全文获取类型
收费全文 | 5951篇 |
免费 | 178篇 |
国内免费 | 62篇 |
专业分类
测绘学 | 123篇 |
大气科学 | 503篇 |
地球物理 | 1373篇 |
地质学 | 1984篇 |
海洋学 | 592篇 |
天文学 | 957篇 |
综合类 | 14篇 |
自然地理 | 645篇 |
出版年
2021年 | 46篇 |
2020年 | 65篇 |
2019年 | 73篇 |
2018年 | 111篇 |
2017年 | 116篇 |
2016年 | 132篇 |
2015年 | 103篇 |
2014年 | 129篇 |
2013年 | 315篇 |
2012年 | 177篇 |
2011年 | 260篇 |
2010年 | 237篇 |
2009年 | 236篇 |
2008年 | 241篇 |
2007年 | 210篇 |
2006年 | 228篇 |
2005年 | 182篇 |
2004年 | 184篇 |
2003年 | 171篇 |
2002年 | 165篇 |
2001年 | 117篇 |
2000年 | 109篇 |
1999年 | 103篇 |
1998年 | 95篇 |
1997年 | 85篇 |
1996年 | 88篇 |
1995年 | 92篇 |
1994年 | 86篇 |
1993年 | 76篇 |
1992年 | 86篇 |
1991年 | 70篇 |
1990年 | 98篇 |
1989年 | 85篇 |
1988年 | 75篇 |
1987年 | 100篇 |
1986年 | 76篇 |
1985年 | 96篇 |
1984年 | 131篇 |
1983年 | 108篇 |
1982年 | 97篇 |
1981年 | 100篇 |
1980年 | 88篇 |
1979年 | 100篇 |
1978年 | 71篇 |
1977年 | 86篇 |
1976年 | 71篇 |
1975年 | 70篇 |
1974年 | 55篇 |
1973年 | 61篇 |
1972年 | 35篇 |
排序方式: 共有6191条查询结果,搜索用时 15 毫秒
861.
862.
863.
Robert W. Milkey 《Solar physics》1970,14(1):62-76
A geometrical optics technique developed in order to study energy transport by weak fast-mode hydromagnetic shock waves in a non-homogeneous, anisotropic medium has been applied to the problem of the heating of the chromosphere in the regions of intensified magnetic field which occur above the boundaries of supergranular cells. The results of the calculation indicate that there should be a temperature enhancement in the regions of the chromospheric network. This temperature enhancement is advanced as a possible mechanism for the origin of the observed calcium emission network.Publications of the Goethe Link Observatory, Indiana University, No. 106.Presently at Los Alamos Scientific Laboratories, Los Alamos, New Mexico. 相似文献
864.
Robert Howard 《Solar physics》1972,25(1):5-13
Observations of the magnetic fields in the polar regions of the Sun are presented for the period 1960–1971. At the start of this interval the fields at the two poles were consistently of opposite sign and averaged around 1 G. Early in 1961 the field in the south decreased suddenly and the field in the north decreased in strength slowly over the next few years. By the mid-1960's the fields at both poles were quite weak and irregular. Throughout the period of these observations the fields at both poles often showed a remarkable tendency to vary in unison. About the middle of 1971 the north polar field became significantly positive, first at lower latitudes, then above 70 °. An autocorrelation analysis of the polar fields in the north shows a weak rotation peak, indicating significant features in these regions. A comparison of field strengths in the east and west quadrants in the north suggests that even at the extreme polar latitudes the following polarity fields are inclined slightly toward the rotation and the preceding polarity field lines are inclined slightly to trail the rotation. 相似文献
865.
A clearly evident large-scale pattern in the interplanetary magnetic field during 1964 is used to search for a similar large-scale pattern in the solar magnetic field. It is found that such a pattern did exist in the photospheric field observations on both sides of the equator over a range of at least 40°N to 35°S. The pattern is basically similar at all these latitudes, and differs from that to be expected from solar differential rotation in three important respects. It is found that the solar magnetic pattern changed at all latitudes investigated within an interval of a few solar rotations. 相似文献
866.
867.
868.
Spectroscopic determinations of solar rotation 总被引:2,自引:0,他引:2
Spectral line shift data obtained from full-disk magnetograms recorded at Mt. Wilson are analyzed for differential rotation. The method of analysis is discussed and the results from the data for 1966 through 1968 are presented. The average equatorial velocity over this period is found to be 1.93 km/sec or 13.76 deg/day (sidereal). This corresponds to a sidereal period of 26.16 days. The average results are = 2.78 × 10-6 - 3.51 × 10-7 sin2
B - 4.43 × 10-7 sin4
B rad/sec, whereB is the solar latitude. This indicates a smaller decrease of angular velocity with latitude than found by earlier investigators. Variations from day to day are caused by large-scale short-lived velocity fields on the solar surface. There also appear to be secular variations.Currently at the Kitt Peak National Observatory, Tucson, Arizona. 相似文献
869.
870.
The importance of interstitial pore water as a vehicle for transport of dissolved ions between sediment at depth and the overlying ocean reservoir may be overestimated. The major cause of this overestimation is the assumption that the rate of ionic diffusion through the sediment is of a similar magnitude to the rate of reaction occurring within the sediment column. Examples are given to indicate that the above assumption may not be correct, at least for diagenetic sulfate reduction. Closed-system modeling, although approximate, is shown to be consistent, both qualitatively and isotopically, with measured changes that are observed for several sedimentary environments. 相似文献