全文获取类型
收费全文 | 6954篇 |
免费 | 332篇 |
国内免费 | 52篇 |
专业分类
测绘学 | 189篇 |
大气科学 | 442篇 |
地球物理 | 2345篇 |
地质学 | 2407篇 |
海洋学 | 474篇 |
天文学 | 1087篇 |
综合类 | 34篇 |
自然地理 | 360篇 |
出版年
2022年 | 45篇 |
2021年 | 128篇 |
2020年 | 136篇 |
2019年 | 109篇 |
2018年 | 276篇 |
2017年 | 272篇 |
2016年 | 405篇 |
2015年 | 294篇 |
2014年 | 360篇 |
2013年 | 433篇 |
2012年 | 356篇 |
2011年 | 405篇 |
2010年 | 317篇 |
2009年 | 369篇 |
2008年 | 328篇 |
2007年 | 252篇 |
2006年 | 257篇 |
2005年 | 208篇 |
2004年 | 201篇 |
2003年 | 161篇 |
2002年 | 150篇 |
2001年 | 143篇 |
2000年 | 105篇 |
1999年 | 93篇 |
1998年 | 117篇 |
1997年 | 88篇 |
1996年 | 60篇 |
1995年 | 47篇 |
1994年 | 70篇 |
1993年 | 53篇 |
1992年 | 63篇 |
1991年 | 47篇 |
1990年 | 66篇 |
1989年 | 47篇 |
1988年 | 42篇 |
1987年 | 38篇 |
1986年 | 36篇 |
1985年 | 41篇 |
1984年 | 37篇 |
1983年 | 44篇 |
1982年 | 39篇 |
1981年 | 34篇 |
1980年 | 35篇 |
1979年 | 40篇 |
1978年 | 38篇 |
1975年 | 32篇 |
1974年 | 33篇 |
1973年 | 37篇 |
1972年 | 33篇 |
1971年 | 40篇 |
排序方式: 共有7338条查询结果,搜索用时 15 毫秒
971.
Four different mountainous locations were selected in the Valencia region, East coast of the Iberian Peninsula, for fog water collection studies. Data for 2004 were obtained by means of an instrument ensemble consisting essentially of a passive cylindrical fog water collector, a raingauge, a wind direction and velocity sensor and a temperature and humidity probe. An approximate data reduction technique was also found for this specific ensemble to eliminate the simultaneous rain water component from the fog water measurements. Main results indicate that fog water collection holds significant potential in this region, and especially for southern locations. Annual rates of fog water yield can be as high as 7.0 l/m2/day in the southern locations, in contrast to 2.0 l/m2/day collected at one site in a northern location. The highest summer fog water yield was 4.6 l/m2/day, a relatively large value. Except for the summer period, fog episodes delivering sizeable water volumes are inherently coupled to rainfall. Hourly frequencies of fog collection were also examined to show a distinct daily cycle in summer, denoting orographic fog formation during this period. Lastly, winds were analysed to resolve the most suitable directions for fog collector alignment. 相似文献
972.
Spatial and temporal patterns of dry spell lengths in the Iberian Peninsula for the second half of the twentieth century 总被引:1,自引:1,他引:0
X. Lana M. D. Martínez A. Burgueño C. Serra J. Martín-Vide L. Gómez 《Theoretical and Applied Climatology》2008,91(1-4):99-116
Summary Daily pluviometric records of 43 meteorological stations across the Iberian Peninsula have permitted a detailed analysis of
dry spell patterns for the period 1951–2000 by distinguishing daily amount thresholds of 0.1, 1.0, 5.0 and 10.0 mm/day. The
analyses are based on three annual series, namely the number of dry spells, N, the average dry spell length, L, and the extreme dry spell length, L
max. First, the statistical significance of local trends for the annual series of N, L and L
max has been investigated by means of the Mann-Kendall test and significant field trends have been established by means of Monte
Carlo simulations. Clear signs of negative field trends are detected for N (1.0 and 10.0 mm/day) and L (0.1 mm/day). Second, the Weibull model fits well the empirical distributions of dry spell lengths for all the rain gauges,
whatever the daily amount threshold, with a well ranged spatial distribution of their parameters u and k. On the basis of the Weibull distribution, return period maps for 2, 5, 10, 25 and 50 years have been obtained for dry spell
lengths with respect to the four daily threshold levels. While for 0.1 and 1.0 mm/day the longest dry spells are expected
at the south of the Iberian Peninsula, for 5.0 and 10.0 mm/day they are mostly detected at the southeast. Finally, the elapsed
time between consecutive dry spells has been analysed by considering the same rain amount thresholds and different dry spell
lengths at increasing intervals of 10 days. This analysis makes evident a significant negative field trend of the elapsed
time between consecutive dry spells of lengths ranging from 10 to 20 days for daily amount thresholds of 1.0, 5.0 and 10.0 mm/day.
