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排序方式: 共有339条查询结果,搜索用时 15 毫秒
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Lucia Fanning Robin Mahon Patrick McConney Jorge Angulo Felicity Burrows Bisessar Chakalall Diego Gil Milton Haughton Sherry Heileman Sergio Martínez L’ouverture Ostine Adrian Oviedo Scott Parsons Terrence Phillips Claudia Santizo Arroya Bertha Simmons Cesar Toro 《Marine Policy》2007
A large marine ecosystem (LME) governance framework, developed from a need to effectively address the sustainable management of the shared living marine resources of the Caribbean, is proposed. The framework is based on four propositions and focuses on a linked examination of two well-known components of LME-level governance: the policy cycle process by which decisions are made and the multi-level nature of LMEs. It accommodates the diversity of policy cycles at multiple levels and the linkages among them required for effective governance of LMEs. The framework takes into account of factors such as context, purpose, jurisdictional scale, capacity and complexity and provides a means to identify critical areas for intervention. 相似文献
224.
Gustavo E. Romero † Diego F. Torres I. Andruchow Luis A. Anchordoqui Bennett Link † 《Monthly notices of the Royal Astronomical Society》1999,308(3):799-806
Based on Link & Epstein's study of temporal asymmetry of 631 gamma-ray bursts from the BATSE 3B catalogue, we identify the population of bursts with rising times that are longer than their decays, thus showing atypical profiles. We analyse their sky distribution, morphology, time–space clustering and other average properties and compare them with those associated with the bulk of the bursts. We show how most of the peculiar bursts analysed are consistent with recent fireball models, but a fraction of bursts (∼4 per cent of the total sample) appear to be inconsistent. 相似文献
225.
A certain vector-tensor theory is revisited. Our attention is focused on cosmology. Against previous suggestions based on
preliminary studies, it is shown that, if the energy density of the vector field is large enough to play the role of the dark
energy and its fluctuations are negligible, the theory is not simultaneously compatible with current observations on: supernovae,
the cosmic microwave background (CMB) anisotropy, and the power spectrum of the energy density fluctuations. However, for
small enough energy densities of the vector field and no scalar fluctuations, the theory becomes compatible with all the above
observations and, moreover, it leads to an interesting evolution of the so-called vector cosmological modes. This evolution
appears to be different from that of general relativity, and the difference might be useful to explain the anomalies in the
low order CMB multipoles. 相似文献
226.
A new crocodyliform specimen is presented here found in the Cerro Castaño Member of the Cerro Barcino Formation (Chubut Group). The material consists of cranial and postcranial remains that represent a new taxon that has strong affinities with Peirosauridae, but also shares derived features present in Araripesuchus. The phylogenetic relationships of this new taxon were tested through a cladistic analysis depicting it as a member of the Peirosauridae. The inclusion of Barcinosuchus within this clade of basal mesoeucrocodylians is supported by the presence of hypapophyses up to the third or fourth dorsal vertebrae, anterolateral facing edge on postorbital, quadrate dorsal surface divided in two planes by a ridge; mandibular symphysis tapering anterirorly in ventral view, lateral surface of dentary convex anterior to mandibular fenestra, distal body of quadrate well developed, anteroposteriorly thin and lateromedially broad. The new specimen broadens the temporal and geographical distribution of Peirosauridae during the Cretaceous of Gondwana, representing the southern-most and the most ancient record of the group in Patagonia. The new material also provides insights on the postcranial anatomy of peirosaurids, a group that has been so far studied almost exclusively from cranial material. 相似文献
227.
Global navigation satellite systems use appropriate satellite constellations to get the coordinates of an user—close to Earth—in an almost inertial reference system. We have simulated both GPS and GALILEO constellations. Uncertainties in the satellite world lines lead to dominant positioning errors. In this paper, a detailed analysis of these errors is developed inside a great region surrounding Earth. This analysis is performed in the framework of the so-called relativistic positioning systems. Our study is based on the Jacobian (J) of the transformation giving the emission coordinates in terms of the inertial ones. Around points of vanishing J, positioning errors are too large. We show that, for any 4-tuple of satellites, the points with J=0 are located at distances, D, from the Earth centre greater than about 2R/3, where R is the radius of the satellite orbits which are assumed to be circumferences. Our results strongly suggest that, for D-distances greater than 2R/3 and smaller than 105 km, a rather good positioning may be achieved by using appropriate satellite 4-tuples without J=0 points located in the user vicinity. The way to find these 4-tuples is discussed for arbitrary users with D<105 km and, then, preliminary considerations about satellite navigation at D<105 km are presented. Future work on the subject of space navigation—based on appropriate simulations—is in progress. 相似文献
228.
Diego F. Torres Thomas M. Dame Gustavo E. Romero 《Astrophysics and Space Science》2005,297(1-4):393-398
In this paper we briefly comment on the observational status of the possible physical association between unidentified EGRET
sources and supernova remnants (SNRs) in our Galaxy. We draw upon recent results presented in the review by Torres et al.
(2003), concerning molecular gas in the vicinity of all 19 SNRs found to be positionally coincident with EGRET sources at
low Galactic latitudes. In addition, we present new results regarding the supernova remnant CTA 1. Our findings disfavor the
possibility of a physical connection with the nearby (in projection) EGRET source. There remains possible, however, that the
compact object produced in the supernova explosion be related with the observed γ-ray flux. 相似文献
229.
We propose and test new statistical tools to study the distribution of cosmic rays based on the use of the minimal spanning tree. The method described is particularly sensitive to filamentary structures, as those expected to arise from strong sources of charged cosmic rays which get deflected by intervening magnetic fields. We also test the method with data available from the AGASA and SUGAR surface detector arrays. 相似文献
230.
Guido Garay Kate J. Brooks Diego Mardones Ray Norris 《Astrophysics and Space Science》2004,292(1-4):517-523
We report multi-wavelength observations towards IRAS 16547–4247, a luminous infrared source with a bolometric luminosity of 6.2 × 104 L ⊙. Dust continuum observations at 1.2-mm indicate that this object is associated with a dust cloud with a size of about 0.4 pc in diameter and a mass of about 1.3 × 103 M ⊙. Radio continuum observations show the presence of a triple radio source consisting of a compact central object and two outer lobes, separated by about 0.3 pc, symmetrically located from the central source. Molecular hydrogen line observations show a chain of knots that trace a collimated flow extending over 1.5 pc. We suggest that IRAS 16547–4247 corresponds to a dense massive core which hosts near its central region a high-mass star in an early stage of evolution. This massive YSO is undergoing the ejection of a collimated stellar wind which drives the H2 flow. The radio emission from the lobes arises in shocks resulting from the interaction of the collimated wind with the surrounding medium. We conclude that the thermal jets found in the formation of low-mass stars are also produced in high-mass stars. 相似文献