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101.
合成孔径雷达干涉测量(InSAR)在地面形变监测中的应用 总被引:13,自引:0,他引:13
运用合成孔径雷达干涉及其差分技术(InSAR及D-InSAR)进行地面微位移监测,是近年来发展起来并得到日益重视的新方法。对不同地区地面形变的最新研究结果表明,合成孔径雷达干涉及其差分技术在地震形变、冰川运移、活动构造、地面沉降及滑坡等研究与监测中有广阔的应用前景,具有不可替代的优势。 与其它方法(如GPS监测等)相比,用InSAR及D-InSAR进行地面形变监测的主要优点在于:(1)覆盖范围大,方便迅速:(2)成本低,不需要建立监测网;(3)空间分辨率高,可以获得某一地区连续的地表形变信息;(4)可以监测或识别出潜在或未知的地面形变信息:(5)全天候,不受云层及昼夜影响。但是由于系统本身因素以及地面植被、湿度及大气条件变化的影响,精度及适用性受到一定的限制,需要在实践中不断加以完善和提高,并与地质研究及其它方法相结合。 为了弥补传统InSAR及D-InSAR方法在地面形变监测方面的不足,提高其精度,近期引入了一种称为永久散射点(PS)的方法。此方法通过选取一定时期内表现出稳定干涉行为的孤立点,克服了许多妨碍传统雷达干涉技术的分辨率、空间及时间上基线限制等问题,使InSAR在城市及岩石出露较好地区地面形变监测精度大大提高,在一定的条件下精度可达到mm级。 相似文献
102.
103.
Onno R. Pols Klaus-Peter Schro¨der Jarrod R. Hurley Christopher A. Tout & Peter P. Eggleton 《Monthly notices of the Royal Astronomical Society》1998,298(2):525-536
We have calculated a grid of empirically well tested evolutionary tracks with masses M between 0.5 and 50 M⊙, spaced by approximately 0.1 in log M , and with metallicities Z = 0.0001, 0.0003, 0.001, 0.004, 0.01, 0.02 and 0.03. We use a robust and fast evolution code with a self-adaptive non-Lagrangian mesh, which employs the mixing-length theory but treats convective mixing as a diffusion process, solving simultaneously for the structure and the chemical composition. The hydrogen and helium abundances are chosen as functions of the metallicity: X = 0.76 − 3.0 Z Y = 0.24 + 2.0 Z . Two sets of models were computed, one without and one with a certain amount of enhanced mixing or 'overshooting'. This amount has been empirically chosen by means of various sensitive tests for overshooting: (1) the luminosity of core helium burning (blue loop) giants of well-known mass, (2) the width of the main sequence as defined by double-lined eclipsing binaries with well-measured masses and radii, and (3) the shape and implied stellar distribution of isochrones of various open clusters. The first two tests have been the subject of previous papers, the third test is discussed in this paper. On the basis of these tests, we recommend the use of the overshooting models for masses above about 1.5M ⊙. We describe here the characteristics of the models, the procedure for constructing isochrones for arbitrary age and metallicity from the models, and the performance of these isochrones for several intermediate-age and old open clusters. All original models are available in electronic form and we describe the means by which they may be obtained. 相似文献
104.
C. J. Phillips R. P. Norris S. P. Ellingsen & P. M. McCulloch 《Monthly notices of the Royal Astronomical Society》1998,300(4):1131-1157
We have used the Australia Telescope Compact Array (ATCA) to make high-resolution images of the 6.7-GHz 51 → 60 A+ maser transition of methanol towards 33 sources in the Galactic plane. Including the results from 12 methanol sources in the literature, we find that 17 out of 45 sources have curved or linear morphology. Most of the 17 have a velocity gradient along the line, which is consistent with masers lying in an edge-on circumstellar disc surrounding a massive star. We also made simultaneous continuum observations of the sources at 8.6 GHz, in order to image any associated H ii region. 25 of the sources are associated with an ultracompact H ii region, with a detection limit of ∼0.5 mJy beam−1 . We argue that the methanol sources without an associated H ii region represent less massive embedded stars, not an earlier stage in the lifetime of the star, as previously suggested. 相似文献
105.
