全文获取类型
收费全文 | 1445篇 |
免费 | 52篇 |
国内免费 | 18篇 |
专业分类
测绘学 | 30篇 |
大气科学 | 163篇 |
地球物理 | 359篇 |
地质学 | 442篇 |
海洋学 | 126篇 |
天文学 | 259篇 |
综合类 | 1篇 |
自然地理 | 135篇 |
出版年
2023年 | 7篇 |
2022年 | 8篇 |
2021年 | 26篇 |
2020年 | 25篇 |
2019年 | 21篇 |
2018年 | 38篇 |
2017年 | 35篇 |
2016年 | 47篇 |
2015年 | 32篇 |
2014年 | 55篇 |
2013年 | 70篇 |
2012年 | 42篇 |
2011年 | 82篇 |
2010年 | 64篇 |
2009年 | 90篇 |
2008年 | 73篇 |
2007年 | 67篇 |
2006年 | 65篇 |
2005年 | 60篇 |
2004年 | 43篇 |
2003年 | 66篇 |
2002年 | 31篇 |
2001年 | 30篇 |
2000年 | 34篇 |
1999年 | 24篇 |
1998年 | 18篇 |
1997年 | 18篇 |
1996年 | 18篇 |
1995年 | 16篇 |
1994年 | 17篇 |
1993年 | 18篇 |
1992年 | 16篇 |
1991年 | 14篇 |
1990年 | 11篇 |
1989年 | 8篇 |
1988年 | 10篇 |
1987年 | 13篇 |
1986年 | 15篇 |
1985年 | 22篇 |
1984年 | 25篇 |
1983年 | 25篇 |
1982年 | 27篇 |
1981年 | 11篇 |
1980年 | 23篇 |
1979年 | 14篇 |
1978年 | 12篇 |
1977年 | 6篇 |
1975年 | 4篇 |
1974年 | 5篇 |
1973年 | 4篇 |
排序方式: 共有1515条查询结果,搜索用时 15 毫秒
1.
2.
Gordon H. Pettengill Steven J. Ostro Irwin I. Shapiro Brian G. Marsden Donald B. Campbell 《Icarus》1979,40(3):350-354
Radar observations of the asteroid 1580 Betulia, made at a wavelength of 12.6 cm, show a mean radar cross section of 2.2 ± 0.8 km2 and a total spectral bandwidth of 26.5 ± 1.5 Hz. Combining our bandwidth measurements with the optically determined rotation period sets a lower limit to the asteroid's radius of 2.9 ± 0.2 km. 相似文献
3.
Radiative recombination of N and O provides a significant source for auroral emission in the γ and δ bands of NO with selective population of vibrational levels in the A2Σ+ and C2Π states. This mechanism may account for emissions detected near 2150 Å. Models are derived for the auroral ionosphere and include estimates for the concentrations of N and NO. The concentration of NO is estimated to have a value of about 108 cm?1 near 140 km in an IBC III aurora. The corresponding density for N is about 5 × 107cm?3 and the concentration ratio has a value of about 5.5. 相似文献
4.
Many applied dispersion models require the knowledge of boundary-layer parameters such as sensible heat flux,Q
H
, friction velocity,u
*, and turbulent energy components, w and
v
. Formulas are suggested for calculating these parameters over a wide variety of types of ground surfaces, based on simple observations of wind speed near the ground and fractional cloud cover, and specification of constants such as roughness length, albedo, and soil moisture availability. Observations ofu
*,Q
H
,
w
, and
v
during field experiments in St. Louis and Indianapolis are used to test the formulas for urban sites. Relative errors of about ±20% in the predictions are seen to occur whenu
*,Q
H
,
w
, and
v
are large. However, when these quantities are small (e.g.,u
* < 0.2 m/s), the errors in the predictions are as large as the mean value of the quantity itself.In addition, it is concluded from studies of available field data and theories that the magnitude of
w
is not well-known at elevations above about 100m during the late afternoon and night. Some simple parameterizations for
w
. are suggested that are consistent with the observed steady decrease in ground-level concentration in the afternoon and the sudden increase in concentration that can occur a few hours after sunset due to wind shears associated with a low-level jet, for continuous plumes emitted from moderate to tall stacks. 相似文献
5.
S. P. Vyas M. D. Steven K. W. Jaggard 《Journal of the Indian Society of Remote Sensing》2005,33(2):315-321
The present work was aimed to compare the abilities of radar and optical satellite data to estimate crop canopy cover, which
is a key component of productivity estimates. Three ERS-1 SAR images were obtained of East Anglia (UK) in 1995 and one ERS-2
SAR image in 1996. The images covered a study area around the IACR Brooms Barn Sugar Beet Research Institute. Field data comprising
radiometric and biophysical measurements of the crop canopy were collected in two fields from June 22 to August 3, 1995 to
coincide with ERS-1 SAR overpass dates. In 1996, field data were collected in two fields from June 11 to July 29 on a weekly
basis. A previously calibrated version of the water cloud model was inverted to estimate Leaf Area Index (LAI) from ERS-1
and ERS-2 SAR backscatter and soil moisture samples. Canopy cover was estimated from the radar-estimated LAI using a standard
exponential relationship that has a well-established coefficient for sugar beet.
