全文获取类型
收费全文 | 174篇 |
免费 | 4篇 |
专业分类
大气科学 | 33篇 |
地球物理 | 30篇 |
地质学 | 72篇 |
海洋学 | 12篇 |
天文学 | 23篇 |
综合类 | 1篇 |
自然地理 | 7篇 |
出版年
2021年 | 2篇 |
2020年 | 3篇 |
2018年 | 4篇 |
2016年 | 2篇 |
2015年 | 3篇 |
2014年 | 3篇 |
2013年 | 7篇 |
2012年 | 7篇 |
2011年 | 7篇 |
2010年 | 6篇 |
2009年 | 7篇 |
2008年 | 6篇 |
2007年 | 10篇 |
2006年 | 3篇 |
2005年 | 5篇 |
2004年 | 4篇 |
2003年 | 8篇 |
2002年 | 7篇 |
2000年 | 5篇 |
1999年 | 1篇 |
1998年 | 5篇 |
1997年 | 1篇 |
1996年 | 2篇 |
1995年 | 2篇 |
1994年 | 3篇 |
1993年 | 1篇 |
1992年 | 1篇 |
1991年 | 2篇 |
1990年 | 2篇 |
1989年 | 1篇 |
1988年 | 2篇 |
1987年 | 2篇 |
1985年 | 4篇 |
1984年 | 2篇 |
1983年 | 3篇 |
1981年 | 3篇 |
1980年 | 5篇 |
1979年 | 4篇 |
1978年 | 4篇 |
1977年 | 5篇 |
1976年 | 1篇 |
1975年 | 4篇 |
1974年 | 8篇 |
1973年 | 2篇 |
1968年 | 1篇 |
1961年 | 1篇 |
1949年 | 1篇 |
1935年 | 1篇 |
1927年 | 1篇 |
1925年 | 2篇 |
排序方式: 共有178条查询结果,搜索用时 15 毫秒
81.
Edgar A. Rhodes Larry G. Evans Larry R. Nittler Richard D. Starr Ann L. Sprague David J. Lawrence Timothy J. McCoy Karen R. Stockstill-Cahill John O. Goldsten Patrick N. Peplowski David K. Hamara William V. Boynton Sean C. Solomon 《Planetary and Space Science》2011,59(15):1829-1841
During its three flybys of Mercury, the MESSENGER spacecraft made the first detection of gamma-ray emission from the planet's surface. With a closest approach distance of ∼200 km, the flybys provided an opportunity to measure elemental abundances of Mercury's near-equatorial regions, which will not be visited at low altitude during MESSENGER's orbital mission phase. Despite being limited by low planetary photon flux, sufficient counts were accumulated during the first two flybys to estimate bounds on abundances for some elements having relatively strong gamma-ray spectral peaks, including Si, Fe, Ti, K, and Th. Only for Si is the standard deviation σ sufficiently small to conclude that this element was detected with 99% confidence. Iron and potassium are detected at the 2−σ (95% confidence) level, whereas only upper bounds on Ti and Th can be determined. Relative to a Si abundance assumed to be 18 weight percent (wt%), 2−σ upper bounds have been estimated as 9.7 wt% for Fe, 7.0 wt% for Ti, 0.087 wt% for K, and 2.2 ppm for Th. The relatively low upper bound on K rules out some previously suggested models for surface composition for the regions sampled. Upper bounds on Fe/Si and Ti/Si ratios are generally consistent with Ti and Fe abundances estimated from the analysis of measurements by the MESSENGER Neutron Spectrometer during the flybys but are also permissive of much lower concentrations. 相似文献
82.
We present new results on the recently discovered 69 ms X-ray pulsar AXS J161730-505505, the sixth youngest example of a rotation-powered pulsar. We have undertaken a comprehensive X-ray-observing campaign of AXS J161730-505505 with the ASCA, BeppoSAX, and RXTE observatories and follow its long-term spin-down history between 1989 and 1999 using these observations and archival Ginga and ASCA data sets. The spin-down is not simply described by a linear function as originally thought, but instead we find evidence of a giant glitch (DeltaP&solm0;P greater, similar10-6) between 1993 August and 1997 September, perhaps the largest yet observed from a young pulsar. The glitch is well described by steps in P and P&d2; accompanied by a persistent P&d3; similar to those seen in the Vela pulsar. The pulse profile of AXS J161730-505505 presents a single asymmetric peak that is maintained over all observation epochs. The energy spectrum is also steady over time, characterized by a highly absorbed power law with a photon index Gamma=1.4+/-0.2, consistent with that found for other young rotation powered pulsars. 相似文献
83.
84.
