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11.
T. K. Saha 《洁净——土壤、空气、水》1991,19(2):175-179
Phosphorus is considered to be one of the most important factors in the maintenance of an aquatic eco-system. The study deals with the relation of available inorganic phosphate in water with phytoplankton abundance. The phytoplankton count ranged between 487 and 1711 indiv./l, while phosphate ranged between 0.18 and 1.23 mg/l. A maximum population of phytoplankton was observed in the month of January 1988 and a minimum observed in April 1988. The correlation between the changes in phosphate concentration and phytoplankton abundance revealed an inverse relationship (r= ?0.0773, P>0.05), and the regression is expressed by Y = 370 + 755 (x), indicating its link in the cycle of autotrophs though not significantly. 相似文献
12.
A simply defined, accurate and efficient criterion of selecting a spectral-band combination for improved land use/land cover classification using remote sensing data is discussed. Results indicate that Brightness Value Overlapping Index (BVOI) is very effective in measuring the degree of overlap in brightness values among land cover types and in selecting suitable spectral-band combination for landuse classification. The results of BVOI are also compared with the results of another band-combination selecting index - Optimum Index Factor (OIF). 相似文献
13.
Rocket-borne observations of the extinction of solar hydrogen Lyman-alpha radiation made during the solar eclipses of 20 May 1966 at Karistos for normal and 44% visibility and of 7 March 1970 at East Quoddy for normal, 10% and 0.6% visibility have been used to study the variation of temperature in the mesosphere during these events. It is seen that near the mesopause the decrease of temperature at Karistos is by 20° K for 44% visibility and at East Quoddy by 100° K for 0.6% visibility. Possible causes of these temperature variationsvis-a-vis molecular oxygen and pressure variations have been briefly discussed. 相似文献
14.
Syntectonic plutons emplaced in shallow crust often contain intermediate-to low-temperature deformation microstructures but
lack a high-temperature, subsolidus deformation fabric, although the relict magmatic fabric is preserved. The Proterozoic
Vellaturu granite emplaced at the eastern margin of the northern Nallamalai fold belt, south India during the late phase of
regional deformation has a common occurrence of intermediate-to low-temperature deformation fabric, superimposed over magmatic
fabric with an internally complex pattern. But high-T subsolidus deformation microstructure and fabric are absent in this
pluton. The main crystal plastic deformation and fluid enhanced reaction softening was concentrated along the margin of the
granite body. Resulting granite mylonites show Y-maximum c-axis fabric in completely recrystallized quartz ribbonds, dynamic recrystallization of perthites, and myrmekite indicative
of fabric development under intermediate temperature (∼ 500–400°C). The weakly-deformed interior shows myrmekite, feldspar
microfracturing and limited bulging recrystallization of quartz. The abundance of prism subgrain boundaries is indicative
of continuing deformation through low-temperature (∼ 300°C). The relative rates of cooling influenced by advective heat transfer
and deformation of the pluton seem to control the overall subsolidus fabric development. The rapid advective heat transfer
from the interior in the early stages of subsolidus cooling was followed by slow cooling through intermediate temperature
window as a well-developed phyllosilicate rich mylonitic skin around the granite body slowed down conductive heat loss. Low-T
crystal plastic deformation of quartz was effected at a late stage of cooling and deformation of the shallow crustal granite
body emplaced within the greenschist facies Nallamlai rocks. 相似文献
15.
The origin of hydrodynamic turbulence in rotating shear flow is a long standing puzzle.Resolving it is especially important in astrophysics when the flow's angular momentum profile is Keplerian which forms an accretion disk having negligible molecular viscosity.Hence,any viscosity in such systems must be due to turbulence,arguably governed by magnetorotational instability,especially when temperature T ≥10 5.However,such disks around quiescent cataclysmic variables,protoplanetary and star-forming disks,and t... 相似文献
16.
We make a detailed analysis of cross-correlation and time-lag between monthly data of galactic cosmic rays (GCRs) intensity and different solar activity indices (e.g., sunspot number, sunspot area, green coronal Fe line and 10.7 cm solar radio flux) during 19–23 solar cycles. GCRs time-series data from Kiel neutron monitor station and solar data from the last 50 years period, covering five solar cycles (19–23), and alternating solar polarity states (i.e., five A < 0 and four A > 0) have been investigated. We find a clear asymmetry in the cross-correlation between GCRs and solar activity indicators for both odd and even-numbered solar cycles. The time-lags between GCRs and solar parameters are found different in different solar cycles as well as in the opposite polarity states (A < 0 and A > 0) within the same solar cycle. Possible explanations of the observed results are discussed in light of modulation models, including drift effects. 相似文献
17.
Evaluation of the intermediate-term periodicities in solar and cosmic ray activities during cycle 23
In this paper we investigate the presence and temporal evolution of galactic cosmic rays (GCRs) time-series and three solar
parameters, namely the daily sunspot number, the coronal green line and the 10.7 cm solar radio flux over the period 1996–2003
by the wavelet technique. A number of short- and intermediate-term quasi-periodicities were also detected in both GCR and
solar parameters. For the short-term range, we have identified quasi-periods of 16–30 days, 40–55 days, 60–70 days, 80–90 days
and 80–100 days. In the case of intermediate range, the significant periods were 120–140 days, 150–170 days, 190–210 days,
240–260 days, ≈1.09 yr. and ≈1.23 yr. The wavelet power spectra show that all the above-mentioned periods are intermittent
in nature and occurred in different time-series in different intervals. The result exhibits that the well-known “Rieger period”
of (150–160 days) was prominent in both GCR and solar data sets during the ascending phase of cycle 23. Possible reasons behind
the observed periods were discussed with the help of previous results and existing numerical models. 相似文献
18.
