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331.
We report a new occurrence of sapphirine-spinel-corundum bearing granulites enclosed in granitic gneisses near Jagtiyal in the Eastern Dharwar Craton (EDC). These granulites are very important in deciphering the prehistory of the thermal peak of metamorphism due to the presence of refractory phases. The appearance of sapphirine is related to the following reactions: (a) Spl1 + Crd1 = Spr1 (2:2:1) (b) Phl (in Bt1) + Crn1 = East (in Bt2) + Spr2 (7:9:3) + Crd2 (c) Bt2 + Crd1 + Crn1 = Spr2 (7:9:3) + Kfs + H2O (d) Crd1 + Spl1 + Crn1 = Spr2 (7:9:3). The P-T evolution of these sapphirine granulites has been constrained through the use of THERMOCALC program. Temperature of formation of sapphirine-spinel assemblages is high, around 800 °C, and pressure ranges from 5–7 kbars, suggesting that sapphirine formation took place during decompression stage. 相似文献
332.
Dipankar Chakraborti Mohammad Mahmudur Rahman Bhaskar Das Bishwajit Nayak Arup Pal Mrinal Kumar Sengupta Md. Amir Hossain Sad Ahamed Manabendranath Sahu Kshitish Chandra Saha Subhash Chandra Mukherjee Shyamapada Pati Rathindra Nath Dutta Quazi Quamruzzaman 《Environmental Earth Sciences》2013,70(5):1993-2008
The authors’ survey of the Ganga–Meghna–Brahmaputra (GMB) plain (area 569,749 km2; population >500 million) over the past 20 years and analysis of more than 220,000 hand tube-well water samples revealed groundwater arsenic contamination in the floodplains of the Ganga–Brahmaputra river (Uttar Pradesh, Bihar, Jharkhand, West Bengal, and Assam) in India and the Padma–Meghna–Brahmaputra river in Bangladesh. On average, 50 % of the water samples contain arsenic above the World Health Organization guideline value of 10 μg/L in India and Bangladesh. More than 100 million people in the GMB plain are potentially at risk. The authors’ medical team screened around 155,000 people from the affected villages and registered 16,000 patients with different types of arsenical skin lesions. Arsenic neuropathy and adverse pregnancy outcomes have been recorded. Infants and children drinking arsenic-contaminated water are believed to be at high risk. About 45,000 biological samples analyzed from arsenic-affected villages of the GMB plain revealed an elevated level of arsenic present in patients as well as non-patients, indicating that many are sub-clinically affected. In West Bengal and Bangladesh, there are huge surface water in rivers, wetlands, and flooded river basins. In the arsenic-affected GMB plain, the crisis is not over water scarcity but about managing the available water resources. 相似文献
333.
Subash Chandra Surendra Atal Md. Ahmeduddin Shakeel Ahmed 《Journal of the Geological Society of India》2012,79(2):155-160
Geophysical techniques are normally employed to explore the subsurface and determine the anomalies but they are always much
larger in dimension. However, a very precise measurement was needed to pin point a misaligned horizontal tunnel made at 47
m depth to intercept an old bore well and rescue a four year child fallen accidently on 9th November at Jagatpura village in Jaipur, India. Due to the greater depth and presence of iron casing, electric power, etc.,
no equipment could work to determine the orientation of the tunnel that has lost its direction. The dimension of the site
and many other constrains didn’t allow conventional geophysical methods to be used. An innovative method was then designed
and successfully applied, which determined 1.92 m deviation of the tunnel end point to the east from the old bore well. The
digging was redirected accordingly and the bore well was intercepted. This paper describes the theoretical background, forward
simulations and the field experiment of the newly designed geophysical method. 相似文献
334.
335.
Establishing and successfully implementing new numerical computational technique(s) with simulation tool is one of the most
important difficult tasks in order to carry out real time scientific astronomical and other sophisticated problems. The main
focus and highlight of this paper is concerned with the introduction of a newly proposed simple embedded RKAHeM(4,4) technique
to determine the distribution of thermodynamic variables inside protoplanets during pre-collapse stage, formed by gravitational
instability, for protoplanetary masses between 0.3 to 10 Jupiter masses. The case of convection is a significant concern for
transference of heat inside the protoplanet and the graphical solution demonstrates positively better performance by inducting
the newly proposed effective RKAHeM(4,4) algorithm for any length of time in comparison with the results through Classical
Runge–Kutta method. Furthermore, the analytic expression for local truncation error, global truncation error and error estimates
are derived for better understanding. A viable quantitative analysis has been carried out to clearly visualize the goodness
and robustness of the proposed RKAHeM(4,4) algorithm. 相似文献
336.
