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931.
Ocean Science Journal - Clove oil (CO) is an effective anesthetic. Many hatcheries and research studies use clove oil to immobilize fish for artificial reproduction and surgery to suppress their... 相似文献
932.
Roger G. Young Aaron J. Quarterman Rebekah F. Eyles Robert A. Smith William B. Bowden 《新西兰海洋与淡水研究杂志》2013,47(4):803-825
We examined the effects of land use, geology, and longitudinal position within the river network on water quality and thermal regime at 23 sites within the Motueka River catchment. The concentrations of suspended solids, nitrate nitrogen, total nitrogen, Escherichia coli, and Campylobacter were higher at sites draining pastoral and horticultural land than in similar‐sized native or plantation forest streams. Average daily mean temperature and minimum temperature in summer and maximum winter temperature were higher in unshaded pastoral and horticultural streams than at native forest sites. Differences in water quality and thermal regime were also observed among sites with contrasting geology. Conductivity, pH, and minimum winter temperatures were highest at sites draining marble terrain. In contrast, longitudinal patterns in water quality and temperature regime along the 120‐km length of the river were relatively weak, although longitudinal patterns in amplitude of daily temperature fluctuation matched theoretical predictions. In this study, differences in land use appeared to have the strongest influence on most water quality and thermal variables examined. However, geology was an important factor explaining variation in certain variables (e.g., pH and conductivity). Longitudinal patterns in water quality and temperature were relatively weak and in many instances were linked with longitudinal patterns in land use and geology rather than catchment location alone. 相似文献
933.
Nak Won Heo Sang Hee Hong Gi Myung Han Sunwook Hong Jongmyoung Lee Young Kyung Song Mi Jang Won Joon Shim 《Ocean Science Journal》2013,48(2):225-233
The spatial distribution of small plastic debris on Heungnam beach in February 2011 was investigated. The abundances of small plastic debris over 2 mm in size along the high strandline and cross-sectional line of the beach were determined. The mean abundances of small plastics were 976 ± 405 particles/m2 at the high strandline in the upper tidal zone along the shoreline and 473 ± 866 particles/m2 at the cross-section perpendicular to the shoreline. Specifically, styrofoam (expanded polystyrene) spherules accounted for 90.7% of the total plastic abundance in the high strandline and 96.3% in the cross-section. The spatial distribution patterns of small plastic debris differed between the high strandline and cross-sectional line. The cross-sectional distribution of small plastic abundance differed among plastic types, indicating that representative sampling of small plastic debris on a beach is necessary. 相似文献
934.
Chang-Woong Shin Sang-Kyung Byun Cheolsoo Kim Jae Hak Lee Bong-Chae Kim Sang-Chull Hwang Young Ho Seung Hong-Ryeol Shin 《Ocean Science Journal》2013,48(1):35-47
Seasonal variations in the low-salinity intermediate water (ESIW) in the region south of the sub-polar front of the East Sea were investigated by using historical hydrographic data. The salinity of the representative density (sigma-0=27.2) of the ESIW was minimal in summer and maximal in winter in the region south of the sub-polar front. The selected four subregions showed different salinity variations. In the west of Oki Spur and the Yamato Basin, salinity fluctuated similarly, with a minimum during summer. In the Ulleung Basin and northwest of Sado Island, however, variations in salinity showed two minima, one is in winter and the other is in summer. These results imply differences in the flow path of the ESIW into the region south of the sub-polar front over time. 相似文献
935.
Z. Bebesi K. Szego A. Balogh N. Krupp G. Erdos A.M. Rymer G.R. Lewis W.S. Kurth D.T. Young M.K. Dougherty 《Planetary and Space Science》2011,59(5-6):445-446
Hubert and Samsonov addressed our paper published in early 2010 (Bebesi et al., 2010) about a plasma event detected in the magnetosheath of Jupiter by the plasma instruments of the Cassini spacecraft. We proposed that the characteristics of the plasma parameter variations were consistent with a slow mode shock (SMS). As our title indicated, we claimed only that the event was a possible “candidate” for an SMS according to our data, which had some restrictions as discussed in the paper. As to the origin, we proposed the following: since there was a crossing of the then highly tilted Heliospheric Current Sheet in less than two days before the event, it might have played a role in initiating the shock front.We highly appreciate the opinion of the authors, but they do not point out any hard fact that would exclude the possibility of the scenario we suggested. 相似文献
936.
C. C. Kuranz H.-S. Park B. A. Remington R. P. Drake A. R. Miles H. F. Robey J. D. Kilkenny C. J. Keane D. H. Kalantar C. M. Huntington C. M. Krauland E. C. Harding M. J. Grosskopf D. C. Marion F. W. Doss E. Myra B. Maddox B. Young J. L. Kline G. Kyrala T. Plewa J. C. Wheeler W. D. Arnett R. J. Wallace E. Giraldez A. Nikroo 《Astrophysics and Space Science》2011,336(1):207-211
The National Ignition Facility (NIF) is capable of creating new and novel high-energy-density (HED) systems relevant to astrophysics. Specifically, a system could be created that studies the effects of a radiative shock on a hydrodynamically unstable interface. These dynamics would be relevant to the early evolution after a core-collapse supernova of a red supergiant star. Prior to NIF, no HED facility had enough energy to perform this kind of experiment. The experimental target will include a 340 ??m predominantly plastic ablator followed by a low-density SiO2 foam. The interface will have a specific, machined pattern that will seed hydrodynamic instabilities. The growth of the instabilities in a radiation-dominated environment will be observed. This experiment requires a ??300?eV hohlraum drive and will be diagnosed using point projection pinhole radiography, which have both been recently demonstrated on NIF. 相似文献
937.
