全文获取类型
收费全文 | 369篇 |
免费 | 101篇 |
国内免费 | 128篇 |
专业分类
测绘学 | 65篇 |
大气科学 | 44篇 |
地球物理 | 93篇 |
地质学 | 219篇 |
海洋学 | 53篇 |
天文学 | 6篇 |
综合类 | 57篇 |
自然地理 | 61篇 |
出版年
2024年 | 6篇 |
2023年 | 14篇 |
2022年 | 31篇 |
2021年 | 39篇 |
2020年 | 42篇 |
2019年 | 23篇 |
2018年 | 39篇 |
2017年 | 24篇 |
2016年 | 36篇 |
2015年 | 24篇 |
2014年 | 32篇 |
2013年 | 52篇 |
2012年 | 38篇 |
2011年 | 41篇 |
2010年 | 19篇 |
2009年 | 21篇 |
2008年 | 22篇 |
2007年 | 16篇 |
2006年 | 10篇 |
2005年 | 8篇 |
2004年 | 4篇 |
2003年 | 15篇 |
2002年 | 6篇 |
2001年 | 6篇 |
2000年 | 6篇 |
1999年 | 6篇 |
1998年 | 2篇 |
1997年 | 3篇 |
1996年 | 3篇 |
1995年 | 2篇 |
1994年 | 1篇 |
1992年 | 2篇 |
1990年 | 2篇 |
1989年 | 1篇 |
1988年 | 2篇 |
排序方式: 共有598条查询结果,搜索用时 15 毫秒
101.
102.
万里长江的形成经历了数次大规模的河流袭夺事件,现今的长江中游河段(川江)曾经作为古长江的西支,自东向西汇入南流的古金沙江,后来由于不断的反向才使其与古长江的东支,即现今的长江下游得以贯通.针对这一河流演化模式,学术界普遍将长江三峡的黄陵背斜视为古长江东支和西支的分水岭,然而却一直未能获得有效的地貌证据,以致于无法解释具体的河流袭夺和反向过程.为此,本文从川东-湘鄂西弧形断褶带的构造地貌特征入手,深入分析了不同区段长江及其支流与构造线的交切关系,提出古长江东支和西支的分水岭应位于弧形带的“中线”附近的向斜谷地内,而并非前人认为的黄陵背斜.通过对向斜谷地内正交型水系样式下的河流袭夺案例分析,结合先进的河流纵剖面分析技术,揭示出由于基准面下降而造成的纵向河段被袭夺并最终反向的机制.另外,根据江汉盆地西缘(宜昌地区)的白垩纪-新生代地层的沉积学和物源分析,进一步限定了长江中游的袭夺和反向开始于始新世,直到中新世才形成现今贯通的长江. 相似文献
103.
地球表面每时每刻都在经历各式各样的侵蚀作用,了解侵蚀过程及其速率大小有助于人们认识许多重要的地质作用和过程.本文介绍的内容是长江流域河流沉积物宇宙成因核素10Be的研究工作,目的是在于定量估算长江流域及其子流域的平均侵蚀速率,更好地理解沉积物的由源到汇过程以及评价人类活动对水土流失的影响提供自然背景,分析样品来自于长江主要干流和支流的表层现代沉积.研究表明,长江干流10Be含量从金沙江流域到长江口呈现出由高到低的趋势,不同的是支流10Be含量值偏低而且比较稳定.这很可能受核素产生率和侵蚀速率两个因素的共同影响.在长江上游干流沉积物中10Be含量最高,随着低含量物质的不断从支流汇入,产生“西高东低”的现象.10Be侵蚀速率估算表明长江干流金沙江上游段平均侵蚀速率较低,在44.7~48.1m/Ma之间;长江中游段(枝江至彭泽)长江干流侵蚀速率数据变化较大,在65.7 ~ 175m/Ma的范围内波动;到长江口平均侵蚀速率比较稳定,在50~60m/Ma之间变化.与干流相比,长江支流侵蚀速率显著偏高.侵蚀速率最高的地区在大渡河-岷江流域,平均侵蚀速率在300m/Ma之上;侵蚀速率最低的区域发生在乌江流域,平均的侵蚀速率在10 ~ 30m/Ma之间.比较长江流域10Be和水文估算的侵蚀速率可以看出,水文估算总体上反映的侵蚀速率要普遍高于10Be反映的侵蚀速率.大渡河-岷江流域地表侵蚀速率高主要与构造活动、地貌发育、岩石特征以及气候条件等自然因素有关.嘉陵江、汉江等流域水文数据估算侵蚀速率明显超过10Be估算的结果,可能与地形地貌等地质因素对侵蚀作用的影响显著下降,以及人类长期活动导致水土流失加剧有关. 相似文献
104.
