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661.
多普勒天气雷达原始资料索引数据库设计 总被引:3,自引:5,他引:3
针对我国现阶段多普勒天气雷达网建设过程中雷达原始资料状况及气象业务发展、教学、科研工作对该类资料的管理需求.尝试设计了适于我国日前布网多普勒天气雷达原始资料的索引数据库管理系统,该系统同样可供由不同类型雷达构成的区域雷达网、全国雷达网雷达原始资料管理作参考。该数据库系统的建立采用结构化程序设计,用Visual C^ 6.0作为应用程序的开发工具,用Microsoft Access 2000做数据库。实现了雷达资料信息入库,修改,查询,资料导出,资料转换,资料回放,数据库备份等功能。 相似文献
662.
本文利用非静力中尺度模式MM5对1998年7月20日-21日发生在湖北东部地区的特大暴雨过程作数值模拟,同时将不同时间的雷达和卫星资料适时加入模式改变当时模式中的水汽场,并与控制试验进行比较分析,结果表明:加入雷达和卫星资料后的数值模拟,由于修正了暴雨区及其邻近区域对流层中低层水汽场,雨区位置和雨量中心值比仅用探空资料的控制试验更接近实况。雷达与卫星资料引入模式对于24小时降雨产生的效果不同,雷达资料的影响是局部的,范围较小,卫星资料影响范围较大,而且适时加入雷达、卫星资料能够及时通过水汽场修正,使24小时预报的雨区范围和中心强度与实况更加接近,而二者结合起来的效果与降水系统的特征有关。 相似文献
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664.
I. B. Araú jo J.C.B. da Silva S. A. Ermakov I. S. Robinson 《Journal of Atmospheric & Ocean Science》2002,8(4):269-281
The relationship between internal wave (IW) signatures in Synthetic Aperture Radar (SAR) images and wind velocity is investigated. The effect of the wind velocity relative to the IW propagation direction on the IW signature is studied by means of a defined signature mode parameter ( S m ). S m is the parameter that quantifies the signature of the IW intensity profile in relation to the mean backscatter of the image background.
A wind contrast model based on a simple first-order Bragg scattering theory is combined with hydrodynamic modulation theory to explain the modulation of IW signatures. It takes into account the modulation of short-scale surface waves by the effect of the relative variations of wind velocity and the surface currents generated by the IWs.
It is shown that the signature mode parameter increases with the angle between the wind velocity and the IW propagation direction so that IWs propagating against the wind direction are imaged mostly as positive sign signatures, while those propagating in the wind direction are mostly negative sign signatures. 相似文献
A wind contrast model based on a simple first-order Bragg scattering theory is combined with hydrodynamic modulation theory to explain the modulation of IW signatures. It takes into account the modulation of short-scale surface waves by the effect of the relative variations of wind velocity and the surface currents generated by the IWs.
It is shown that the signature mode parameter increases with the angle between the wind velocity and the IW propagation direction so that IWs propagating against the wind direction are imaged mostly as positive sign signatures, while those propagating in the wind direction are mostly negative sign signatures. 相似文献
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667.
利用常规观测资料、FY 4A气象卫星红外云图以及多普勒天气雷达资料,分析了2019年5月17日夜间发生在京津冀中部伴有强冰雹、短时强降水和短时大风的强对流天气过程。利用VDRAS资料与国家自动站资料进一步揭示对流风暴形成的环境条件以及后向传播的机制。结果表明:在有利于强对流发生发展的大尺度环流背景场下,京津冀中部的对流系统迅速发展。前期京津一带的强对流天气形成较强的东北风冷池出流,与渤海湾的东南气流交汇,在廊坊北京交界一带形成了向南移动的地面辐合线,并触发了对流。由于新生风暴单体与成熟风暴之间的正反馈作用,使得在廊坊北部形成东西向带状风暴系统,造成对流风暴不断向西传播。向西传播的风暴与西北东南向的平流共同作用,最终导致风暴运动方向为西南方向,成为典型的后向传播风暴。 相似文献
668.
669.
Using a meteor orbit radar, a total of more than 2.5 million meteoroids with masses ∼10−7 kg have had orbits measured in the interval 2002-2006. From these data, a total of 45 meteoroid streams have been identified using a wavelet transform approach to isolate enhancements in radiant density in geocentric coordinates. Of the recorded streams, 12 are previously unreported or unrecognized. The survey finds >90% of all meteoroids at this size range are part of the sporadic meteoroid background. A large fraction of the radar detected streams have q<0.15 AU suggestive of a strong contribution from sungrazing comets to the meteoroid stream population currently intersecting the Earth. We find a remarkably long period of activity for the Taurid shower (almost half the year as a clearly definable radiant) and several streams notable for a high proportion of small meteoroids only, among these a strong new shower in January at the time of the Quadrantids (January Leonids). A new shower (Epsilon Perseids) has also been identified with orbital elements almost identical to Comet 96P/Machholz. 相似文献
670.
M.D. Campbell-Brown 《Icarus》2008,196(1):144-163
Five years of meteor orbit data from CMOR (the Canadian Meteor Orbit Radar) are used to study the high-resolution orbital structure of the sporadic meteoroid complex. The large number of high quality orbits (2.35 million) allows the orbital characteristics of meteoroids to be studied not only in the five sporadic sources accessible from the latitude of London, Ontario, Canada, but at a resolution of 2 degrees. The radiant distribution of sporadic meteors is investigated, applying corrections for observing biases, and weighting to a constant limiting mass, and to a constant limiting energy. The orbital distribution of the sporadic sources is compared to other studies. The variation of average geocentric speed, semimajor axis, eccentricity, inclination and perihelion distance with meteoroid radiant is investigated. The source of a ring depleted in meteor radiants at 55 degrees from the apex is attributed to shorter collisional lifetimes inside the ring, due to a higher probability of catastrophic collisions with particles in the zodiacal cloud for the predominantly retrograde meteoroids inside the ring. 相似文献