全文获取类型
收费全文 | 1705篇 |
免费 | 92篇 |
国内免费 | 48篇 |
专业分类
测绘学 | 59篇 |
大气科学 | 133篇 |
地球物理 | 365篇 |
地质学 | 609篇 |
海洋学 | 117篇 |
天文学 | 412篇 |
综合类 | 10篇 |
自然地理 | 140篇 |
出版年
2024年 | 5篇 |
2023年 | 13篇 |
2022年 | 10篇 |
2021年 | 36篇 |
2020年 | 42篇 |
2019年 | 40篇 |
2018年 | 82篇 |
2017年 | 72篇 |
2016年 | 81篇 |
2015年 | 74篇 |
2014年 | 79篇 |
2013年 | 113篇 |
2012年 | 68篇 |
2011年 | 98篇 |
2010年 | 81篇 |
2009年 | 91篇 |
2008年 | 89篇 |
2007年 | 91篇 |
2006年 | 76篇 |
2005年 | 60篇 |
2004年 | 64篇 |
2003年 | 49篇 |
2002年 | 48篇 |
2001年 | 36篇 |
2000年 | 44篇 |
1999年 | 34篇 |
1998年 | 22篇 |
1997年 | 24篇 |
1996年 | 19篇 |
1995年 | 11篇 |
1994年 | 13篇 |
1993年 | 11篇 |
1992年 | 16篇 |
1991年 | 8篇 |
1990年 | 9篇 |
1989年 | 6篇 |
1988年 | 6篇 |
1987年 | 7篇 |
1986年 | 10篇 |
1985年 | 12篇 |
1984年 | 7篇 |
1983年 | 9篇 |
1982年 | 5篇 |
1981年 | 7篇 |
1980年 | 7篇 |
1979年 | 8篇 |
1978年 | 7篇 |
1977年 | 5篇 |
1976年 | 5篇 |
1973年 | 4篇 |
排序方式: 共有1845条查询结果,搜索用时 93 毫秒
721.
Ian Alexander 《The Australian geographer》1988,19(1):117-130
This paper examines the strength of Western Australia's claim to be ‘the resource state’. It traces the history of the state's mineral development and points to close links between the development, the growth of the economy and the spread of settlement. The crucial role of the state government in facilitating capital investment and fostering a growth ideology is also highlighted. The paper argues that while resource development and capital investment have brought tangible economic benefits to Western Australia and the nation, certain costs have also been generated. Growth has caused damage to the physical environment and the once‐numerous Aboriginal population. Moreover, given the international commodity crisis of the 1980s, mineral export strength is no sure recipe for economic success. 相似文献
722.
D. M. Alexander † 《Monthly notices of the Royal Astronomical Society》2001,320(1):L15-L19
We present X-ray imaging spectroscopy of the extremely luminous infrared galaxy IRAS 09104+4109 obtained with the Chandra X-ray Observatory. With the arcsec resolution of Chandra , an unresolved source at the nucleus is separated from the surrounding cluster emission. A strong iron K line at 6.4 keV on a very hard continuum is detected from the nuclear source, rendering IRAS 09104+4109 the most distant reflection-dominated X-ray source known. Combined with the BeppoSAX detection of the excess hard X-ray emission, it provides further strong support for the presence of a hidden X-ray source of quasar luminosity in this infrared galaxy. Also seen is a faint linear structure to the north, which coincides with the main radio jet. An X-ray deficit in the corresponding region suggests an interaction between the cluster medium and the jet driven by the active nucleus. 相似文献
723.
