全文获取类型
收费全文 | 2319篇 |
免费 | 473篇 |
国内免费 | 570篇 |
专业分类
测绘学 | 112篇 |
大气科学 | 488篇 |
地球物理 | 569篇 |
地质学 | 1249篇 |
海洋学 | 243篇 |
天文学 | 155篇 |
综合类 | 233篇 |
自然地理 | 313篇 |
出版年
2024年 | 2篇 |
2023年 | 46篇 |
2022年 | 138篇 |
2021年 | 145篇 |
2020年 | 100篇 |
2019年 | 117篇 |
2018年 | 165篇 |
2017年 | 140篇 |
2016年 | 153篇 |
2015年 | 124篇 |
2014年 | 155篇 |
2013年 | 139篇 |
2012年 | 134篇 |
2011年 | 133篇 |
2010年 | 148篇 |
2009年 | 118篇 |
2008年 | 116篇 |
2007年 | 84篇 |
2006年 | 72篇 |
2005年 | 74篇 |
2004年 | 38篇 |
2003年 | 61篇 |
2002年 | 44篇 |
2001年 | 43篇 |
2000年 | 73篇 |
1999年 | 110篇 |
1998年 | 92篇 |
1997年 | 90篇 |
1996年 | 91篇 |
1995年 | 94篇 |
1994年 | 66篇 |
1993年 | 63篇 |
1992年 | 42篇 |
1991年 | 28篇 |
1990年 | 20篇 |
1989年 | 23篇 |
1988年 | 21篇 |
1987年 | 11篇 |
1986年 | 12篇 |
1985年 | 9篇 |
1984年 | 5篇 |
1983年 | 8篇 |
1982年 | 5篇 |
1981年 | 2篇 |
1980年 | 1篇 |
1979年 | 3篇 |
1976年 | 2篇 |
1958年 | 2篇 |
排序方式: 共有3362条查询结果,搜索用时 31 毫秒
71.
近20年京津唐主体城区地表热场空间特征变化分析 总被引:3,自引:1,他引:2
基于Landsat遥感影像获取京津唐主体城区1995~2015年地表温度(Land Surface Temperature, LST)和不透水地表盖度(Impervious Surface Percentage, ISP)数据。采用热点聚集和阈值分割法,依据地表的温度和不透水盖度属性将京津唐主体城区划分成9种地表热场类型,分析并探讨地表热场的发展规律、年际变化状况和区域贡献作用。研究发现,京津唐主体城区地表温度与不透水地表盖度间存在显著的正向相关关系,两者分别呈现“阶梯降”和“两端高、中间低”的变化特征。京津唐主体城区地表热场的发展主轴保持在西北-东南方向,且随时间推移沿主轴呈聚集态势。 京津唐主体城区地表热场的影响范围在空间上持续扩张,对于不同的主体城区,其在整体区域的热场贡献中有差异化表现。 相似文献
72.
This paper studies negative bias temperature instability (NBTI) under alternant and alternating current (AC) stress. Under alternant stress, the degradation smaller than that of single negative stress is obtained. The smaller degradation is resulted from the recovery of positive stress. There are two reasons for the recovery. One is the passivation of H dangling bonds, and another is the detrapping of charges trapped in the oxide. Under different frequencies of AC stress, the parameters all show regular degradation, and also smaller than that of the direct current stress. The higher the frequency is, the smaller the degradation becomes. As the negative stress time is too small under higher frequency, the deeper defects are hard to be filled in. Therefore, the detrapping of oxide charges is easy to occur under positive bias and the degradation is smaller with higher frequency. 相似文献
73.
Light curves are usually constructed from discrete observational data by interpolation. In most cases, the observation data is temporally uneven, and therefore the light curve is usually derived by the interpolation of the binned data with the spline function, which is intended for reducing the “high sample noise” (i.e., the variability in the timescales comparable with the bin width). Such a practice of course reduces the time resolution of the light curve. It is known that function approximation is one of the most important applications of the artificial neural networks (ANN). In this work, for the first time we tentatively use the ANN to construct light curves from unevenly sampled variability data. To demonstrate the advantages of ANN for signal reconstruction over commonly used cubic spline function scheme, two sets of simulated periodic functions are used with random noises of varying magnitudes, one single frequency based and one multiple (two) frequency based. These signal reconstruction tests show that the ANN is clearly superior to the cubic spline scheme. As a case study, we use the uneven long-term multi-band monitoring data of BL lacertae to derive the light curves with ANN. It is found that the light curves derived with ANN have higher time resolution than those with the cubic spline function adopted in previous works. We recommend using ANN for the signal reconstruction in astrophysical data analysis as well as that of in other fields. 相似文献
74.
Kwangsu Ahn Jongchul Chae Kyung-Suk Cho Donguk Song Heesu Yang Philip R. Goode Wenda Cao Hyungmin Park Jakyung Nah Bi-Ho Jang Young-Deuk Park 《Solar physics》2014,289(11):4117-4136
The Fast Imaging Solar Spectrograph (FISS) is being operated on the New Solar Telescope of the Big Bear Solar Observatory. It simultaneously records spectra of Hα and Ca ii 8542 Å lines, and this dual-spectra measurement provides an estimate of the temperature and nonthermal speed components. We observed a loop structure in AR 11305 using the FISS, SDO/AIA, and STEREO/EUVI in 304 Å, and found plasma material falling along the loop from a coronal height into the umbra of a sunspot, which accelerated up to 80 km?s?1. We also observed C2 and C7 flare events near the loop. The temperature of the downflows was in the range of 10?000?–?33?000 K, increasing toward the umbra. The temperature of the flow varied with time, and the temperature near the footpoint rose immediately after the C7 flare, but the temperature toward the umbra remained the same. There seemed to be a temporal correlation between the amount of downflow material and the observed C-class flares. The downflows decreased gradually soon after the flares and then increased after a few hours. These high-speed red-shift events occurred continuously during the observations. The flows observed on-disk in Hα and Ca ii 8542 Å appeared as fragmented, fuzzy condensed material falling from the coronal heights when seen off-limb with STEREO/EUVI at 304 Å. Based on these observations, we propose that these flows were an on-disk signature of coronal rain. 相似文献
75.
