全文获取类型
收费全文 | 1760篇 |
免费 | 46篇 |
国内免费 | 14篇 |
专业分类
测绘学 | 32篇 |
大气科学 | 170篇 |
地球物理 | 331篇 |
地质学 | 515篇 |
海洋学 | 211篇 |
天文学 | 433篇 |
综合类 | 7篇 |
自然地理 | 121篇 |
出版年
2020年 | 14篇 |
2017年 | 14篇 |
2016年 | 15篇 |
2015年 | 24篇 |
2014年 | 42篇 |
2013年 | 106篇 |
2012年 | 35篇 |
2011年 | 59篇 |
2010年 | 48篇 |
2009年 | 77篇 |
2008年 | 62篇 |
2007年 | 57篇 |
2006年 | 52篇 |
2005年 | 46篇 |
2004年 | 42篇 |
2003年 | 56篇 |
2002年 | 42篇 |
2001年 | 24篇 |
2000年 | 32篇 |
1999年 | 19篇 |
1998年 | 33篇 |
1997年 | 29篇 |
1996年 | 25篇 |
1995年 | 33篇 |
1994年 | 34篇 |
1993年 | 26篇 |
1992年 | 27篇 |
1991年 | 38篇 |
1990年 | 29篇 |
1989年 | 27篇 |
1988年 | 26篇 |
1987年 | 33篇 |
1986年 | 45篇 |
1985年 | 24篇 |
1984年 | 41篇 |
1983年 | 27篇 |
1982年 | 22篇 |
1981年 | 32篇 |
1980年 | 33篇 |
1979年 | 32篇 |
1978年 | 33篇 |
1977年 | 37篇 |
1976年 | 22篇 |
1975年 | 32篇 |
1974年 | 18篇 |
1973年 | 30篇 |
1972年 | 35篇 |
1971年 | 27篇 |
1970年 | 15篇 |
1969年 | 18篇 |
排序方式: 共有1820条查询结果,搜索用时 15 毫秒
141.
Dr. Matthias Tomczak Jr. 《Ocean Dynamics》1968,21(4):145-151
Zusammenfassung Für winderzeugte interne Wellen wird gezeigt, daß bei der Trägheitsperiode in erster Näherung Resonanz eintritt, die in zweiter Näherung in zwei symmetrisch zur Trägheitsperiode liegende Resonanzen zerfällt. Der Effekt wächst mit zunehmender Schichtung und ist außerdem abhängig vom virtuellen Austauschkoeffizienten und der WellenlängeL der internen Wellen. Die Näherung erfolgt in Termen des Verhältnissesd
2
H
2
(d=Dicke der winderzeugten Grenzschicht,H=Wassertiefe).
On internal waves near the inertia period
Summary Wind-generated internal waves are shown to have a resonance at the inertia period to first order of an analytical approximation which, to second order, splits into two resonances lying symmetrically to the inertia period. The effect is large for strong stratification and depends also on the Austausch coefficient and the wave lengthL of the internal waves. The approximation is done in terms ofd 2 H 2 whered=thickness of the wind-generated boundary layer andH=water depth.
Sur les ondes internes près de la période d'inertie
Résumé On montre que pour les ondes internes dues au vent, il se produit en première approximation, à la période d'inertie, une résonance qui, en deuxième approximation, se décompose en deux résonances symétriques par rapport à la période d'inertie. L'effet augmente avec une stratification croissante et dépend en outre du coefficient de turbulence virtuel et de la longueur d'ondeL des ondes internes. L'approximation s'obtient en termes du rapportd 2 H 2 (d=épaisseur de la couche-limite due au vent,H=profondeur de l'eau).相似文献
142.
