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51.
用固相反应法和sol-gel法合成了不同类型的磷灰石(AP),并采用TEM、XRD、IR、BET比表面积法及静、动态吸附等方法研究了不同AP的比表面积、结晶度、晶胞参数、结晶尺寸、晶格缺陷度、Ca/P摩尔比和煅烧温度等与吸氟能力的关系,结果表明:结晶度高、晶粒大的AP有较小的吸氟量,属表面单分子层化学络合吸附机理;酸活化的AP有较大的吸氟量,属溶解-沉淀与沉淀物表面纳米尺寸效应吸附的复合去氟机理;具纳米尺寸的HAP在常温、常压、无二次污染、小于11mg/L的低含氟浓度废水中且不酸化情况下有较大吸氟量,属纳米尺寸效应吸附机理。 相似文献
52.
53.
Żaneta Polkowska Aleksander Astel Marzena Grynkiewicz Tadeusz Górecki Jacek Namieśnik 《Journal of Atmospheric Chemistry》2002,41(3):239-264
The paper presents monitoring results and environmental pollution assessment for the Gdask-Sopot-Gdynia Tricity (Poland), based onanalysis of precipitation. Precipitation samples were collected over a period of 12 months (January–December 1998) at ten locations in the Tricity. The following selected ions were determined in the samples:SO4
2–, F–, Cl–, NO3
–,PO4
3–, NH4
+, Na+,Mg2+, Ca2+, K+. The results were subjected to full statistical evaluation. Values of the parameters determined were correlated with each other. An attempt was made to explain co-occurrences of certain ions and the significance of their mutual effects. Pollutant concentrations and loads in precipitation were also correlated with data on wind direction and temperature in the region.Deposition of pollutants was very high in spring due to the prevailing air circulation patterns and low temperatures. Analysis of the correlations between co-occurring ions confirmed the significant impact of the location (sea coast) on the composition of rain water. Ionic ratios in rainwater were similar to those observed for sea salt samples. In addition, heavy traffic was most probably responsible for high concentrations of various forms of nitrogen and sulphates in the vicinity of major highways. 相似文献
54.
微波辅助提取-氢化物发生原子荧光光谱法测定土壤中无机砷 总被引:1,自引:1,他引:1
建立了微波辅助提取-氢化物发生原子荧光光谱法测定土壤中无机砷的分析方法。用正交试验设计结合单因素试验优化了样品粒度、提取温度、提取时间、固液比等微波提取条件,研究了共存离子对无机砷测定的干扰情况。方法的线性范围为0.25~40.0μg/g,无机砷的检出限为0.05μg/g,样品加标回收率为92.9%~105.0%。方法的精密度(RSD,n=11)为0.3%。与水浴提取法相比,微波辅助提取法具有快速、高效的优势。方法已用于分析3个不同产地有代表性土壤中无机砷含量。 相似文献
55.
The role of silicate and carbonate weathering in contributing to the major cation and Sr isotope geochemistry of the headwaters
of the Ganga-Ghaghara-Indus system is investigated from the available data. The contributions from silicate weathering are
determined from the composition of granites/ gneisses, soil profiles developed from them and from the chemistry of rivers
flowing predominantly through silicate terrains. The chemistry of Precambrian carbonate outcrops of the Lesser Himalaya provided
the data base to assess the supply from carbonate weathering. Mass balance calculations indicate that on an average ∼ 77%
(Na + K) and ∼ 17% (Ca + Mg) in these rivers is of silicate origin. The silicate Sr component in these waters average ∼40%
and in most cases it exceeds the carbonate Sr. The observations that (i) the87Sr/86Sr and Sr/Ca in the granites/gneisses bracket the values measured in the head waters; (ii) there is a strong positive correlation
between87Sr/86Sr of the rivers and the silicate derived cations in them, suggest that silicate weathering is a major source for the highly
radiogenic Sr isotope composition of these source waters. The generally low87Sr/86Sr (< 0.720) and Sr/Ca (∼ 0.2 nM/ μM) in the Precambrian carbonate outcrops rules them out as a major source of Sr and87Sr/86Sr in the headwaters on a basin-wide scale, however, the high87Sr/86Sr (∼ 0.85) in a few of these carbonates suggests that they can be important for particular streams. The analysis of87Sr/86Sr and Ca/Sr data of the source waters show that they diverge from a low87Sr/86Sr and low Ca/Sr end member. The high Ca/Sr of the Precambrian carbonates precludes them from being this end member, other
possible candidates being Tethyan carbonates and Sr rich evaporite phases such as gypsum and celestite. The results of this
study should find application in estimating the present-day silicate and carbonate weathering rates in the Himalaya and associated
CO2 consumption rates and their global significance. 相似文献
56.
