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81.
Long-slit spectra of intermediate spectral and high spatial resolution of new Herbig-Haro objects in AFGL 5142, AFGL 5157 and IRAS 2237+7455 and of the already known GGD17/HH1 were obtained. The results are shown in the form of position-velocity diagrams. Radial velocities and electron densities were measured. 相似文献
82.
自转本身是恒星的基本物理量之一,同时影响恒星的其它许多物物量,包括对恒星半径、形状和体积的影响;对光度、包指数、谱线轮廓、等值宽度、偏振度等观测量的影响;对引力加速度、元素丰度的影响;对恒星内部结构,如中心压力、温度、密度的影响。这些将会影响到恒星在H—R图上的位置,演化路径以及年龄和寿命等。因此,无论是理论模型还是实测研究,对自转快的恒星应该进行自转影响的修正。 相似文献
83.
本文利用红外天文卫星点源表及哈勃望远镜导星星表对1990年新发表的75个S星进行了IRAS红外源及GSC光学对应体的证认,给出41个S星有IRAS对应体,12个S星有GSC光学对应体。 相似文献
84.
Dolomite in caves: Recent dolomite formation in oxic, non-sulfate environments. Castañar Cave, Spain
Dolomite is a common mineral in the rock record but rare in recent superficial environments. Where it does occur, it is related to anoxic, sulfate-rich environments and microbial activity. The occurrence of some dolomite deposits in caves, however, indicates that dolomite formation is also possible in oxic, non-sulfate settings. Dolomite is forming at 17 °C and in oxic-vadose conditions on the host rocks and aragonite speleothems of the Castañar Cave, Cáceres, Spain. It appears as spheroids and dumbbells 50–300 μm in diameter that internally consist of micron-sized rhombic to rounded crystals. Initially this dolomite is Ca-rich, non-stoichiometric and poorly ordered. Mg-rich solutions allow the precipitation of metastable Mg-rich carbonates, such as huntite. This soon transforms into this Ca-rich dolomite, which later “ages” to form a more stoichiometric dolomite. These dolomites show similarities to those grown under anoxic, sulfate-rich conditions and their presence in caves provides a different setting that may contribute to the understanding of the “dolomite problem”, including their initial formation and later recrystallization processes. 相似文献
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87.
The investigation of a limestone cave on the Ryonggok-ri of Sangwon County, North Hwanghae Province, DPRK, has yielded many faunal remains including Late Pleistocene deer, brown bears and horses. Uranium series dating of fossil teeth yielded dates of ~72ka at the base of Layer 2 – the bone-bearing unit – and ~44ka at the top. The rich and diverse mammal remains of Ryonggok Cave No. 1 are indicative of warm and humid temperate conditions during the Late Pleistocene, and reflect the presence of both dense forests and open grassland. In addition, pollen and spores from the site include two families and 24 genera of trees, six families and a genus of grasses and herbs, and two families and six genera of ferns, corroborating the environments inferred from the faunal remains. 相似文献
89.
Thomas Boyle 《The Australian geographer》2012,43(4):393-410
As the social, ecological and economic benefits of green buildings become more established, firms, especially professional service firms, are responding by adopting sustainable office space (SOS). Accelerating this uptake demands a nuanced appreciation of firms’ understandings of and motivations for adopting SOS. Through a qualitative study of professional service firms in Sydney, this paper brings together a decentred understanding of the contemporary firm drawn from the ‘new economic geographies’ approach and theories of corporate social responsibility to trace and interpret the diverse and overlapping motivations shaping the uptake of SOS amongst these firms. The firm is shown to be a site of plurality and agency, governed by multiple logics. Whilst motivations informed by economic logic remain persuasive and pervasive, the adoption of SOS is simultaneously informed by a wider palette of logics, including environmental and social logics. The paper argues that a decentred conceptualisation of the firm brings the multiplicity of firms’ orientations towards SOS into view and, in so doing, has the potential to inform a politics of intervention for steering firms towards more socially and environmentally sustainable behaviours. 相似文献
90.
《Experimental Astronomy》2009,23(1):277-302
The Molecular Hydrogen Explorer, H2EX, was proposed in response to the ESA 2015 - 2025 Cosmic Vision Call as a medium class space mission with NASA and CSA participations.
The mission, conceived to understand the formation of galaxies, stars and planets from molecular hydrogen, is designed to
observe the first rotational lines of the H2 molecule (28.2, 17.0, 12.3 and 9.7 μm) over a wide field, and at high spectral resolution. H2EX can provide an inventory of warm (≥ 100 K) molecular gas in a broad variety of objects, including nearby young star clusters,
galactic molecular clouds, active galactic nuclei, local and distant galaxies. The rich array of molecular, atomic and ionic
lines, as well as solid state features available in the 8 to 29 μm spectral range brings additional science dimensions to
H2EX. We present the optical and mechanical design of the H2EX payload based on an innovative Imaging Fourier Transform Spectrometer fed by a 1.2 m telescope. The 20’×20’ field of view
is imaged on two 1024×1024 Si:As detectors. The maximum resolution of 0.032 cm − 1 (full width at half maximum) means a velocity resolution of 10 km s − 1 for the 0 – 0 S(3) line at 9.7 μm. This instrument offers the large field of view necessary to survey extended emission in
the Galaxy and local Universe galaxies as well as to perform unbiased extragalactic and circumstellar disks surveys. The high
spectral resolution makes H2EX uniquely suited to study the dynamics of H2 in all these environments. The mission plan is made of seven wide-field spectro-imaging legacy programs, from the cosmic
web to galactic young star clusters, within a nominal two years mission. The payload has been designed to re-use the Planck platform and passive cooling design.
相似文献
J. P. Maillard (Corresponding author)Email: |