube) and coupling fluxes (10 el m–1 s–2) are computed by means of an accurate curve fitting method developed by Tarcsai (1975) and are in good agreement with the results reported by other workers. 相似文献
97.
The purpose of this paper is to find correlation between OI 6300 Å line intensity with solar and ionospheric parameters. A critical study have been made and the following important results are obtained:
相似文献
(i) | Solar flare index plays more important role for the emissions of 6300 Å line than other solar parameters. |
(ii) | Intensity of 6300 Å line increases linearly with the increase of solar flare index. |
(iii) | Virtual height plays more important role than critical frequency for the emission of 6300 Å line-intensity. |
(iv) | Possible explanation of this type of variation is also presented. |
98.
Chantal Guillard Hervé Delprat Can Hoang-van Pierre Pichat 《Journal of Atmospheric Chemistry》1993,16(1):47-59
The photodegradation of naphthalene (NPH), chosen as a model of polynuclear aromatic pollutants, has been studied in the presence of a layer of four water-insoluble inorganic solids which can be found in the troposphere (TiO2, Fe2O3, muscovite, and a fly ash sample). Direct photolysis of NPH is negligible at >340 nm. Dark adsorption of NPH on TiO2 (mainly anatase, nonporous, 50 m2 g–1) at 293 K corresponds to a surface coverage ofca. 50% at equilibrium. Under these conditions (saturated surface), the stationary-state photocatalytic degradation reaches 0.4 molecule nm–2 h–1 (>340 nm, radiant fluxca. 22 mW cm–2). Dioxygen is required and its partial pressure in air is such that the degradation is zero order in O2. Water vapor markedly increases the rate. The other particulates have also an effect, less important than that of TiO2, however quite noticeable with respect to surface area unit for the fly ash sample which contains 3.2% Fe2O3. Apart from 1,4-naphthoquinone, which is the main intermediate product in all cases, 2-naphthol, phthalide, phthaldialdehyde, phthalic acid, acetophenone, benzaldehyde, benzoic acid are also formed on dry TiO2. Depending on their volatility, these compounds are transferred to the gas phase or remain principally adsorbed on the solid particles where they are further transformed. For instance, phthalic acid (or anhydride) and benzoic acid are generated from 1,4-naphthoquinone. Degradation mechanisms are briefly discussed. 相似文献
99.
A. V. Krivov L. L. Sokolov V. V. Dikarev 《Celestial Mechanics and Dynamical Astronomy》1995,63(3-4):313-339
This paper deals with dynamics of impact ejecta from Phobos and Deimos initially on near-circular equatorial orbits around Mars. For particles emitted in a wide size regime of 1 micron and greater, and taking into account the typical particle lifetimes to be less than 100 years, the motion is governed by two perturbing forces: solar radiation pressure and influence of Mars' oblateness. The equations of motion of particles in Lagrangian non-singular elements are deduced and solved, both analytically and numerically, for different-sized ejecta. We state that the coupled effect of both forces above is essential so that on no account can the oblateness of Mars are be neglected. The dynamics of grains prove to be quite different for the ejecta of Phobos and Deimos. For Deimos, the qualitative results are relatively simple and imply oscillations of eccentricity and long-term variations of orbital inclination, with amplitudes and periods both depending on grain size. For Phobos, the dynamics are shown to be much more complicated, and we discuss it in detail. We have found an intriguous peculiar behavior of debris near 300 µm in size. Another finding is that almost all the Phobos ejecta with radii less than 30 µm (against the values of 5 to 20 µm adopted earlier by many authors) should be rapidly lost by collisions with martian surface. The results of the paper may be the base for constructing an improved model of dust belts that presumably exist around Mars. 相似文献
100.
Nicole Borderies Pierre-yves Longaretti 《Celestial Mechanics and Dynamical Astronomy》1990,49(1):69-98
The purpose of this paper is to present a model for the radiation pressure acceleration of a spherical satellite, due to the radiation reflected by a planet with a uniform albedo. A particular choice of variables allows one to reduce the surface integrals over the lit portion of the planet visible to the satellite to one-dimensional integrals. Exact analytical expressions are found for the integrals corresponding to the case where the spacecraft does not "see" the terminator. The other integrals can be computed either numerically, or analytically in an approximate form. The results are compared with those of Lochry (1966). The model is applied to Magellan, a spacecraft orbiting Venus. 相似文献