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排序方式: 共有147条查询结果,搜索用时 218 毫秒
91.
M. Hernandez W. P. S. Meikle A. Aparicio C. R. Benn M. R. Burleigh A. C. Chrysostomou A. J. L. Fernandes T. R. Geballe P. L. Hammersley J. Iglesias-Paramo D. J. James P. A. James S. N. Kemp T. A. Lister D. Martinez-Delgado A. Oscoz D. L. Pollacco M. Rozas S. J. Smartt P. Sorensen R. A. Swaters J. H. Telting W. D. Vacca N. A. Walton M. R. Zapatero-Osorio 《Monthly notices of the Royal Astronomical Society》2000,319(1):223-234
We present first-season infrared (IR) and optical photometry and spectroscopy of the Type Ia Supernova 1998bu in M96. We also report optical polarimetry of this event. SN 1998bu is one of the closest type Ia supernovae of modern times, and the distance of its host galaxy is well determined. We find that SN 1998bu is both photometrically and spectroscopically normal. However, the extinction to this event is unusually high, with We find that SN 1998bu peaked at an intrinsic Adopting a distance modulus of 30.25 (Tanvir et al.) and using Phillips et al.'s relations for the Hubble constant, we obtain Combination of our IR photometry with those of Jha et al. provides one of the most complete early-phase IR light curves for a SN Ia published so far. In particular, SN 1998bu is the first normal SN Ia for which good pre- t B max IR coverage has been obtained. It reveals that the J , H and K light curves peak about 5 days earlier than the flux in the B -band curve. 相似文献
92.
Larry L. Gordley Mark E. Hervig Chad Fish James M. Russell Scott Bailey James Cook Scott Hansen Andrew Shumway Greg Paxton Lance Deaver Tom Marshall John Burton Brian Magill Chris Brown Earl Thompson John Kemp 《Journal of Atmospheric and Solar》2009,71(3-4):300-315
The Solar Occultation For Ice Experiment (SOFIE) was launched onboard the Aeronomy of Ice in the Mesosphere (AIM) satellite on 25 April 2007, and began science observations on 14 May 2007. SOFIE conducts solar occultation measurements in 16 spectral bands that are used to retrieve vertical profiles of temperature, O3, H2O, CO2, CH4, NO, and polar mesospheric cloud (PMC) extinction at wavelengths from 0.330 to 5.006 μm. SOFIE performs 15 sunset measurements at latitudes from 65° to 85°S and 15 sunrise measurements from 65° to 85°N each day. This work describes the SOFIE instrument, measurement approach, and retrieval results for the northern summer of 2007. 相似文献
93.
Long-Term Trends in Chesapeake Bay Seasonal Hypoxia,Stratification, and Nutrient Loading 总被引:1,自引:0,他引:1
A previously observed shift in the relationship between Chesapeake Bay hypoxia and nitrogen loading has pressing implications
on the efficacy of nutrient management. Detailed temporal analyses of long-term hypoxia, nitrogen loads, and stratification
were conducted to reveal different within-summer trends and understand more clearly the relative role of physical conditions.
Evaluation of a 60-year record of hypoxic volumes demonstrated significant increases in early summer hypoxia, but a slight
decrease in late summer hypoxia. The early summer hypoxia trend is related to an increase in Bay stratification strength during
June from 1985 to 2009, while the late summer hypoxia trend matches the recently decreasing nitrogen loads. Additional results
show how the duration of summertime hypoxia is significantly related to nitrogen loading, and how large-scale climatic forces
may be responsible for the early summer increases. Thus, despite intra-summer differences in primary controls on hypoxia,
continuing nutrient reduction remains critically important for achieving improvements in Bay water quality. 相似文献
94.
95.