The oxygen isotope geochemistry of igneous rocks 总被引:34,自引:0,他引:34
Hugh P. Taylor Jr. 《Contributions to Mineralogy and Petrology》1968,19(1):1-71
Oxygen isotope analyses have been obtained for 443 igneous rock and mineral samples from various localities throughout the world. Detailed studies were made on the Medicine Lake, Newberry, Lassen, Clear Lake, S. E. Guatemala, Hawaii and Easter I. volcanic complexes and on the Bushveld, Muskox, Kiglapait, Guadalupe, Duluth, Nain, Egersund, Lac St. Jean, Laramie, Skaergaard, Mull, Skye, Ardnamurchan and Alta, Utah plutonic complexes, as well as upon several of the zoned ultramafic intrusions of S. E. Alaska. Basalts, gabbros, syenites and andesites are very uniform in O18/O16, commonly with δ-values of 5.5 to 7.0 per mil. Many rhyolite obsidians, particularly those from oceanic areas and the Pacific Coast of the United States, also lie in this range; this indicates that such obsidians are differentiates of basaltic or andesitic magma at high temperatures (about 1,000° C). They cannot represent melted sialic crust. The only plutonic granites with such low δ-values are some of the hypersolvus variety, suggesting that these also might form by fractional crystallization. Obsidians from the continental interior, east of the quartz-diorite line, have higher δ-values. This is compatible with their having assimilated O18-rich sialic crust. A correlation generally exists between the O18/O16 ratios of SiO2-rich differentiates and the chemical trends in volcanic complexes. High O18/O16 ratios accompany those trends having the lower Fe/Mg ratios, while ferrogabbro trends are associated with depletion in O18. Variations in oxygen fugacity may be responsible for these effects, as abundant early precipitation of magnetite should lead to both O18-enrichment and Fe-depletion in later differentiates. Plutonic granites have higher O18/O16 ratios than their volcanic equivalents, because (a) their differentiation occurred at much lower temperatures, or (b) they are in large part derived from O18-rich sialic crust by partial melting or assimilation. Also, the oxygen isotope fractionations among coexisting minerals are distinctly larger in plutonic rocks than in volcanic rocks. This is in keeping with their lower crystallization temperatures and their longer cooling history, which promotes post-crystallization oxygen isotope exchange. Hydrated obsidians and perlites have δO18-values that are much different from their primary, magmatic values. A correlation exists between D/H and O18/O16 ratios in hydrated volcanic glass from the western U.S.A., proving that the isotopic compositions are a result of exchange with meteoric waters. The O18 contents of the glasses appear to be about 25 per mil higher than their associated waters; hence, these hydrated glasses have not simply absorbed H2O, but they have exchanged with large quantities of it. The igneous rocks from Mull, Skye, Ardnamurchan and the Skaergaard intrusion are all abnormally depleted in O18 relative to “normal” igneous rocks. This is a result of their having exchanged at high temperatures with meteoric water that was apparently abundant in the highly jointed plateau lavas into which these igneous rocks were intruded. In part, this exchange occurred with liquid magma and in part with the crystalline rock; in the latter case the feldspar was more easily exchanged and has become much more depleted in O18 than has coexisting quartz or pyroxene. The later differentiates of the Muskox intrusion are markedly O18-rich, but this is not a result of fractional crystallization. It is in large part a result of deuteric exchange between feldspars and an oxygen-bearing fluid (H2O ?) that was either O18-rich or had a relatively low temperature. This phenomenon was also observed in a number of granophyres from other localities, particularly those containing brick-red alkali feldspar. The exchanged feldspars in all these examples are turbid or cloudy, and may be filled with hematite dust. It is concluded that most such feldspar in nature is the result of deuteric exchange and is probably drastically out of oxygen isotopic equilibrium with its coexisting quartz. 相似文献
143.
144.
145.
147.
148.
Alfred Clark Jr. 《Solar physics》1968,4(4):386-400
Some theoretical models are given which illustrate the structure of chromospheric magnetic fields associated with supergranulation. It is found that the chromospheric fields depend critically on whether or not there are large-scale vertical motions at the level where the horizontal supergranule motions are observed. In the absence of such motions, the concentration of field produced in the photosphere does not persist more than a few scale heights into the chromosphere; however, the chromospheric mass density is increased above the supergranule boundaries in this case. Completely different results-such as a chromospheric potential field-may be obtained by the inclusion of vertical motions. It is concluded that a rather wide range of chromospheric-field structures is consistent with present observational knowledge of the supergranulation. 相似文献
149.
150.