David J. Lawrence John K. Harmon William C. Feldman John O. Goldsten David A. Paige Patrick N. Peplowski Edgar A. Rhodes Christina M. Selby Sean C. Solomon 《Planetary and Space Science》2011,59(13):1665-1669
From radar images of Mercury's poles and MESSENGER Neutron Spectrometer (NS) measurements obtained during the spacecraft's flybys of Mercury, predictions of neutron count rates and their uncertainties are calculated for Mercury's north polar region as of the end of the MESSENGER primary orbital mission. If Mercury's poles contain large amounts of water ice, as has been suggested on the basis of the radar data, then during the one-year-long orbital mission the NS should detect signals indicative of excess polar hydrogen with a significance of at least 4σ, where σ is the standard deviation derived from Poisson counting statistics. If the polar deposits are not enriched with hydrogen, but are dominated by other elements, such as sulfur, then the MESSENGER neutron measurements should be able to confirm the absence of deposits having surface concentrations in excess of 50 wt% H2O on permanently shadowed floors of craters near Mercury's north pole. Because of the large spatial footprint of the NS data, individual polar deposits will not be spatially resolved, but longitudinal asymmetries may be detected if residual systematic uncertainties are sufficiently low. 相似文献
85.
A. Stettler P. Eberhardt J. Geiss N. Grögler 《Earth and Planetary Science Letters》1974,23(3):453-461
39Ar-40Ar ages and37Ar-38Ar exposure ages of samples representing four different lithologies of the Apollo 17 station 7 boulder were measured. The age of the dark veinlet material77015of3.98 ± 0.04AE is interpreted as representing the time of intrusion of this veinlet into the 77215 clast. The data obtained so far indicate that the vesicular basalt 77135 formed 100–200 m.y. later. However, this has to be confirmed by39Ar-40Ar investigations on separated mineral and/or grain-size fractions. A small clast enclosed in the 77135 basalt gives a well-defined high temperature age of3.99 ± 0.02AE. A sample of the noritic clast 77215 gave4.04 ± 0.03AE, the highest age found so far in this boulder. The39Ar-40Ar ages obtained are in agreement with the age relationships deduced from the stratigraphic evidence.Taking into account the shielding by the boulder itself, an average37Ar-38Ar exposure age of(27.5 ± 2.5)m.y. is obtained for the samples collected from the boulder. 相似文献
86.
87.
88.
A granitic batholith in the Tso Morari Culmination of the most internal High Himalayan thrust sheets (Ladakh Himalaya, India) has been investigated by Rb/Sr isotopic methods as well as by typological studies on its zircon population (Pupin 1980). The good alignment and spread of the single muscovite and the 6 whole rock data points allow the tracing of a fairly good isochron of 460±8 Ma which may be considered as the granite's crystallisation age. Its Sr initial ratio (I.R.) of 0.7365±2 is very high even in respect to other anatectic granites of this suite known in the Himalayas and in continental blocks to the north. In terms of the lower Cambrian to middle Ordovician ages known for this granitic suite, the Nyimaling Granite is among the youngest. The zircon population perfectly confirms isotope data interpretation and field observations inasmuch as it is characteristic for aluminous, intrusive granites of crustal origin (cf. high Sr I.R.); moreover, the batholith is intrusive into Lower Cambrian metasediments affected by a marked contact metamorphism and a regional overprint of greenschist facies. Its crustal level is thus very high. 相似文献
89.
Substitution mechanisms and solubility of titanium in phlogopites from rocks of probable mantle origin 总被引:1,自引:0,他引:1
Previously proposed substitution mechanisms for Ti in phlogopites, based on experimental studies and crystal chemistry, have
been examined using data for 81 phlogopites from mantle-derived rocks (primarily as nodules in kimberlites and also from alkali
basalts, lamprophyres and carbonatites), 49 phlogopites from high-K rocks with basaltic affinities, and from 32 phlogopites
crystallized in high pressure experiments mainly on high-K rock compositions. For the majority of phlogopites from the kimberlite
group and for all those crystallized in the experimental studies, the substitution of Ti can be represented by a combination
of the mechanisms represented by 2Mg[VI]⇌ Ti[VI]□[VI] and Mg[VI]2Si[IV]⇌Ti[VI]2Al[IV]. Some phlogopites in ultrapotassic rocks have only the former substitution mechanism. The Ti contents of phlogopites generally
increase with decreasing octahedral site occupancy and decreasing Si+Al[VI]. For the phlogopites crystallized in the experiments on high-K rocks, the solubility of Ti increases with increasing fO2 and temperature, and possibly with decreasing pressure at constant fO2. The effect of the composition of the liquids used in the experimental studies from which these phlogopites have crystallized
has only minor effect on either the substitution mechanism or the solubility of Ti in phlogopites. This suggests that phlogopite
in high-K rocks may be a potential geothermometer and possibly a geobarometer. 相似文献
90.
Edgar L. Andreas Reginald J. Hill James R. Gosz Douglas I. Moore William D. Otto Achanta D. Sarma 《Boundary-Layer Meteorology》1998,86(3):409-420
From a set of turbulence data collected with a three-axis sonic anemometer/thermometer and described in a companion paper, we simulate the eddy-accumulation process for sensible heat and momentum fluxes. The resulting eddy-accumulation coefficient for momentum clearly depends on surface-layer stability; at neutral stability, its value is 0.63. On supplementing the scalar eddy-accumulation coefficients that we derive from our sensible heat flux data with values of sensible and latent heat flux coefficients reported by Businger and Oncley, we also find that scalar eddy-accumulation coefficients depend on stability, though more weakly than does the momentum coefficient. The coefficients for sensible and latent heat show no significant difference; we, thus, fit them with one function of stability whose value is 0.52 for neutral stratification. 相似文献