全文获取类型
收费全文 | 271篇 |
免费 | 17篇 |
国内免费 | 2篇 |
专业分类
测绘学 | 7篇 |
大气科学 | 21篇 |
地球物理 | 71篇 |
地质学 | 73篇 |
海洋学 | 31篇 |
天文学 | 67篇 |
综合类 | 1篇 |
自然地理 | 19篇 |
出版年
2023年 | 2篇 |
2022年 | 4篇 |
2021年 | 5篇 |
2020年 | 7篇 |
2019年 | 9篇 |
2018年 | 12篇 |
2017年 | 9篇 |
2016年 | 19篇 |
2015年 | 9篇 |
2014年 | 8篇 |
2013年 | 17篇 |
2012年 | 15篇 |
2011年 | 18篇 |
2010年 | 17篇 |
2009年 | 17篇 |
2008年 | 12篇 |
2007年 | 21篇 |
2006年 | 10篇 |
2005年 | 13篇 |
2004年 | 4篇 |
2003年 | 11篇 |
2002年 | 5篇 |
2001年 | 7篇 |
2000年 | 4篇 |
1999年 | 5篇 |
1998年 | 6篇 |
1997年 | 2篇 |
1996年 | 1篇 |
1995年 | 3篇 |
1994年 | 4篇 |
1993年 | 2篇 |
1992年 | 1篇 |
1991年 | 1篇 |
1990年 | 1篇 |
1988年 | 2篇 |
1987年 | 1篇 |
1984年 | 3篇 |
1981年 | 1篇 |
1978年 | 1篇 |
1964年 | 1篇 |
排序方式: 共有290条查询结果,搜索用时 31 毫秒
281.
F. Snchez‐Bajo A. Garrigs‐Snchez J.M. Gmez‐Forrellad J. Nomen‐Torres W. Kleikamp P. Frank W. Moschner W. Quester E. García‐Melendo 《Astronomische Nachrichten》2003,324(6):511-515
Results of the photometric analysis by means of the Wilson‐Devinney method, combined with an empirical massradius relation for LC IV stars support the hypothesis that GX Gem is a well detached evolved system of subgiant stars. The solution is consistent with the known spectroscopic parameters obtained by Popper (1996) and the photometric data of Lacy (2002a). (© 2003 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) 相似文献
282.
Geotectonics - Extension parallel to fold axis represents a rarely documented tectonic process that occur in different tectonic settings such as large-scale orogenic belts, mountain ranges, and... 相似文献
283.
Paulo Torres Gil Penha-Lopes Luís Narciso Adriano Macia José Paula 《Estuarine, Coastal and Shelf Science》2008
Variations in egg volume and fatty acid (FA) content through embryogenesis were evaluated in Uca species from Inhaca island, Mozambique. Egg volume increased 96.1%, 93.3%, 84.2%, 92.9%, 96.3%, respectively, in Uca annulipes, Uca inversa, Uca urvillei, Uca chlorophthalmus and Uca vocans (p < 0.05). Fatty acid content decreased through embryogenesis, showing its importance as fuel during embryonic development. Major fatty acids were 16:0, 18:0, 16:1n-7, 18:1n-9, 18:1n-7, 18:2n-6, 20:5n-3 and 20:4n-3. Unsaturated fatty acids (UFA) and saturated fatty acids (SFA) were used up at a similar rate for U. annulipes and U. inversa contrarily to the other three species. Within the UFA, MUFA were more consumed than PUFA for all species except U. chlorophthalmus. The high values detected for fatty acid trophic markers (essential C18 and C20 PUFAs) and odd-numbered fatty acid suggest that Uca species occupy medium trophic level, primarily omnivores and scavengers/detritivores consuming algae common in the intertidal habitats. The fatty acid consumption pattern during embryonic development was essentially similar between species with some variation as expected, as FA content varies within species mainly due to female feeding ecology, nutritional and physiological conditions, differential demands on resource allocation and geographic and seasonal variations in embryonic development. 相似文献
284.
2006年度印度洋天然气水合物规划(NG—HP)的目标是调查控制印度近海天然气水合物分布及其特征的地质因素,以便最终评价作为潜在能源的天然气水合物的开采可能性。海洋中聚集的天然气水合物的总量是巨大的,大约25000~10000亿t。 相似文献
285.