Authors’ addresses: X. Lana, C. Serra, Departament de Física i Enginyeria Nuclear, ETSEIB, Universitat Politècnica de Catalunya,
Av. Diagonal 647 planta 11, 08028 Barcelona, Spain; M. D. Marínez, Departament de Física Aplicada, Universitat Politècnica
de Catalunya, 08028 Barcelona, Spain; A. Burgue?o, Departament de Meteorologia i Astronomia, Universitat de Barcelona, 08028
Barcelona, Spain; J. Martín-Vide, L. Gómez, Grup de Climatologia, Universitat de Barcelona, 08028 Barcelona, Spain. 相似文献
973.
Investigation of regional climate models’ internal variability with a ten-member ensemble of 10-year simulations over a large domain 总被引:2,自引:1,他引:1
Previous investigations on regional climate models’ (RCM) internal variability (IV) were limited owing to small ensembles, short simulations and small domains. The present work extends previous studies with a ten-member ensemble of 10-year simulations performed with the Canadian Regional Climate Model over a large domain covering North America. The results show that the IV has no long-term tendency but rather fluctuates in time following the synoptic situation within the domain. The IV of mean-sea-level pressure (MSLP) and screen temperature (ST) show a small annual cycle with larger values in spring, which differs from previous studies. For precipitation (PCP), the IV shows a clear annual cycle with larger values in summer, as previously reported. The 10-year climatology of the IV for MSLP and ST shows a well-defined spatial distribution with larger values in the northeast of the domain, near the outflow boundary. A comparison of the IV of MSLP and ST in summer with the transient-eddy variance reveals that the IV is close to its maximum in a small region near the outflow boundary. Same analysis for PCP in summer shows that the IV reaches its maximum in most parts of the domain, except for a small region on the western side near the inflow boundary. Finally, a comparison of the 10-year climate of each simulation of the ensemble showed that the IV may have a significant impact on the climatology of some variables. 相似文献
974.
We present an analysis of a regional simulation of present-day climate (1981–1990) over southern South America. The regional
model MM5 was nested within time-slice global atmospheric model experiments conducted by the HadAM3H model. We evaluate the
capability of the model in simulating the observed climate with emphasis on low-level circulation patterns and surface variables,
such as precipitation and surface air mean, maximum and minimum temperatures. The regional model performance was evaluated
in terms of seasonal means, seasonal cycles, interannual variability and extreme events. Overall, the regional model is able
to capture the main features of the observed mean surface climate over South America, its seasonal evolution and the regional
detail due to topographic forcing. The observed regional patterns of surface air temperatures (mean, maxima and minima) are
well reproduced. Biases are mostly within 3°C, temperature being overestimated over central Argentina and underestimated in
mountainous regions during all seasons. Biases in northeastern Argentina and southeastern Brazil are positive during austral
spring season and negative in other seasons. In general, maximum temperatures are better represented than minimum temperatures.
Warm bias is larger during austral summer for maximum temperature and during austral winter for minimum temperature, mainly
over central Argentina. The broad spatial pattern of precipitation and its seasonal evolution are well captured; however,
the regional model overestimates the precipitation over the Andes region in all seasons and in southern Brazil during summer.
Precipitation amounts are underestimated over the La Plata basin from fall to spring. Extremes of precipitation are better
reproduced by the regional model compared with the driving model. Interannual variability is well reproduced too, but strongly
regulated by boundary conditions, particularly during summer months. Overall, taking into account the quality of the simulation,
we can conclude that the regional model is capable in reproducing the main regional patterns and seasonal cycle of surface
variables. The present reference simulation constitutes the basis to examine the climate change simulations resulting from
the A2 and B2 forcing scenarios which are being reported in a separate study. 相似文献
975.
R. Dimitrova Jean-François Sini K. Richards M. Schatzmann M. Weeks E. Perez García C. Borrego 《Boundary-Layer Meteorology》2009,131(2):223-243
Micrometeorological conditions in the vicinity of urban buildings strongly influence the requirements that are imposed on
building heating and cooling. The goal of the present study, carried out within the Advance Tools for Rational Energy Use
towards Sustainability (ATREUS) European research network, is the evaluation of the wind field around buildings with walls
heated by solar radiation. Two computational fluid dynamics (CFD) codes were validated against extensive wind-tunnel observations
to assess the influence of thermal effects on model performance. The code selected from this validation was used to simulate
the wind and temperature fields for a summer day in a specific region of the city of Lisbon. For this study, the meteorological
data produced by a non-hydrostatic mesoscale atmospheric model (MM5) were used as boundary conditions for a CFD code, which
was further applied to analyze the effects of local roughness elements and thermodynamic conditions on the air flow around
buildings. The CFD modelling can also provide the inflow parameters for a Heating, Ventilation and Air Conditioning (HVAC)
system, used to evaluate the building energy budgets and to predict performance of the air-conditioning system. The main finding
of the present three-dimensional analyses is that thermal forcing associated with the heating of buildings can significantly
modify local properties of the air flow. 相似文献
976.