Mutsumi KOMATSU Alexander N. KROT Mikhail I. PETAEV Alexander A. ULYANOV Klaus KEIL Masamichi MIYAMOTO 《Meteoritics & planetary science》2001,36(5):629-641
Abstract— Amoeboid olivine aggregates (AOAs) from the reduced CV chondrites Efremovka, Leoville and Vigarano are irregularly‐shaped objects, up to 5 mm in size, composed of forsteritic olivine (Fa<10) and a refractory, Ca, Al‐rich component. The AOAs are depleted in moderately volatile elements (Mn, Cr, Na, K), Fe, Ni‐metal and sulfides and contain no low‐Ca pyroxene. The refractory component consists of fine‐grained calcium‐aluminum‐rich inclusions (CAIs) composed of Al‐diopside, anorthite (An100), and magnesium‐rich spinel (~1 wt% FeO) or fine‐grained intergrowths of these minerals; secondary nepheline and sodalite are very minor. This indicates that AOAs from the reduced CV chondrites are more pristine than those from the oxidized CV chondrites Allende and Mokoia. Although AOAs from the reduced CV chondrites show evidence for high‐temperature nebular annealing (e.g., forsterite grain boundaries form 120° triple junctions) and possibly a minor degree of melting of Al‐diopside‐anorthite materials, none of the AOAs studied appear to have experienced extensive (>50%) melting. We infer that AOAs are aggregates of high‐temperature nebular condensates, which formed in CAI‐forming regions, and that they were absent from chondrule‐forming regions at the time of chondrule formation. The absence of low‐Ca pyroxene and depletion in moderately volatile elements (Mn, Cr, Na, K) suggest that AOAs were either removed from CAI‐forming regions prior to condensation of these elements and low‐Ca pyroxene or gas‐solid condensation of low‐Ca‐pyroxene was kinetically inhibited. 相似文献
724.
725.
726.
An extension to kinetic theory and hydrodynamic models is proposed that accounts for the existence of multi-particle contacts and leads to a correction of the cooling rate. The other hydrodynamic terms remain unchanged. In the presence of multi-particle contacts a class of different models leads to deviations from the classical inelastic hard sphere (IHS) results. For the homogeneous cooling state (HCS), as examined here, the theoretical results are found to be in perfect agreement with the numerical simulations.
We acknowledge partial support from the Deutsche Forschnugsgemeinschaft (DFG) and the Israel Science Foundation, grant no. 53/01. 相似文献
727.
728.
Alfvén wave turbulence is considered as the source of the non-thermal line broadenings observed in soft X-rays in solar flares. The waves are assumed to lose energy to particle acceleration and the temporal development for the case of Fermi acceleration,W(k)k
–2, is investigated. The decay of the wave energy density is compared to that of the non-thermal velocity for the event of 1980 June 29. The wave energy densities required to explain the degree of non-thermal broadening and its temporal characteristics are consistent with those typically inferred from-ray observations. A relationship between the degree of non-thermal broadening and-ray fluxes is predicted. In general, the larger the-ray flux the shorter the time scales for the decay of the wave energy. 相似文献
729.
Alexander R. McBirney 《Contributions to Mineralogy and Petrology》1998,132(1):103-105
Received: 15 August 1997 / Accepted: 30 January 1998 相似文献
730.
Side-scan sonar, seismic and core data are used to identify mega-flutes, transverse and ‘V’ shaped bedforms in turbidites around the Valencia channel mouth, north-west Mediterranean. Long-range side-scan sonar data reveal a broad, curved, asymmetric, channel, that widens and terminates downfan. The western channel bank near the channel mouth has been partly eroded by turbidity currents that spilled out of the channel. Transverse bedforms on the east of the channel floor are interpreted as antidunes and, if this interpretation is correct, they indicate that the flow was probably supercritical at least locally within the channel. Trains of mega-flutes, are incised into coarse-grained sediments of the channel floor near the channel mouth. The association of mega-flutes and antidunes is thought to be diagnostic of channel–lobe transitions on deep-sea fans. The mega-flutes pass downfan into an area of streaks that diverge at up to 45° and indicates flow expansion from the channel mouth. About 75 km downfan from the channel mouth, deep-towed side-scan data record transverse bedforms (interpreted as antidunes) passing downfan into an area covered by ‘V’ shaped bedforms with upflow pointing apices (named chevrons here). The chevrons are commonly c. 200 m from limb to limb and c. 2 m in amplitude with flow-parallel wavelengths of c. 400 m. We propose that chevrons were formed by a strong, probably supercritical (or near critical) turbidity current spreading from the channel mouth and flowing towards the Balearic Abyssal Plain. Thinning of the turbidity current, resulting from flow spreading would allow the Froude number to remain high up to 100 km from the channel mouth and could explain the observed reduction in antidune wavelength. 相似文献