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901.
Wavelet Analysis of Several Important Periodic Properties in the Relative Sunspot Numbers 总被引:8,自引:0,他引:8
Gui-Ming Le Jia-Long Wang Center for Space Science Applied Research Chinese academy of Sciences Beijing lgm National Astronomical Observatories Chinese Academy of Sciences Beijing 《中国天文和天体物理学报》2003,3(5):391-394
We investigate the wavelet transform of yearly mean relative sunspot number series from 1700 to 2002. The curve of the global wavelet power spectrum peaks at 11-yr, 53-yr and 101-yr periods. The evolution of the amplitudes of the three periods is studied. The results show that around 1750 and 1800, the amplitude of the 53-yr period was much higher than that of the the 11-yr period, that the ca. 53-yr period was apparent only for the interval from 1725 to 1850, and was very low after 1850, that around 1750, 1800 and 1900, the amplitude of the 101-yr period was higher than that of the 11-yr period and that, from 1940 to 2000, the 11-yr period greatly dominates over the other two periods. 相似文献
902.
系统聚类方法在房地产周期分析中的应用 总被引:1,自引:0,他引:1
选取了9项房地产经济波动指标,经过相关性分析,确定房地产经济综合指标体系,并运用聚类分析方法对我国房地产经济波动进行了分析,为进一步分析研究我国房地产周期提供了方法和手段。 相似文献
903.
We have obtainedK-band imaging observations of Gamma-Ray Burst (GRB) host galaxies with the near-infrared spectro-imager ISAAC installed on
the Very Large Telescope at Paranal (Chile). The derivedK magnitudes, combined with other photometric data taken from the literature, are used to investigate theR-K colors of GRB hosts. We do not find any extremely reddened starbursts in our sample, despite the capability of GRBs to trace
star formation even in dusty regions. The observedR-K colors are on the contrary typical of irregular and spiral blue galaxies at high redshift. 相似文献
904.
905.
906.
The amino acid and hydrocarbon contents of the Paris meteorite: Insights into the most primitive CM chondrite
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Zita Martins Paola Modica Brigitte Zanda Louis Le Sergeant d'Hendecourt 《Meteoritics & planetary science》2015,50(5):926-943
The Paris meteorite is one of the most primitive carbonaceous chondrites. It is reported to be the least aqueously altered CM chondrite, and to have experienced only weak thermal metamorphism. We have analyzed for the first time the amino acid and hydrocarbon contents of this pristine meteorite by gas chromatography–mass spectrometry (GC–MS). When plotting the relative amino acids abundances of several CM chondrites according to the increasing hydrothermal scale (petrologic subtypes), from the CM2.7/2.8 Paris to the CM2.0 MET 01070, Paris has the lowest relative abundance of β‐alanine/glycine (0.15), which fits with the relative abundances of β‐alanine/glycine increasing with increasing aqueous alteration for CM chondrites. These results confirm the influence of aqueous alteration on the amino acid abundances and distribution. The amino acid analysis shows that the isovaline detected in this meteorite is racemic (d /l = 0.99 ± 0.08; l ‐enantiomer excess = 0.35 ± 0.5%; corrected d /l = 1.03; corrected l ‐enantiomer excess = ?1.4 ± 2.6%). The identified hydrocarbons show that Paris has n‐alkanes ranging from C16 to C25 and 3‐ to 5‐ring nonalkylated polycyclic aromatic hydrocarbons (PAHs). The lack of alkylated PAHs in Paris seems to be also related to this low degree of aqueous alteration on its parent body. The extraterrestrial hydrocarbon content, suggested by the absence of any biomarker, may well have a presolar origin. The chemistry of the Paris meteorite may thus be closely related to the early stages of the solar nebula with a contribution from interstellar (molecular cloud) precursors. 相似文献
907.
In order to derive the distribution of olivine and pyroxene in Crater Copernicus,we compute two band ratios(950/750 and 2 000/1 500 nm) ,percent content of elements(Al%,Ca%,Mg%,FeO%) and maturity(Is/FeO) based on Clementine UVVIS and NIR image data.The central peaks of Copernicus,which are known to be olivine-rich or pyroxene-rich,are chosen as ground truth and ROIs used to derive the distribution of olivine and pyroxene with a decision tree and spectral angle mapper(SAM) .Additionally,we compared previous ... 相似文献
908.
E. M. Blanter J.-L. Le Mouél M. G. Shnirman V. Courtillot 《Doklady Earth Sciences》2011,440(1):1316-1319
This paper describes seasonal peculiarities of modern climate warming in the European region. It is shown that warming scenarios
considerably differ in cold and warm periods of the year. The warming is accompanied with growth and considerable change in
the phase of the yearly cycle in solarity data. A strong half-year cycle is recognized in seasonal variation of long-term
trends over the last few years. Peculiarities of climate change in Europe and the increased influence of the tropics are discussed
in view of the results obtained. 相似文献
909.
910.
Jean-Charles Poilvet Marc Poujol Pavel Pitra Jean Van Den Driessche Jean-Louis Paquette 《Comptes Rendus Geoscience》2011,343(7):454-461
Dating the magmatism in the Montagne Noire gneiss dome in the southern French Massif Central is a key point for understanding the Late Palaeozoic evolution of this part of the Variscan belt, which is characterised by compressive tectonics during the Carboniferous and extensional tectonics during Stephanian-Permian times. The Montalet granite crops out in the north-western part of the dome and was first considered as an early syntectonic intrusion related to compressive deformation. More recently, it has been dated at 327 Ma and considered as contemporaneous with the diapiric ascent of the Montagne Noire gneiss dome before the Stephanian-Permian extension. We show that in fact, this pluton was emplaced 294 ± 1 Ma ago and is therefore contemporaneous with the Stephanian-Permian extension. This age is consistent with the interpretation of the Montagne Noire Massif as an extensional gneiss dome. 相似文献