Peng K. Hong Seiji Sugita Yasuhito Sekine Naruhisa Takatoh Tetsuharu Fuse Hideyo Kawakita Eliot F. Young Kosuke Kurosawa Junichi Haruyama Toshihiko Kadono Shunichi Kamata Tomohiko Sekiguchi Hirotomo Noda 《Icarus》2011,214(1):21-29
The Lunar Crater Observation and Sensing Satellite (LCROSS) mission was an impact exploration searching for a volatile deposit in a permanently shadowed region (PSR) by excavating near-surface material. We conducted infrared spectral and imaging observations of the LCROSS impacts from 15 min before the first collision through 2 min after the second collision using the Subaru Telescope in order to measure ejecta dust and water. Such a ground-based observation is important because the viewing geometry and wavelength coverage are very different from the LCROSS spacecraft. We used the Echelle spectrograph with spectral resolution λ/Δλ ∼ 10,000 to observe the non-resonant H2O rotational emission lines near 2.9 μm and the slit viewer with a K′ filter for imaging observation of ejecta plumes. Pre-impact calculations using a homogeneous projectile predicted that 2000 kg of ejecta and 10 kg of H2O were excavated and thrown into the analyzed area immediately above the slit within the field of view (FOV) of the K′ imager and the FOV of spectrometer slit, respectively. However, no unambiguous emission line of H2O or dust was detected. The estimated upper limits of the amount of dust and H2O from the main Centaur impact were 800 kg and 40 kg for the 3σ of noise in the analyzed area within the imager FOV and in the slit FOV, respectively. If we take 1σ as detection limit, the upper limits are 300 kg and 14 kg, respectively. Although the upper limit for water mass is comparable to a prediction by a standard theoretical prediction, that for dust mass is significantly smaller than that predicted by a standard impact theory. This discrepancy in ejecta dust mass between a theoretical prediction and our observation result suggests that the cratering process induced by the LCROSS impacts may have been substantially different from the standard cratering theory, possibly because of its hollow projectile structure. 相似文献
938.
Mechanisms driving polymagmatic activity at a monogenetic volcano, Udo, Jeju Island, South Korea 总被引:3,自引:1,他引:2
Marco Brenna Shane J. Cronin Ian E. M. Smith Young Kwan Sohn Karoly Németh 《Contributions to Mineralogy and Petrology》2010,160(6):931-950
High-resolution, stratigraphically ordered samples of the Udo tuff cone and lava shield offshore of Jeju Island, South Korea,
show complex geochemical variation in the basaltic magmas that fed the eruption sequence. The eruption began explosively,
producing phreatomagmatic deposits with relatively evolved alkali magma. The magma became more primitive over the course of
the eruption, but the last magma to be explosively erupted had shifted back to a relatively evolved composition. A separate
sub-alkali magma batch was subsequently effusively erupted to form a lava shield. Absence of weathering and only minor reworking
between the tuff and overlying lava implies that there was no significant time break between the eruptions of the two magma
batches. Modelling of the alkali magma suggests that it was generated from a parent melt in garnet peridotite at c. 3 to 3.5 GPa
and underwent mainly clinopyroxene + olivine ± spinel fractionation at c. 1.5 to 2 GPa. The sub-alkali magma was, by contrast,
generated from a chemically different peridotite with residual garnet at c. 2.5 GPa and evolved through olivine fractionation
at a shallower level compared to its alkali contemporary. The continuous chemostratigraphic trend in the tuff cone, from relatively
evolved to primitive and back to evolved, is interpreted to have resulted from a magma batch having risen through a single
dyke and erupted the batch’s head, core and margins, respectively. The alkali magma acted as a path-opener for the sub-alkali
magma. The occurrence of the two distinct batches suggests that different magmatic systems in the Jeju Island Volcanic Field
have interacted throughout its history. The polymagmatic nature of this monogenetic eruption has important implications for
hazard forecasting and for our understanding of basaltic field volcanism. 相似文献
939.
Abstract: To determine the geochemical characteristics of the Imgok creek impacted by acid mine drainage (AMD) generated from the abandoned Youngdong coal mine in Korea, chemical analyses of water samples and precipitates and the geochemical modelling of the precipitates were conducted. Acid mine drainage drained from the mine adit and coal refuse piles shows a low pH, high conductivity and high concentrations of Fe, Al, SO4 and heavy metals such as Co, Cu, Ni and Zn. In the Imgok creek, the concentrations of heavy metals and major cations besides Fe are decreased by dilution, but concentrations of Fe are decreased by the formation of precipitates as well as dilution. From the results of geochemical modelling, goethite is oversaturated, and schwertmannite is the most stable solid phase in the Imgok creek. Yellowish red Fe-precipitates collected at the Imgok creek are recognized as amorphous or poorly crystallized minerals from XRD patterns and Feox /Fetot ratios, and as containing chemically bonded SO4 and OH by an IR analysis. The mole ratios of Fe/S in these precipitates, which are determined by EPMA, are 5. 1 and 6. 1. 相似文献
940.
南昌市青年气象志愿者专题小组 《气象与减灾研究》2002,25(1):43-46
通过对南昌市区和城郊1个月的对比观测与分析,发现了造成南昌市盛夏城区最高气温比城郊高的一些原因,并对南昌市盛夏高温预报服务提出了参考建议。 相似文献