105.
Soil containing calcic nodules is widely present on the northern Loess Plateau of China owing to soil genesis under local climate conditions. In most studies, little attention is payed to the effect of calcic nodules on soil evaporation and ecoenvironment, resulting in inaccurate evaporation estimation in this kind of soil and further improper field water management measures and irrigation effects. In this paper, soil column experiments were conducted in order to investigate evaporation process in soil containing calcic nodules and the effect of calcic nodules on soil evaporation was determined. The results indicated that evaporation reduction was positively related to calcic nodule content (CNC = mass of calcic nodules/total mass), and could be estimated by the experiential equation: Esoil = E0 (1 – 0.4 CNC) (Esoil = actual evaporation, E0 = theory evaporation in soil without calcic nodules). When CNC was below 0.2, the impact could be neglected. While, as CNC exceeded 0.2, the impact needed to be considered during soil evaporation estimation. As CNC reached 0.5, soil evaporation could be reduced by 7.5 mm, accounting for around 10% of the total soil water. Water balance calculation in soil columns showed that water absorbed by calcic nodules was partially available to evaporation. Water available to evaporation was positively related to CNC, and this water could not exceed 63% of the water absorbed by calcic nodules. Generally, evaporation behavior was dominated by calcic nodule quantity and its water absorption. These results provide new ideas for irrigation measures in arid areas of the globe. 相似文献
106.
Yetang Hong Dongsheng Liu Hongbo Jiang Liping Zhou J. Beer Bing Hong Yongxuan Zhu Handing Li Xuetian Leng Xiaoguang Qin Wang Yu Qinghua Lin Yiqiang Zeng 《中国科学D辑(英文版)》2000,43(2):217-224
There have been a number of investigations for examining the possible link between long-term climate variability and solar
activity. A continuous δ18O record of peat cellulose covering the past 6 000 years and the response of climate variation inferred from the proxy record
to solar forcing are reported. Results show that during the past 5 000 years the abrupt climate variations, including 17 warming
and 17 cooling, and a serious of periodicities, such as 86, 101, 110, 127, 132, 140, 155, 207, 245, 311, 820 and 1 050 years,
are strikingly correlative to the changes of solar irradiation and periodicity. These observations are considered as further
evidence for a close relationship between solar activity and climate variations on time scales of decades to centuries. 相似文献
107.
对金属矿床成矿溶液的性质 ,特别是 pH值 (酸碱度 )的确定 ,是认识含矿溶液的成因、成矿条件和成矿机理的关键。目前对成矿溶液性质的研究主要局限在对围岩蚀变矿物包裹体的测定方面 ,并得出近中性热卤水成矿的结论。作者认为 ,多数围岩蚀变矿物的包裹体溶液不能代表原成矿溶液的性质 ,“近中性的热卤水成矿”的认识有误 ,应是酸性水形成的含矿溶液成矿 ,并从矿物包裹体溶液的特征、Roedder的高金属含量的矿物包裹体溶液的发现、氢氧同位素资料、矿物包裹体中高卤水溶液的起源以及成矿溶液的演化机理等方面论述了酸性金属含矿溶液的成因及成矿演化过程。 相似文献
108.
In this study,three methods were used to analyze 17 large-scale local high-temperature regions with durations exceeding 2 h within magnetic clouds(MCs)observed by advanced composition explorer from 1998 to 2008.Results show that five of these large-scale regions may have been caused by flare heating;seven of the regions may have been caused by nonuniform expansion when MCs propagated in the solar-terrestrial space;four large-scale high temperature regions may likely result from combined non-uniform expansion and flare heating;and only one large-scale local high-temperature region was not related to either flare heating nor non-uniform expansion.No evidence indicated that magnetic reconnection occurred or had occurred within the high-temperature regions.Based on our results,we infer that such local high-temperature phenomena within MCs are caused primarily as a result of flare heating and non-uniform expansion,either separately or jointly,and that magnetic reconnection plays only a minor role in the formation of high-temperature regions. 相似文献