Noah Brosch Ana Heller & Elchanan Almoznino 《Monthly notices of the Royal Astronomical Society》1998,300(4):1091-1097
The location of H II regions, which indicates the locus of present star formation in galaxies, is analysed for a large collection of 110 irregular galaxies (Irr) imaged in Hα and nearby continuum. The analysis is primarily by visual inspection, although a two-dimensional quantitative measure is also employed. The two different analyses yield essentially identical results. H II regions appear preferentially at the edges of the light distribution, predominantly on one side of the galaxy, contrary to what is expected from stochastic self-propagating star formation scenarios. This peculiar distribution of star-forming regions cannot be explained by a scenario of star formation triggered by an interaction with extragalactic gas, or by a strong one-armed spiral pattern. 相似文献
106.
Zhang?MeiliangEmail author Yuan?Daoxian Lin?Yushi Cheng?Hai Qin?Jiaming Zhang?Huiling 《中国科学D辑(英文版)》2004,47(1):1-12
A high-resolution climate record from 163.00 kaBP to 113.80 kaBP has been obtained through TIMS-U series dating and carbon
and oxygen isotope analysis of the three large stalagmites from two caves in the south of Guizhou Province, China. The record
of the oxygen isotopes from the stalagmites reveals that the undulation characteristics between the cooling event of the glacial
period and the warming event of the interglacial period in the research area can compare well to those of ice cores, lake
sediments, loess and deep sea sediments on the scale of ten-thousand years or millennium time scale. The climate undulation
provided by the record of the stalagmites has a coherence with the global changes and a tele-connection to the paleoclimate
changes in the north polar region. Our results suggest that the direct dynamics of paleo-monsoon circulation changes reflected
in the record of the stalagmites might be caused by changes of the global ice volume, and in turn related to various factors,
including the solar radiation strength at the mid-latitudes in the Northern Hemisphere, the southern extension of the ice-rafted
event in the North Atlantic, and changes of the equatorial Pacific sea surface temperature at the low-latitudes. Using °18O values, we have calculated the temperatures and the results show that the temperature difference between the penultimate
glacial period (with an average temperature of 8.1°C, and a minimum temperature range from 0.65°C to-1.43°C at stage 6) and
the last interglacial period (with an average temperature of 18.24°C at sub-stage 5e) was about 10°C. This temperature difference
from the record of the stalagmites corresponds in general to the record temperature variation (about 10°C) of measured ice
cores. The climate records from the three stalagmites in the two caves have shown that the circulation strength of the Asian
summer monsoon and the winter monsoon in the penultimate glacial period and the last inter-glacial period had a clear change.
With the TIMS-U series method, termination II of the penultimate glacial period has been precisely dated at an age of (129.28±
1.10) kaBP for the three stalagmites in the south of Guizhou Province, China. This borderline age represents the beginning
of the last interglacial period or the boundary between the Middle Pleistocene and the Late Pleistocene, and corresponds to
the beginning age of the last interglacial period shown by the ice cores and in the SPECMAP curve of the marine oxygen isotopes.
The chronology determination of termination II is not only of stratigraphic and chronological significance, but also lays
an important foundation for discussing the short time scales of climate oscillation and rapidly changing events of paleoclimate
in the circulation region of the East Asian monsoon. 相似文献
107.
基于出版的地图符号库系统的建立 总被引:2,自引:1,他引:2
提出并解决了基于出版的地图符号库需要解决的关键技术:符号制作软件的设计、符号与属性库的连接、RGB色彩到CMYK色彩的转换、基于出版的地图符号分层、PS文件的生成;在此基础上论述了全数字出版系统中建立地图符号库系统的方法。 相似文献
108.
109.
太平洋岛国对澳大利亚地缘战略影响的历史考察 总被引:1,自引:1,他引:0
历史上太平洋岛国对澳大利亚地缘战略的影响以第二次世界大战为分水岭,主要分为三个阶段:二战前是地缘战略缺失阶段,当时澳大利亚无视周边地缘环境,将国家安全系于遥远英帝国的庇护,忽视近邻岛屿的防御屏障作用,导致国家遭受战火;二战时期是地缘战略构建阶段,随着澳美战时同盟成立,太平洋上的海空航线成为澳大利亚的“生命线”,澳大利亚的独立防务意识也不断加强,意图凭借《澳新协定》将太平洋岛国纳入势力范围;二战后是地缘战略丰富阶段,在太平洋岛国发展问题日益突出和岛屿地区安全态势日趋复杂的背景下,澳大利亚实施援助战略以促进地区的繁荣与稳定。未来,澳大利亚将继续保持该地区最大援助国的地位。 相似文献
110.