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71.
Richard B. Rood 《Pure and Applied Geophysics》1985,123(5):733-755
The concept of planetary wave breaking (McIntyre andPalmer, 1983; 1984) is critically reviewed. It is concluded that the wave breaking signature is not unique to any particular dynamic event in the stratosphere. Therefore, the classification of stratospheric transport events, such as wave breaking, groups fundamentally different events together. Better qualification of the wave breaking signature and a more solid theoretical basis of planetary wave breaking must be presented if the concept is to be of significant utility in describing stratospheric tracer transport. 相似文献
72.
D. A. Mendis 《Journal of Earth System Science》1984,93(3):177-188
Recent spacecraft observations of the Saturnian and Jovian ring systems have highlighted a plethora of interesting new phenomena
associated with those regions containing fine (micron and sub-micron sized) dust. Recognizing that these dust grains, by virtue
of being immersed within the planetary magnetospheres, are electrostatically charged to the point that they experience comparable
gravitational and electric forces, a new “gravito-electrodynamic” theory has been developed to describe their dynamics. This
theory has been successful in explaining all these phenomena in a systematic way. In this review, the basic model and its
range of validity are outlined, and its application to the Saturnian and Jovian ring systems are discussed. 相似文献
73.
牛广林 《吉林大学学报(地球科学版)》1987,(3)
本文以太阳系星球的物质状态、形态面貌、体积、物质密度、运动速度、运动方向和角动量等作为根据,研究它们在宇宙空间上的分布特点、相互关系、内在联系以及规律的基础上,提出太阳系(乃至宇宙星球)是在46亿年前,宇宙中一个巨大灼热的星球,在高速度左旋旋转(公转和自转)运动的过程中,从尾部分离出来的物质,经过……恒星、行星和卫星依次波状旋转分离运动产生的。 相似文献
74.
E.V. Pitjeva 《Celestial Mechanics and Dynamical Astronomy》2001,80(3-4):249-271
The JPL planetary and lunar ephemerides – DE200/LE200, DE403/LE403, DE405/LE405 and the planetary and lunar ephemerides, EPM87, EPM98, and EPM2000, constructed in the Institute of Applied Astronomy of RAS are described. Common properties and differences of the various ephemerides are given. Graphical comparisons of the DE ephemerides with each other and with the EPM ephemerides are presented. A fairly good agreement of planetary orbits is between DE403, DE405 and EPM98, EPM2000, respectively, over the interval of 120 years (1886–2006) covered by EPM98 and EPM2000. Some differences are explained by a slight disagreement in representing the orbits of Ceres, Pallas, and Vesta as they affect the planets. The accurate radar observations of planets and spacecraft make it possible not only to improve the orbital elements of planets but to determine a broad set of astronomical constants as well: km/AU, parameters of Mars rotation including its precessional rate, the masses of Jupiter, Ceres, Pallas, and Vesta, relativistic parameters of the PPN formalism, the variability of the gravitational constant G. These have been obtained in the fitting process of the DE405 and EPM2000 ephemerides to observational data, including nearly 80000 American and Russian radar observations of planets (1961–1997), ranging and doppler to the Viking and Pathfinder landers, and other miscellaneous measurements from various sources and spacecraft. 相似文献
75.
Pantelis Soupios Nikos Papadopoulos Ilias Papadopoulos Maria Kouli Filippos Vallianatos Apostolos Sarris Thrassyvoulos Manios 《Environmental Geology》2007,53(3):661-675
An integrated suite of environmental methods was used to characterize the hydrogeological, geological and tectonic regime
of the largest waste disposal landfill of Crete Island, the Fodele municipal solid waste site (MSW), to determine the geometry
of the landfill (depth and spatial extent of electrically conductive anomalies), to define the anisotropy caused by bedrock
fabric fractures and to locate potential zones of electrically conductive contamination. A combination of geophysical methods
and chemical analysis was implemented for the characterization and management of the landfill. Five different types of geophysical
surveys were performed: (1) 2D electrical resistance tomography (ERT), (2) electromagnetic measurements using very low frequencies
(VLF), (3) electromagnetic conductivity (EM31), (4) seismic refraction measurements (SR), and (5) ambient noise measurements
(HVSR). The above geophysical methods were used with the aim of studying the subsurface properties of the landfill and to
define the exact geometrical characteristics of the site under investigation. 相似文献
76.
Investigation of waste disposal areas using electrical methods: a case study from Chania,Crete, Greece 总被引:1,自引:0,他引:1
Pantelis Soupios Ilias Papadopoulos Maria Kouli Irene Georgaki Filippos Vallianatos Eleni Kokkinou 《Environmental Geology》2007,51(7):1249-1261
A geophysical investigation of a landfill area was conducted as inextricable phase of a preliminary geotechnical, geological
and hydrogeological study of the area under investigation. Electrical resistivity tomography (ERT), one of the most promising
prospecting techniques mainly concerning its effective contribution to resolve several environmental problems, was applied
for the geophysical modeling. ERT is a robust imaging method the theory and implementation of which are well documented in
geophysical research literature. The survey site is located in Akrotirion Peninsula, about 7 km east of Chania city in Crete
I. The geological setting comprises Trypalion limestones, marly limestones and a clayed weathered layer. Cavities are also
identified at various scales which are recent tectono-karstic voids. Due to the above-mentioned geological singularity and
in the light of the requirement for an environmentally safe construction of the landfill, an ERT survey was carried out. Specifically,
seven geoelectrical tomographies were conducted reaching the prospecting depth of 36 m. The resulted images conduced, to overcome
geotechnical problems since the spatial distribution of karstic voids was determined, to plan the future sites for waste disposal
as the geological conditions were studied in detail and to reliably estimate the thickness of the already deposited wastes.
The resulted images were confirmed using available borehole logs and ambient noise measurements. 相似文献
77.
78.
吉林通化南岔式金矿地质—地球物理—地球化学综合找矿模型 总被引:9,自引:0,他引:9
老岭成矿带为吉林省最重要的贵金属、有色金属成矿带,南岔金矿是该成矿带近几年新发现的金矿床。在阐述南岔金矿成矿地质条件、岩(矿)石物性参数特征、地球物理场、地球化学特征的基础上,归纳并提取了控矿地质因素和物化控找矿标志,从而建立了“南岔式”金矿的地质-地球物理-地球化学找矿模型。 相似文献
79.
夏季西风带定常扰动对东北亚阻塞高压的影响 总被引:6,自引:4,他引:6
利用ECMWF 1980~1988年9年的格点资料,分析了定常扰动与东北亚阻塞高压之间的关系。分析结果表明:定常扰动的分布对阻塞高压维持日数有着重要的影响,定常扰动的季节变化可以很好地说明阻塞高压冬季多在太平洋和大西洋上发生和维持,而夏季多在东北亚地区发生和维持的特征。此外,从定常扰动的分布可以看到,不仅中高纬地区上空的正距平强度可以影响着阻塞高压的发生和维持,其南侧的负距平强度也同样重要地影响着阻塞高压。分析结果还表明:不仅定常扰动的水平结构对阻高有着重要影响,其垂直结构亦有着重要影响。最后,对夏季定常扰动进行了波数域分析,表明在夏季定常扰动的作用主要通过其中所包含的行星波、特别是行星波1波来实现,定常扰动中行星波部分的振幅变化是影响阻塞高压发生和维持的重要物理机制。 相似文献
80.