In Jabalpur area about 18 m to 45 m thick Lameta Formation is stratigraphically divisible into five lithounits namely, Green
Sandstone, Lower Limestone, Mottled Nodular Beds, Upper Limestone and Upper Sandstone. Having differentiated lithofacies constitution
and here grouped as facies associations, these units are intensively burrowed and sparingly fossiliferous. Ichnogenera including
Arenicolites, Calycraterion, Fucusopsis, Laevicyclus, Macanopsis, Ophiomorpha, Paleomeandron, Rhizocorallium, Stipsellus,
Thalassinoides and Zoophycos are recovered from the Lower Limestone, Mottled Nodular Beds and Upper Limestone associations of the Lameta Formation of
Jabalpur area.Among these, Arenicolites, Calycraterion, Laevicyclus, Ophiomorpha, Rhizocorallium, Stipsellus and Thalassinoides belong to mixed Skolithos and Cruziana ichnofacies and indicate sandy backshore to sublittoral condition of deposition. Additionally rhyzocretes, some times chertified,
are also present in different parts of the Lameta Formation. Ichnofacies assemblage supported by sedimentological information
suggests that the Lameta Formation of Jabalpur area was deposited in coastal marine settings where sediments were subaerially
exposed intermittently. 相似文献
19.
Abhishek Saha Avik Dhang Jyotisankar Ray Suvankar Chakraborty David Moecher 《Journal of Earth System Science》2010,119(3):365-381
Field studies supplemented by petrographic analyses clearly reveal complete preservation of ophiolite suite from Port Blair
(11°39′N: 92°45′E) to Chiriyatapu (11°30′24″N: 92°42′30″E) stretch of South Andaman. The ophiolite suite reveals serpentinite
at the base which is overlain unconformably by cumulate ultramafic-mafic members with discernible cumulus texture and igneous
layering. Basaltic dykes are found to cut across the cumulate ultramafic-mafic members. The succession is capped by well exposed
pillow basalts interlayered with arkosic sediments. Olivine from the basal serpentinite unit are highly magnesian (Fo80.1–86.2). All clinopyroxene analyses from cumulate pyroxenite, cumulate gabbro and basaltic dyke are discriminated to be ‘Quad’ and
are uniformly restricted to the diopside field. Composition of plagioclase in different lithomembers is systematically varying
from calcic to sodic endmembers progressively from cumulate pyroxenite to pillow basalt through cumulate gabbro and basaltic
dyke. Plagioclase phenocrysts from basaltic dyke are found to be distinctly zoned (An60.7-An35.3) whereas groundmass plagioclase are relatively sodic (An33-An23.5). Deduced thermobarometric data from different lithomembers clearly correspond to the observed preservation of complete ophiolite
suite. 相似文献
20.
Soma Sen Roy Subhendu Brata Saha S. K. Roy Bhowmik P. K. Kundu 《Meteorology and Atmospheric Physics》2014,124(3-4):143-166
Nowcasting in the India Meteorological Department (IMD) is being provided for T + 0 to T + 2 h, using the Warning Decision Support System (WDSS-II) software. Prior to operational nowcasting over the Indian region, the parameters of the nowcast algorithm tool of the software were optimized, and accuracy was evaluated for various weather systems over Delhi. This optimization is demonstrated in this study with reference to three weather systems over Delhi, with each case representing one of three typical types of cloud systems over the region. These are—(a) convective lines associated with winter and early pre-monsoon weather systems, (b) deep convective cells that form in the pre-monsoon (April–June) and post-monsoon season (October–November) and (c) wide convective echoes that form during the monsoon season. The efficacy of the algorithm was assessed on a frame-by-frame basis as well as holistically for entire convective episodes. The important findings of the frame-by-frame study are (1) the inability of the inbuilt growth-decay algorithm to capture the evolution of storm cells, (2) setting of the threshold of detection of storms and tracking storms and (3) number of scales through which storms should be tracked. The holistic capabilities of the nowcast algorithm were tested for entire convective episodes using Model Evaluation Tools software. The results indicate that the advection algorithm tends to move the convective areas faster than observed at all time scales. Hence the multi-scale segmentation approach (over the two-scale approach) increases the smoothening of the output, at the cost of decreased nowcast skill. The inter-event comparison indicates that the low-intensity convective line zones, which are characteristic of winter and early pre-monsoon weather systems, have the most rapid temporal change in the overall area under convection. This leads to larger area errors during nowcasting of these systems. On the other hand, pre-monsoon systems comprised mostly isolated cells that reach great heights and move very fast, but do not have much horizontal area growth. The error in the nowcasting of these systems is mostly in respect of location error, as well as error in forecast of the intensity of the cells. The overall error in nowcasting is least for the monsoon systems over the Delhi region. 相似文献