Arvind Chandra Pandey Amit Kumar A. T. Jeyaseelan 《Journal of the Indian Society of Remote Sensing》2013,41(1):141-155
In the present study, the Cartosat-I digital elevation model (DEM) was utilized to deduce the vertical characteristics of Ranchi urban area and its relation to long term built-up expansion (1927–2010). The DEM represents moderate variation in terrain relief ranging from 595 m to 754 m with majority of area exhibiting upto 3° of slope and 3° to 6° indicating flat to undulating nature of terrain in Ranchi township. The DEM was used to generate location of sinks within urban area, which are generally delineated along the drainage channels, adjacent to high-rise built-up land and along the elevated road network. The pattern of urban sprawl over the eight decades (1927–2010) were examined with reference to terrain relief zones, which indicated that the built-up growth was mainly taken place over the elevation range of moderate (620–660 m) (67.0%) and high relief (660–680 m) (19.8%) zones. Although earlier preference for built-up development was more in high elevation zones (660–680 m), the low elevation zones (<600–620 m) are now preferred for multistoried built-up land development where better groundwater availability occur. The spatial pattern of vertical growth of built-up land was assessed using contour density obtained from Cartosat-I DEM. The results show that the high density contours predominately correspond to hilly area and high-rise buildings at majority of locations. The urban sprawl pattern and population trend exhibited rapid increase in vertical built-up growth after 1996 indicating beginning of urban densification in Ranchi township. 相似文献
337.
AbstractA laboratory model of thermal convection under a central force field has been constructed using a strong, alternating electric field gradient in a dielectric liquid. Both the electric field gradient and a temperature gradient are maintained between concentric vertical cylinders. The onset of thermal convection is detected by heat transfer and temperature measurements. It is governed by an electrical Rayleigh number, in which the electric force replaces gravity. Marginal stability analysis gives a critical electrical Rayleigh number in agreement with the experimentally determined value. 相似文献
338.
Ramesh Chandra Rajmal Jain Wahab Uddin Keiji Yoshimura Takeo Kosugi Taro Sakao Anita Joshi M. R. Deshpande 《Solar physics》2006,239(1-2):239-256
We present Hα observations from ARIES (Nainital) of a compact and impulsive solar flare that occurred on March 10, 2001 and
which was associated with a CME. We have also analyzed HXT, SXT/Yohkoh observations as well as radio observations from the Nobeyama Radio Observatory to derive the energetics and dynamics of this
impulsive flare. We coalign the Hα, SXR, HXR, MW, and magnetogram images within the instrumental spatial-resolution limit.
We detect a single HXR source in this flare, which is found spatially associated with one of the Hα bright kernels. The unusual
feature of HXR and Hα sources, observed for the first time, is the rotation during the impulsive phase in a clockwise direction.
We propose that the rotation may be due to asymmetric progress of the magnetic reconnection site or may be due to the change
of the peak point of the electric field. In MW emission we found two sources. The main source is at the main flare site and
another is in the southwest direction. It appears that the remote source is formed by the impact of accelerated energetic
electrons from the main flare site. From the spatial correlation of multiwavelength images of the different sources, we conclude
that this flare has a three-legged structure. 相似文献
339.
Kuntal Misra Dave Pooley † Poonam Chandra D. Bhattacharya Alak K. Ray Ram Sagar Walter H. G. Lewin 《Monthly notices of the Royal Astronomical Society》2007,381(1):280-292
We present X-ray, broad-band optical and low-frequency radio observations of the bright type IIP supernova SN 2004et. The Chandra X-ray Observatory observed the supernova at three epochs, and the optical coverage spans a period of ∼470 d since explosion. The X-ray emission softens with time, and we characterize the X-ray luminosity evolution as L X ∝ t −0.4 . We use the observed X-ray luminosity to estimate a mass-loss rate for the progenitor star of ∼2 × 10−6 M⊙ yr−1 . The optical light curve shows a pronounced plateau lasting for about 110 d. Temporal evolution of photospheric radius and colour temperature during the plateau phase is determined by making blackbody fits. We estimate the ejected mass of 56 Ni to be 0.06 ± 0.03 M⊙ . Using the expressions of Litvinova & Nadëzhin we estimate an explosion energy of (0.98 ± 0.25) × 1051 erg . We also present a single epoch radio observation of SN 2004et. We compare this with the predictions of the model proposed by Chevalier, Fransson & Nymark. These multiwavelength studies suggest a main-sequence progenitor mass of ∼20 M⊙ for SN 2004et. 相似文献
340.
Amar Agarwal K K Agarwal R Bali Chandra Prakash Gaurav Joshi 《Journal of Earth System Science》2016,125(4):873-884
The present study aims to understand evolution of the Lesser Himalaya, which consists of (meta) sedimentary and crystalline rocks. Field studies, microscopic and rock magnetic investigations have been carried out on the rocks near the South Almora Thrust (SAT) and the North Almora Thrust (NAT), which separates the Almora Crystalline Zone (ACZ) from the Lesser Himalayan sequences (LHS). The results show that along the South Almora Thrust, the deformation is persistent; however, near the NAT deformation pattern is complex and implies overprinting of original shear sense by a younger deformational event. We attribute this overprinting to late stage back-thrusting along NAT, active after the emplacement of ACZ. During this late stage back-thrusting, rocks of the ACZ and LHS were coupled. Back-thrusts originated below the Lesser Himalayan rocks, probably from the Main Boundary Thrust, and propagated across the sedimentary and crystalline rocks. This study provides new results from multiple investigations, and enhances our understanding of the evolution of the ACZ. 相似文献