本文运用磁场的最小方差分析法和磁场-电子密度的相关分析法分析了欧洲空间局Giotto飞船对P/Grigg-Skjellerup(简称G-S)彗星弓激波附近磁场和电子能流的部分观测数据.结果表明彗星附近存在大量的频率靠近新生水族离子回旋频率的波动,它们是由彗星新生水族离子环流激发的低频左旋电磁波.波在近似平行于磁场方向传播,斜传播角小于15°.电子数据和磁场数据相关分析表明即使在离彗星很远的地方仍然存在压缩波. 相似文献
57.
Sven Israelsson 《Pure and Applied Geophysics》1977,115(3):561-574
The standard deviations and time-spectra of small ion number density have been measured at ground level under different atmospheric stability conditions. The auto-correlation correlograms and the time-spectra imply a scale of fluctuations corresponding to 1 to 4 min. No clear relationships between standard deviations of small ion number density and micro-meteorological parameters are observed. Thus the results are not a support for Monin-Obukhov similarity theory. For the highest frequencies the slopes of the spectra seem to follow the –5/3-law fairly well and the frequencies of the peak values of individual spectra lnfS(f) increase when the atmosphere stability increases, which is valid for ordinary micrometeorological parameters. 相似文献
58.
春季水华对南黄海总溶解态无机砷生物地球化学行为的影响 总被引:1,自引:0,他引:1
利用氢化物发生-原子荧光光谱法(HG-AFS)对2007年3月30日至4月23日南黄海海域总溶解态无机砷(TDIAs,[TDIAs]=[As5+]+[As3+])的含量进行了测定,其中针对水华中心区域(BM1站)进行了25h的连续观测,以探讨春季水华对有毒类金属元素砷的生物地球化学行为的影响。结果表明,TDIAs的浓度范围为7.9~22.3nmol/L,平均值为(17.8±1.9)nmol/L。TDIAs在南黄海的分布主要表现为由近岸向外海逐渐升高的趋势,最大值出现在南部海域底层海水中。近岸海域表、底层TDIAs的含量相当,而中、南部海域由于存在明显的密度跃层,表、底层TDIAs的浓度具有显著性差异。2007年3月31日至4月1日研究区域西南部受到沙尘天气和降雨的影响,表层海水中TDIAs的含量显著升高。研究区域中、南部海域在观测期间暴发了典型的黄海春季水华,通过大面观测和对重点区域的连续观测可以发现,水华期间TDIAs的分布和磷酸盐类似,与Chl a呈现出较好的负相关关系(r=0.51,P0.05,n=39)。经初步计算,浮游植物水华对10m以上表层水体中TDIAs的清除量约为2.4nmol/L,占表层保有量的15%左右。通过箱式模型计算得出黄海TDIAs的停留时间约为(18.2±8.5)a,远远低于大洋。通过对该海域砷、磷摩尔比值的计算可以发现,南黄海砷、磷摩尔比值约为大洋中的20倍左右,这可能会引起浮游生物对砷酸盐的大量吸收和转化,从而带来潜在的生态危机,需要引起足够的重视。 相似文献
59.
60.
Spatial and seasonal variation of major ions in Himalayan snow and ice: A source consideration 总被引:2,自引:0,他引:2
The spatial and temporal variation of major ions (Ca2+, Mg2+, Na+, K+, , , and Cl−) in Himalayan snow and ice is investigated by using two snow pits from the East Rongbuk glacier (28°01′N, 86°58′E, 6500 m a.s.l.), one snow pit from the Nangpai Gosum glacier (28°03′N, 86°39′E, 5700 m a.s.l.), one snow pit from the Gyabrag glacier (28°11′N, 86°38′E, 6303 m a.s.l.), and three ice cores from the Sentik (35°59′N, 75°58′E, 4908 m a.s.l.), Dasuopu (28°33′N, 85°44′E, 7000 m a.s.l.), and East Rongbuk (27°59′N, 86°55′E, 6450 m a.s.l.) glaciers, respectively. In general, the major ions show a significant seasonal variation, with high concentrations during the non-monsoon (pre-monsoon and post-monsoon) season and relatively low concentrations during the monsoon season. Monsoon precipitation with high local/regional dust loading related to summer circulation is possibly responsible for the high concentrations occurring sporadically during the monsoon season. The crest of the Himalayas is an effective barrier to the spatial distribution of Na+, Cl− and concentrations, but not to the major ions associated with dust influx (e.g. Ca2+ and Mg2+). Atmospheric backward trajectories from the HYSPLIT_4 model used in identifying chemical species sourcing suggest that the major ions in the Himalayan snow and ice come mainly from the Thar Desert located in the North India, as well as West Asia, or even the distant Sahara Desert in the North Africa during the winter and spring seasons. This is different from the conventionally assumed arid and semi-arid regions of the central Asia. Factors, such as different vapor sources due to atmospheric circulation patterns and geographical features (e.g. altitude, topography), may contribute to the differences in major ionic concentrations between the western and eastern Himalayas. 相似文献