76.
Xia Yao Yan ZhuYongChao Tian Wei FengWeiXing Cao 《International Journal of Applied Earth Observation and Geoinformation》2010
Hyperspectral sensing can provide an effective means for fast and non-destructive estimation of leaf nitrogen (N) status in crop plants. The objectives of this study were to design a new method to extract hyperspectral spectrum information, to explore sensitive spectral bands, suitable bandwidth and best vegetation indices based on precise analysis of ground-based hyperspectral information, and to develop regression models for estimating leaf N accumulation per unit soil area (LNA, g N m−2) in winter wheat (Triticum aestivum L.). Three field experiments were conducted with different N rates and cultivar types in three consecutive growing seasons, and time-course measurements were taken on canopy hyperspectral reflectance and LNA under the various treatments. Then, normalized difference spectral indices (NDSI) and ratio spectral indices (RSI) based on the original spectrum and the first derivative spectrum were constructed within the range of 350–2500 nm, and their relationships with LNA were quantified. The results showed that both LNA and canopy hyperspectral reflectance in wheat changed with varied N rates, with consistent patterns across different cultivars and seasons. The sensitive spectral bands for LNA existed mainly within visible and near infrared regions. The best spectral indices for estimating LNA in wheat were found to be NDSI (R860, R720), RSI (R990, R720), NDSI (FD736, FD526) and RSI (FD725, FD516), and the regression models based on the above four spectral indices were formulated as Y = 26.34x1.887, Y = 5.095x − 6.040, Y = 0.609 e3.008x and Y = 0.388x1.260, respectively, with R2 greater than 0.81. Furthermore, expanding the bandwidth of NDSI (R860, R720) and RSI (R990, R720) from 1 nm to 100 nm at 1 nm interval produced the LNA monitoring models with similar performance within about 33 nm and 23 nm bandwidth, respectively, over which the statistical parameters of the models became less stable. From testing of the derived equations, the model for LNA estimation on NDSI (R860, R720), RSI (R990, R720), NDSI (FD736, FD526) and RSI (FD725, FD516) gave R2 over 0.79 with more satisfactory performance than previously reported models and physical models in wheat. It can be concluded that the present hyperspectral parameters of NDSI (R860, R720), RSI (R990, R720), NDSI (FD736, FD526) and RSI (FD725, FD516) can be reliably used for estimating LNA in winter wheat. 相似文献
77.
78.
Jian Cao Zhijun Jin Wenxuan Hu Yijie Zhang Suping Yao Xulong Wang Yueqian Zhang Yong Tang 《Marine and Petroleum Geology》2010
Calcite veins and cements occur widely in Carboniferous and Permian reservoirs of the Hongche fault zone, northwestern Junggar Basin in northwest China. The calcites were investigated by fluid inclusion and trace-element analyses, providing an improved understanding of the petroleum migration history. It is indicated that the Hongche fault behaved as a migration pathway before the Early Cretaceous, allowing two oil charges to migrate into the hanging-wall, fault-core and footwall reservoirs across the fault. Since the Late Cretaceous, the Hongche fault has been sealed. As a consequence, meteoric water flowed down only into the hanging-wall and fault-core reservoirs. The meteoric-water incursion is likely an important cause for degradation of reservoir oils. In contrast, the footwall reservoirs received gas charge (the third hydrocarbon event) following the Late Cretaceous. This helps explain the distribution of petroleum across the fault. This study provides an example of how a fault may evolve as pathway and seal over time, and how reservoir diagenetic minerals can provide clues to complex petroleum migration histories. 相似文献
79.
坛紫菜(于1988年采自青岛太平角海区人工养殖筏上)的水溶性色素粗提物经过硫酸铵沉淀和羟基磷灰石(HA)柱层析后,分离出藻蓝蛋白(RPC)、藻红蛋白(RPE)和变藻蓝蛋白(APC)。在中性介质中,其吸收光谱和荧光发射光谱与文献报道基本一致;但在酸性(pH=3)或碱性(pH=12)介质中,吸收光谱较在中性介质中有明显改变,原有的荧光性质也消失。RPC和APC只分离到一种聚集体,但RPE有两种不同的聚集体。用SephadexG—100凝胶过滤方法测量藻胆蛋白的分子量分别为:RPC117000,APC112000,小分子RPE38000,大分子RPE232000。对三种藻胆蛋白的氨基酸分析的结果表明,三种藻胆蛋白中都是酸性氨基酸的含量大于碱性氨基酸的含量。 相似文献
80.
二色桌片参酶解液对转化细胞的效应 总被引:3,自引:2,他引:3
用二色桌片参(Mensamariaintercedens)酶解液处理转化的人胚肺成纤维细胞(NLF)后,细胞生长受到显著抑制,抑制率达64.84%,光镜下细胞透光性加强,铺展较好,细胞核形更为规则,核畸形现象减少;线粒体结构趋于正常;软琼脂集落实验表明,细胞集落形成率由23x10-5下降至12.5x10-5,裸小鼠致瘤实验显示抑瘤率为82.39%,差异显著(p<5%)。结果提示,二色桌片参酶解液可能逆转转化的HLF细胞的恶性表型,对其有一定的诱导分化作用。 相似文献