L. González-Miqueo D. Elustondo E. Lasheras R. Bermejo J. M. Santamaría 《Journal of Atmospheric Chemistry》2009,62(1):59-72
A biomonitoring survey using the moss species Hypnum cupressiforme Hedw. was performed in the North of Navarra (Spain) in 2006. The levels of V, Cr, Mn, Ni, Cu, Zn, As, Zr, Cd, Hg and Pb,
and the total nitrogen content were determined in the samples by means of ICP-MS, CV-AA, and the Kjeldahl method. PCA analysis
showed a differentiation between lithogenic (V, Cr, Mn, Ni, As and Zr) and anthropogenic elements (Mn, Cu, Zn, Cd, Hg and
Pb). Spatial distribution maps were drawn using the kriging method, in order to identify the most affected areas and the main
pollution sources. A similar spatial distribution was observed for the elements belonging to each group separated by the PCA,
showing an important contribution from metal industries located in the Basque Country, as well as influence of long-range
transboundary pollution processes. Background levels were also determined for the study area, along with the contamination
factor for the different elements analysed. Mosses seemed to be good biomonitors of N deposition in areas of accumulation. 相似文献
977.
José Antonio Belinchón 《Astrophysics and Space Science》2009,323(3):307-315
We study a massive cosmic strings with BII symmetries cosmological models in two contexts. The first of them is the standard
one with a barotropic equation of state. In the second one we explore the possibility of taking into account variable “constants”
(G and Λ). Both models are studied under the self-similar hypothesis. We put special emphasis in calculating the numerical values
for the equations of state. We find that for ω∈(0,1], G, is a growing time function while Λ, behaves as positive decreasing time function. If ω=0, both “constants”, G and Λ, behave as true constants. 相似文献
978.
István Horváth 《Astrophysics and Space Science》2009,323(1):83-86
The BeppoSAX Catalog has been very recently published. In this paper we analyze—using the Maximum Likelihood (ML) method—the
duration distribution of the 1003 GRBs listed in the catalog with duration. The ML method can identify the long and the intermediate
duration groups. The short population of the bursts is identified only at a 96% significance level. MC simulation has been
also applied and gives a similar significance level; 95%. However, the existence of the short bursts is not a scientific question
after the Compton Gamma-Ray Observatory’s observation. Our minor result is this well-known fact that in the BeppoSAX data
the short bursts are under-represented, mainly caused by the different triggering system. Our major result is the identification
of the intermediate group in the BeppoSAX data. Therefore, four different satellites (CGRO, Swift, RHESSI and BeppoSAX) observed
the intermediate type Gamma-Ray Burst. 相似文献
979.
Sergiy Silich Guillermo Tenorio-Tagle Casiana Muñoz-Tuñón 《Astrophysics and Space Science》2009,324(2-4):215-217
The existence of compact H?ii regions around massive stellar clusters with ages exceeding several Myr challenges our understanding of the physical processes occurring inside such clusters, and their impact on the interstellar medium of the host galaxy. Here, we summarize our recent results dealing with the hydrodynamics of matter ejected by massive stars inside the cluster and show that compact H?ii regions found around some massive clusters may indicate that these are evolving in a bimodal hydrodynamic regime. The latter is characterized by the accumulation of the injected matter in the central, thermally unstable zone, and by the ejection of mass supplied by massive stars in the outer regions of the cluster. 相似文献
980.
Javier Rodríguez Zaurín Joanna Holt Clive N. Tadhunter Rosa M. González Delgado 《Astrophysics and Space Science》2009,324(2-4):225-229
We use long-slit spectra taken with the William Herschel Telescope on La Palma and high-resolution Hubble Space Telescope imaging to study the gas kinematic in the halo of the ultraluminous infrared/radio galaxy PKS1345+12 (z=0.122). Our long-slit spectra show line splitting at the locations of massive star clusters ( $10^{6}<M_{\mathrm{SSC}}^{\mathrm{YSP}}<10^{7}$ M⊙), indicating that they are moving at up to 450 km?s?1 with respect to the local ambient gas. Given their kinematics, it is plausible that these super star clusters have been formed either in fast-moving gas streams or tidal tails that are falling back into the nuclear regions as part of the merger process, or as a consequence of jet-induced star formation linked to the extended, diffuse radio emission detected in the halo of the galaxy. 相似文献