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21.
Machine-learning algorithms are applied to explore the relation between significant flares and their associated CMEs. The
NGDC flares catalogue and the SOHO/LASCO CME catalogue are processed to associate X and M-class flares with CMEs based on
timing information. Automated systems are created to process and associate years of flare and CME data, which are later arranged
in numerical-training vectors and fed to machine-learning algorithms to extract the embedded knowledge and provide learning
rules that can be used for the automated prediction of CMEs. Properties representing the intensity, flare duration, and duration
of decline and duration of growth are extracted from all the associated (A) and not-associated (NA) flares and converted to
a numerical format that is suitable for machine-learning use. The machine-learning algorithms Cascade Correlation Neural Networks
(CCNN) and Support Vector Machines (SVM) are used and compared in our work. The machine-learning systems predict, from the
input of a flare’s properties, if the flare is likely to initiate a CME. Intensive experiments using Jack-knife techniques
are carried out and the relationships between flare properties and CMEs are investigated using the results. The predictive
performance of SVM and CCNN is analysed and recommendations for enhancing the performance are provided. 相似文献
22.
Robert M. Suggs William J. Cooke Ronnie J. Suggs Wesley R. Swift Nicholas Hollon 《Earth, Moon, and Planets》2008,102(1-4):293-298
NASA’s Meteoroid Environment Office has implemented a program to monitor the Moon for meteoroid impacts from the Marshall
Space Flight Center. Using off-the-shelf telescopes and video equipment, the Moon is monitored for as many as 10 nights per
month, depending on weather. Custom software automatically detects flashes which are confirmed by a second telescope, photometrically
calibrated using background stars, and published on a website for correlation with other observations. Hypervelocity impact
tests at the Ames Vertical Gun Range facility have begun to determine the luminous efficiency and ejecta characteristics.
The purpose of this research is to define the impact ejecta environment for use by lunar spacecraft designers of the Constellation
manned lunar program. The observational techniques and preliminary results will be discussed.
The U.S. Government's right to retain a non-exclusive, royalty-free license in and to any copyright is acknowledged. 相似文献
23.
Gerhard Drolshagen Valeri Dikarev Markus Landgraf Holger Krag Wim Kuiper 《Earth, Moon, and Planets》2008,102(1-4):191-197
Over the last decade several new models for the sporadic interplanetary meteoroid flux have been developed. These include
the Divine-Staubach and the Dikarev model. They typically cover mass ranges from 10−18 g to 1 g and are applicable for model specific Sun distance ranges between 0.1 AU and 20 AU Near 1 AU averaged fluxes (over
direction and velocities) for all these models are tuned to the well established interplanetary model by Grün et al. However,
in many respects these models differ considerably. Examples are the velocity and directional distributions and the assumed
meteoroid sources. In this paper flux predictions by the various models to Earth orbiting spacecraft are compared. Main differences
are presented and analysed. The persisting differences even for near Earth space can be seen as surprising in view of the
numerous ground based (optical and radar) and in situ (captured Inter Stellar Dust Particles, in situ detectors and analysis
of retrieved hardware) measurements and simulations. 相似文献
24.
Wei Yong Rong Zhaojin Zhong Jun Chai Lihui Yue Xin an Liu Libo Yu Sheng Zhu Rixiang Wan Weixing 《地球科学进展》2017,32(1):15-20
It has been 60 years since the space physics as new branch of geophysics started to grow in 1957 when the space age was opened by a small satellite called sputnik. The knowledge of Earth and planetary space has been significantly extended and deepened, but the questions we are facing today are more challenging. A consensus reached is that we have to regard the Earth (planet) as an integrated system including all spheres from the inner core to the magnetosphere, and we should try to investigate some questions standing on the ground of interdisciplinary study, especially those questions related to Earth’s (planetary) evolution. Space environment as the outer part of a planetary system, commonly exists in all planets but also exhibits strong diversity. Here, we introduce the short history of basic ideas and methods of comparative study, the advantages on understanding of some issues of global scale, and the prospect from comparative perspective. 相似文献
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探讨利用SCIAMACHY数据反演温室气体二氧化碳 总被引:1,自引:0,他引:1
自工业革命以来CO2已经成为引起全球气候变暖的一种最主要的人为温室气体,由此引起的全球气候变化是当今社会经济可持续发展面临的最严峻挑战之一.为了更好的研究二氧化碳在时间与空间尺度上的格局及变化,综合分析CO2与太阳辐射、地面反照率、气溶胶等要素之间的关系,本文回顾了以往利用新型卫星传感器获取多源遥感数据的特点,分析了多种反演计算方法的优缺点,并结合地面实测数据进行对比分析的方法与理论,全面阐述国际上有关CO2柱浓度反演的思想.作者认为目前在地面观测站较少的情况下,针对先进的SCIAMACHY传感器数据利用DOAS相关算法及BESD算法进行CO2柱体浓度反演的数据连续,技术成熟,并由此提出了下一步工作中应解决的3个问题. 相似文献
27.
随着“智慧地球”“智慧城市”的发展,以及人类科学技术和对自然认识水平的提高,传统的空间信息显示与简单的数据存储、管理已不能满足我们对空间认知的需求,空间信息获取的广泛性、时效性、便捷性以及地图服务的智能化与人性化已经成为当前地图行业需求热点.同时,物联网、云计算等新兴信息技术的迅速发展所引爆的第三代信息革命为现代地图学的发展带来了新的契机.本文以地图学历史发展为主线,系统梳理“地图”的相关概念、内涵及技术理论,并结合当前经济、社会及技术背景,重新整合地图的发展需求、内涵及技术体系,提出一种全新的“智慧地图”概念,为现代地图学及数字地图技术的发展提供一种新的视角与理论方法框架. 相似文献
28.
利用1988,1992,2001,2008年4个时相的遥感影像和GIS技术获取历史数据,采用SLEUTH模型,对焦作市未来城市空间演变进行研究。结果显示:SLEUTH模型重现了焦作市1988~2008年城市空间演变形态,模拟结果与实际情况比较吻合,充分证明SLEUTH模型具有普适性,通过校正能较好地描述城市增长的自然规律;预测模拟了2009~2020年城市空间增长,城市扩展趋势是新扩展中心出现边缘式扩展,向周围地区蔓延,在交通轴线连接下,形成组团式布局。研究结果为研究区城市发展及政府制定规划提供了科学决策依据。 相似文献
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