Petrographic and geochemical evidence for multiphase formation of carbonates in the Martian orthopyroxenite Allan Hills 84001
下载免费PDF全文
![点击此处可从《Meteoritics & planetary science》网站下载免费的PDF全文](/ch/ext_images/free.gif)
Carles E. Moyano‐Cambero Josep M. Trigo‐Rodríguez M. Isabel Benito Jacinto Alonso‐Azcárate Martin R. Lee Narcís Mestres Marina Martínez‐Jiménez Francisco J. Martín‐Torres Jordi Fraxedas 《Meteoritics & planetary science》2017,52(6):1030-1047
Martian meteorites can provide valuable information about past environmental conditions on Mars. Allan Hills 84001 formed more than 4 Gyr ago, and owing to its age and long exposure to the Martian environment, and this meteorite has features that may record early processes. These features include a highly fractured texture, gases trapped during one or more impact events or during formation of the rock, and spherical Fe‐Mg‐Ca carbonates. In this study, we have concentrated on providing new insights into the context of these carbonates using a range of techniques to explore whether they record multiple precipitation and shock events. The petrographic features and compositional properties of these carbonates indicate that at least two pulses of Mg‐ and Fe‐rich solutions saturated the rock. Those two generations of carbonates can be distinguished by a very sharp change in compositions, from being rich in Mg and poor in Fe and Mn, to being poor in Mg and rich in Fe and Mn. Between these two generations of carbonate is evidence for fracturing and local corrosion. 相似文献
286.
Mnica Susana Hoffmeyer Menndez María Clara Biancalana Florencia Nizovoy Alicia Mabel Torres Eduardo Ramn 《Estuarine, Coastal and Shelf Science》2009,84(3):181-392
This study focuses on the composition, abundance and distribution of ichthyoplankton in the inner shelf area off Bahía Blanca Estuary on the SW Atlantic Ocean during late spring. Eggs and larvae of Brevoortia aurea, Engraulis anchoita, Parona signata, Sciaenidae spp. – such as Cynoscion guatucupa and Micropogonias furnieri –, and Odontesthes argentinensis were found. Species richness was low probably as a result of season and shallow depths. Ichthyoplankton abundance reached values close to 10 000 per 10 m−3 (eggs) and 4000 per 10 m−3 (larvae) and displayed a spatial distribution pattern with maximum abundance values restricted to a band parallel to the coast. Differences between egg and larval patterns, probably derived from a different displacement and hydrodynamic behavior, were observed. Egg and larvae distribution patterns were found related with spawning areas and to directly depend on salinity and mesozooplankton. The larvae distribution pattern, in particular, was found to inversely depend on particulate organic carbon. In addition, the geographic location of egg and larvae maxima strongly coincided with a saline front reported for this area in springtime, thus suggesting a direct relationship with it. 相似文献
287.
水分子与烃类气体沉积物孔隙中结合形成水合物的过程中,只吸取孔隙中的淡水,而盐类物质不能进入水合物的晶体结构,在水合物形成过程中会引起局部孔隙水离子浓度的浓缩,增加周围沉积物孔隙水的盐度;而当水合物分解时,孔隙水就会被稀释,使得钻孔获得的水合物样品比不含水合物的样品具有更低的盐度.因为C1-是浅层海洋没积物孔隙水中一种丰富且保守的离子,C1-离子浓度变化通常被用来监测天然气水合物的形成和分解.…… 相似文献
288.
289.
290.
W.J. Chaplin T. Appourchaux T. Arentoft J. Ballot J. Christensen‐Dalsgaard O.L. Creevey Y. Elsworth S.T. Fletcher R.A. García G. Houdek S.J. Jimnez‐Reyes H. Kjeldsen R. New C. Rgulo D. Salabert T. Sekii S.G. Sousa T. Toutain the rest of the asteroFLAG group 《Astronomische Nachrichten》2008,329(5):549-557
We report on initial results from the first phase of Exercise #1 of the asteroFLAG hare and hounds. The asteroFLAG group is helping to prepare for the asteroseismology component of NASA's Kepler mission, and the first phase of Exercise #1 is concerned with testing extraction of estimates of the large and small frequency spacings of the low‐degree p modes from Kepler‐like artificial data. These seismic frequency spacings will provide key input for complementing the exoplanet search data. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) 相似文献