全文获取类型
收费全文 | 97767篇 |
免费 | 1947篇 |
国内免费 | 839篇 |
专业分类
测绘学 | 2296篇 |
大气科学 | 6857篇 |
地球物理 | 19605篇 |
地质学 | 35085篇 |
海洋学 | 8601篇 |
天文学 | 21920篇 |
综合类 | 282篇 |
自然地理 | 5907篇 |
出版年
2022年 | 559篇 |
2021年 | 984篇 |
2020年 | 1097篇 |
2019年 | 1193篇 |
2018年 | 2505篇 |
2017年 | 2393篇 |
2016年 | 2911篇 |
2015年 | 1700篇 |
2014年 | 2869篇 |
2013年 | 5054篇 |
2012年 | 3034篇 |
2011年 | 4154篇 |
2010年 | 3561篇 |
2009年 | 4664篇 |
2008年 | 4252篇 |
2007年 | 4130篇 |
2006年 | 3874篇 |
2005年 | 3016篇 |
2004年 | 2950篇 |
2003年 | 2871篇 |
2002年 | 2613篇 |
2001年 | 2373篇 |
2000年 | 2246篇 |
1999年 | 1851篇 |
1998年 | 1944篇 |
1997年 | 1872篇 |
1996年 | 1550篇 |
1995年 | 1542篇 |
1994年 | 1339篇 |
1993年 | 1214篇 |
1992年 | 1137篇 |
1991年 | 1094篇 |
1990年 | 1187篇 |
1989年 | 1029篇 |
1988年 | 934篇 |
1987年 | 1104篇 |
1986年 | 988篇 |
1985年 | 1240篇 |
1984年 | 1348篇 |
1983年 | 1279篇 |
1982年 | 1229篇 |
1981年 | 1072篇 |
1980年 | 1007篇 |
1979年 | 937篇 |
1978年 | 906篇 |
1977年 | 861篇 |
1976年 | 818篇 |
1975年 | 787篇 |
1974年 | 784篇 |
1973年 | 772篇 |
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
561.
F. Steinhauser O. Burkard W. Mörikofer M. Toperczer 《Meteorology and Atmospheric Physics》1962,13(2):290-304
Ohne Zusammenfassung 相似文献
562.
Summary The process of radon diffusion in space and time through rocks is treated in detail from the point of view of radiometric prospecting for oil. Taking into account the depth and diffusivity conditions encountered in nature it is stated that vertical radon diffusion reaching from the oil deposits up to the surface cannot be expected. Time intervals as required for setting in of a stationary concentration state and decay conditions of the radon lead to the conclusion that the penetration of emanometric measurements seldom exceeds the depth of 5–10 m. 相似文献
563.
M. A. Anastassiades L. N. Carapiperis N. K. Kariambas P. G. Paraskevopoulos 《Pure and Applied Geophysics》1962,52(1):143-152
Summary In this study the different forms of the electromagnetic field strength recordings at the Thera-Crete microwave line of link are examined, in comparison with the corresponding weather situations prevailing over that area. According to the amplitude of fluctuations, the different forms of recordings have been classified in three basic typesA, B, C and the annual frequency of the appearance of these types has been observed. Finally, the influence of weather situations on radio wave propagation was examined and it has been found that in most cases a close relationship exists between weather situations and the different fading forms of the electromagnetic field so that a prediction of the fading form be possible by means of the weather forecast.This study was sponsored by a research grant from NATO's Scientific Committee. 相似文献
564.
Ohne Zusammenfassung 相似文献
565.
566.
M. Čadež 《Pure and Applied Geophysics》1960,47(1):172-182
Zusammenfassung Man beobachtet Antizyklonen, die als Folge einer Konzentration von Kaltluftmasssen auf ein kleineres Gebiet gedeutet werden können. Die Konzentration der Kaltluft ist durch die Umwandlung der kinetischen Energie der Kaltluft in potentielle Energie oder durch die Wärmezufuhr der kalten Luft bedingt. Solche Antizyklonen bilden sich oft in Berggebieten, da dort wegen der grossen äusseren Reibung die erwähnte Umwandlung der Energie beschleunigt wird. Wie gross solche antizyklogenetischen Effekte sein können, ist berechnet.
Summary The origin of some anticyclones can be explained as a consequence of the concentration of the cold air on a smaler area. The concentration of the cold air is caused by a transformation of the kinetic energy of the cold air into the potential energy or by the heating of the cold air. Such anticyclones often appear in mountain regions where the transformation of the mentioned energy is more intense. The intensity of such anticyclogenetical effects is evaluated.相似文献
567.
568.
G. R. Huguenin A. E. Lilley W. H. McDonough M. D. Papagiannis 《Planetary and Space Science》1964,12(12):1157-1167
Radio noise observations at frequencies of 0·700 Mc and 2·200 Mc were made at altitudes between 3000 and 11,000 km from a Blue Scout Jr. high-altitude rocket probe on 30 July 1963. A steady background flux of (7·5−3+6) × 10−19 W m−2)(c/s)−1 at 0·700 Mc and (1·8+1.0−0.5 × 10−19 W m−2 (c/s)−1 at 2·200 Mc was observed. Assuming a galactic origin of the observed fluxes at both frequencies, the averaged sky brightnesses are b(0·700 Mc) = (6−3+5) × 10−20 W m−2 (c/s)−1 sr−1b(2·200 Mc) = (1.4+1.0−0.5 × 10−20 W m−2 (c/s)−1 sr−1 The observed brightness at 2·200 Mc is in reasonable agreement with the results of other observers. The apparent brightness at 0·700 Mc is, however, greater than was expected from previous observations. An alternative source of the 0·700 Mc flux in the terrestrial exosphere, as well as characteristics of several noise bursts observed during the flight, is briefly discussed. 相似文献
569.
570.
With an appropriate system of higher order approximations the Faraday-effect is calculated for instantaneous ionospheric models the data of which are derived from the results of vertical soundings. Only one parameter which corresponds to the thickness of the outer ionosphere is left open; it is determined by global comparison with simultaneous Faraday-observations of satellite emissions. The thickness parameter shows various forms of variation with latitude; an increase towards north is the rule for quiet daytime conditions. Comparison with local methods shows considerable differences due to the indetermination of the absolute number of rotations. 相似文献