全文获取类型
收费全文 | 62篇 |
免费 | 1篇 |
专业分类
地球物理 | 12篇 |
地质学 | 17篇 |
海洋学 | 2篇 |
天文学 | 30篇 |
自然地理 | 2篇 |
出版年
2017年 | 2篇 |
2016年 | 2篇 |
2013年 | 1篇 |
2012年 | 1篇 |
2011年 | 2篇 |
2009年 | 3篇 |
2008年 | 5篇 |
2007年 | 6篇 |
2006年 | 7篇 |
2005年 | 6篇 |
2004年 | 2篇 |
2003年 | 4篇 |
2002年 | 1篇 |
2001年 | 3篇 |
2000年 | 1篇 |
1999年 | 2篇 |
1997年 | 2篇 |
1996年 | 3篇 |
1992年 | 1篇 |
1990年 | 1篇 |
1989年 | 1篇 |
1988年 | 1篇 |
1987年 | 1篇 |
1984年 | 1篇 |
1983年 | 1篇 |
1982年 | 1篇 |
1981年 | 1篇 |
1978年 | 1篇 |
排序方式: 共有63条查询结果,搜索用时 15 毫秒
31.
We test for age and metallicity gradients in the Galactic Bulgebetween the two low extinction windows Baade's window (l = 1° .1b=−4° .8) and Sagittarius-I (l=1° .3 b=−2° .7). We derive ametallicity difference of ≤ 0.2 dex between BW andSGR-I window. This corresponds to a metallicity gradient
of 1.3 dexkpc-1. This steep gradient is reconcilable with the existence of ashort scale length inner component to the Bulge, most likely
thatprominent in the NIR, which perhaps forms a separate entitysuperimposed on the larger, optical Bulge. Through number counts
incolour-magnitude diagram around the turnoff for several fields andclusters, extending over a range in galactic longitude
we find no evidencefor a significant young stellar population in the GalacticBulge. Previous suggestions of the existence
of a significant youngstellar population have most likely incorrectly identified theforeground disk stars.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
32.
Jun Yi I.Yücel Akkutlu C.Özgen Karacan C.R. Clarkson 《International Journal of Coal Geology》2009,77(1-2):137-144
In this paper, single-component gas sorption and transient diffusion processes are described within coal matrix exhibiting bimodal pore structure. The coal matrix is treated as a poroelastic medium manifesting swelling and shrinkage effects due to the sorption of gas under effective overburden stress. Gas transport is considered Fickian with molecular (bulk) and surface diffusion processes simultaneously taking place in the macro- and micropores of coal, respectively. The numerical formulation is intended to be explicit in nature to investigate the influences of sorption phenomena on the macropore volumes and on the overall gas transport for the cases of gas uptake by and release from coal.Results of the study show the presence of hysteresis during a sorption–desorption cycle of the gas. It is also found that the overall gas transport takes place at a rate significantly less than that in the macropores only. Thus the existence of a retardation effect in the overall gas transport is concluded. This retardation effect is primarily due to the micropore resistances, in particular gas adsorption, and is independent of the changes in the macropore volumes. It is shown that macroporosity of the coal matrix may change during gas transport due to combined effects of pressure and sorption-induced swelling or shrinkage of the coal. It is estimated that the macroporosity variation is non-uniform in space and time, as it is expected in reality, and typically taking values less than ± 10 percent of the initial porosity. 相似文献
33.