Radio-metrically and atmospherically corrected data from three SPOT images in 1995 and one SPOT image in 1996 were used to
calculate the Optimised Soil Adjusted Vegetation Index (OSAVI), from which crop canopy cover was estimated using a relationship
determined previously by canopy modelling. The crop cover values estimated by satellite were in good agreement with those
measured on ground with the Parkinson radiometer. Radar data may be able to provide useful estimates of canopy cover for crop
production modelling, especially in the case of loss of optical data due to cloud. 相似文献
6.
Berman’s (1983) activity-composition model for CaO-MgO-Al2O3-SiO2 liquids is used to calculate the change in bulk chemical and isotopic composition during simultaneous cooling, evaporation, and crystallization of droplets having the compositions of reasonable condensate precursors of Types A and B refractory inclusions in CV3 chondrites. The degree of evaporation of MgO and SiO2, calculated to be faithfully recorded in chemical and isotopic zoning of individual melilite crystals, is directly proportional to evaporation rate, which is a sensitive function of PH2, and inversely proportional to the droplet radius and cooling rate. When the precursors are partially melted in pure hydrogen at peak temperatures in the vicinity of the initial crystallization temperature of melilite, their bulk chemical compositions evolve into the composition fields of refractory inclusions, mass-fractionated isotopic compositions of Mg, Si, and O are produced that are in the range of the isotopic compositions of natural inclusions, and melilite zoning profiles result that are similar to those observed in real inclusions. For droplets of radius 0.25 cm evaporating at PH2 = 10−6 bar, precursors containing 8 to 13 wt.% MgO and 20 to 23% SiO2 evolve into objects similar to compact Type A inclusions at cooling rates of 2 to 12 K/h, depending on the precise starting composition. Precursors containing 13 to 14 wt.% MgO and 23 to 26% SiO2 evolve into objects with the characteristics of Type B1 inclusions at cooling rates of 1.5 to 3 K/h. The relatively SiO2-poor members of the Type B2 group can be produced from precursors containing 14 to 16 wt.% MgO and 27 to 33% SiO2 at cooling rates of <1 K/h. Type B2’s containing 27 to 35 wt.% SiO2 and <12% MgO require precursors with higher SiO2/MgO ratios at MgO > 15% than are found on any condensation curve. The characteristics of fluffy Type A inclusions, including their reversely zoned melilite, can only be understood in the context of this model if they contain relict melilite. 相似文献
7.
8.
9.
Edith L Gego P. Steven Porter John S. Irwin Christian Hogrefe S. Trivikrama Rao 《Pure and Applied Geophysics》2005,162(10):1919-1939
Airborne fine particulate matter across the United States is monitored by different networks, the three prevalent ones presently being the Clean Air Status and Trend Network (CASTNet), the Interagency Monitoring of PROtected Visual Environment Network (IMPROVE) and the Speciation and Trend Network (STN). If combined, these three networks provide speciated fine particulate data at several hundred locations throughout the United States. Yet, differences in sampling protocols and samples handling may not allow their joint use. With these concerns in mind, the objective of this study is to assess the spatial and temporal comparability of the sulfate, nitrate and ammonium concentrations reported by each of these networks. One of the major differences between networks is the sampling frequency they adopted. While CASTNet measures pollution levels on seven-day integrated samples, STN and IMPROVE data pertain to 24-hour samples collected every three days. STN and IMPROVE data therefore exhibit considerably more short-term variability than their CASTNet counterpart. We show that, despite their apparent incongruity, averaging the data with a window size of four to six weeks is sufficient to remove the effects of differences in sampling frequency and duration and allow meaningful comparison of the signals reported by the three networks of concern. After averaging, all the sulfate and, to a lesser degree, ammonium concentrations reported are fairly similar. Nitrate concentrations, on the other hand, are still divergent. We speculate that this divergence originates from the different types of filters used to collect particulate nitrate. Finally, using a rotated principal component technique (RPCA), we determined the number and the geographical organization of the significant temporal modes of variation (clusters) detected by each network for the three pollutants of interest. For sulfate and ammonium, the clusters’ geographical boundaries established for each network and the modes of variations within each cluster seem to correspond. RPCA erformed on nitrate concentrations revealed that, for the CASTNet and IMPROVE networks, the modes of variation do not correspond to unified geographical regions but are found more sporadically. For STN, the clustered areas are unified and easily delineable. We conclude that the possibility of jointly using the data collected by CASTNet, IMPROVE and STN has to be weighed pollutant by pollutant. While sulfate and ammonium data show some potential for joint use, at this point, combining the nitrate data from these monitoring networks may not be a judicious choice. 相似文献
10.