Jessica L. McKenzie Gerry P. QuinnTy G. Matthews Jan BartonAlecia Bellgrove 《Estuarine, Coastal and Shelf Science》2011
Outflows from estuaries potentially contribute to the productivity of adjacent coastal waters, although most previous work has been on estuaries with considerable river discharge. We investigated the influence of estuary outflow on aspects of coastal sediments adjacent to two seasonally intermittent estuaries, the Curdies and Anglesea Rivers, in southwest Victoria, Australia. For each estuary, we measured sediment organic matter, microphytobenthic chlorophyll a and microbial utilization of carbon sources at three locations associated with each estuary: (1) inside estuary mouth, (2) estuary swash and (3) control swash (an open beach distant from any estuarine influences). Sampling occurred one week before and at one and nine weeks after both an artificial mouth opening and a separate natural flood at both estuaries. Significant temporal changes were detected for all three variables at the estuary mouth and estuary swash but the direction of change was inconsistent across the two estuaries and between the artificial mouth opening and natural flood. Organic matter in both estuaries showed no difference after the artificial mouth openings. Only Anglesea showed an increase in organic matter in the estuary mouth and estuary swash after the floods. Microphytobenthic chlorophyll a concentrations were highest when the estuary mouths were closed. Concentrations decreased at all locations at Curdies after the mouth was artificially opened. The estuary mouth at Anglesea sustained high chlorophyll concentrations and the estuary swash increased one week post artificial opening. The flood event resulted in an increase in chlorophyll a at the estuary mouth and swash at both estuaries, one week post flood. At Curdies, the microbial utilization of different carbon sources changed after both mouth events; estuary mouth and estuary swash showed similar patterns at one and nine weeks post opening. At Anglesea, the bacteria utilized different carbon sources between locations and the only significant interaction between location and time was post flood with change in carbon sources utilized by bacteria in the estuary mouth and estuary swash for one and nine weeks post flood. The southern coastline of Australia is characterized by estuaries with small catchments. This study highlights the spatial and temporal variability in the effects of the output of relatively small, intermittent estuaries on coastal sediment of adjacent beaches, particularly during prolonged periods of drought. 相似文献
34.
A. Collier Cameron D. M. Wilson R. G. West L. Hebb X.-B. Wang S. Aigrain F. Bouchy D. J. Christian W. I. Clarkson B. Enoch M. Esposito E. Guenther C. A. Haswell G. Hébrard C. Hellier K. Horne J. Irwin S. R. Kane B. Loeillet T. A. Lister P. Maxted M. Mayor C. Moutou N. Parley D. Pollacco F. Pont D. Queloz R. Ryans I. Skillen R. A. Street S. Udry P. J. Wheatley 《Monthly notices of the Royal Astronomical Society》2007,380(3):1230-1244
35.
36.
37.
38.
D. J. Christian D. L. Pollacco I. Skillen R. A. Street F. P. Keenan W. I. Clarkson A. Collier Cameron S. R. Kane T. A. Lister R. G. West B. Enoch A. Evans A. Fitzsimmons C. A. Haswell C. Hellier S. T. Hodgkin K. Horne J. Irwin A. J. Norton J. Osborne R. Ryans P. J. Wheatley D. M. Wilson 《Monthly notices of the Royal Astronomical Society》2006,372(3):1117-1128
39.
D. Pollacco I. Skillen A. Cameron D. Christian J. Irwin T. Lister R. Street R. West W. Clarkson N. Evans A. Fitzsimmons C. Haswell C. Hellier S. Hodgkin K. Horne B. Jones S. Kane F. Keenan A. Norton J. Osborne R. Ryans P. Wheatley 《Astrophysics and Space Science》2006,304(1-4):253-255
The WASP project and infrastructure supporting the SuperWASP Facility are described. As the instrument, reduction pipeline and archive system are now fully operative we expect the system to have a major impact in the discovery of bright exo-planet candidates as well in more general variable star projects. 相似文献
40.
R. A. Street D. J. Christian W. I. Clarkson A. Collier Cameron B. Enoch S. R. Kane T. A. Lister R. G. West D. M. Wilson A. Evans A. Fitzsimmons C. A. Haswell C. Hellier S. T. Hodgkin K. Horne J. Irwin F. P. Keenan A. J. Norton J. Osborne D. L. Pollacco R. Ryans I. Skillen P. J. Wheatley J. Barnes 《Monthly notices of the Royal Astronomical Society》2007,379(2):816-832