Robert Bolhar Uwe Ring Anthony I. S. Kemp Martin J. Whitehouse Steve D. Weaver Jon D. Woodhead I. Tonguc Uysal Rose Turnbull 《Contributions to Mineralogy and Petrology》2012,164(6):915-933
Zircons from 14 compositionally variable granitic rocks were examined in detail using CL image-guided micro-analysis to unravel the complex magmatic history above the southward retreating Hellenic subduction zone system in the Aegean Sea. Previously published U–Pb ages document an episodic crystallisation history from 17 to 11?Ma, with peraluminous (S-type) granitic rocks systematically older than closely associated metaluminous (I-type) granitic rocks. Zircon O- and Hf isotopic data, combined with trace element compositions, are highly variable within and between individual samples, indicative of open-system behaviour involving mantle-derived melts and evolved supracrustal sources. Pronounced compositional and thermal fluctuations highlight the role of magma mixing and mingling, in accord with field observations, and incremental emplacement of distinct melt batches coupled with variable degrees of crustal assimilation. In the course of partial fusion, more fertile supracrustal sources dominated in the earlier stages of Aegean Miocene magmatism, consistent with systematically older crystallisation ages of peraluminous granitic rocks. Differences between zircon saturation and crystallisation temperatures (deduced from zircon Ti concentrations), along with multimodal crystallisation age spectra for individual plutons, highlight the complex and highly variable physico-compositional and thermal evolution of silicic magma systems. The transfer of heat and juvenile melts from the mantle varied probably in response to episodic rollback of the subducting lithospheric slab, as suggested by punctuated crystallisation age spectra within and among individual granitic plutons. 相似文献
96.
97.
Justine Kemp Lynda C. Radke Jon Olley Steve Juggins Patrick De Deckker 《Quaternary Research》2012,77(1):65-76
Palaeosalinity records for groundwater-influenced lakes in the southwest Murray Basin were constructed from an ostracod-based, weighted-averaging transfer function, supplemented with evidence from Campylodiscus clypeus (diatom), charophyte oogonia, Coxiella striata (gastropod), Elphidium sp. (foraminifera), Daphniopsis sp. ephippia (Cladocera), and brine shrimp (Parartemia zietziana) faecal pellets, the δ18O of ostracods, and > 130 μm quartz sand counts. The chronology is based on optically stimulated luminescence and calibrated radiocarbon ages. Relatively wet conditions are marked by lower salinities between 9600 yr and 5700 yr ago, but mutually exclusive high- and low-salinity ostracod communities suggest substantial variability in effective precipitation in the early Holocene. A drier climate was firmly in place by 4500 yr and is marked at the groundwater-dominated NW Jacka Lake by an increase in aeolian quartz and, at Jacka Lake, by a switch from surface-water to groundwater dominance. Short-lived, low-salinity events at 8800, 7200, 5900, 4800, 2400, 1300 and 400 yr are similar in timing and number to those recorded on Australia's southern continental shelf, and globally, and provide evidence for the existence of the ~ 1500-yr cycle in mainland southern Australia. We surmise that these are cool events associated with periodic equatorward shifts in the westerly wind circulation. 相似文献
98.
Andrew C. Kemp Benjamin P. Horton Daria Nikitina Christopher H. Vane Marina Potapova Elizabeth Weber‐Bruya Stephen J. Culver Tatyana Repkina David F. Hill 《Boreas: An International Journal of Quaternary Research》2017,46(3):562-584
In support of efforts to reconstruct relative sea level (RSL), we investigated the utility of foraminifera, diatoms and bulk‐sediment geochemistry (δ13C, C:N and parameters measured by Rock‐Eval pyrolysis) as sea‐level indicators in Eurasian sub‐Arctic salt marshes. At three salt marshes (<15 km apart) in Dvina Bay (White Sea, Russia), we collected surface sediment samples along transects from subtidal to Taiga forest environments. Foraminifera at all sites formed bipartite assemblages, where elevations below mean high higher water (MHHW) were dominated by Miliammina spp. and elevations between MHHW and the highest occurrence of foraminifera were dominated by Jadammina macrescens and Balticammina pseudomacrescens. Five high‐diversity groups of diatoms were identified and they displayed pronounced variability amongst the study sites. Bulk‐sediment geochemistry recognized two groups (clastic‐dominated environments below MHHW and organic‐rich environments above MHHW). As one group included subtidal elevations and the other included supratidal elevations, we conclude that the measured geochemical parameters are not stand‐alone sea‐level indicators. Core JT2012 captured a regressive sediment succession of clastic, tidal‐flat sediment overlain by salt‐marsh organic silt and freshwater peat. The salt‐marsh sediment accumulated at 2804±52 years before present and preserved foraminifera (Jadammina macrescens and Balticammina pseudomacrescens) with good analogy to modern assemblages indicating that RSL was +2.60±0.47 m at this time. Diatoms confirm that marine influence decreased through time, but the lack of analogy between modern and core assemblages limited their utility as sea‐level indicators. Geochemical parameters also indicate a reduction in marine influence through time. We conclude that RSL reconstructions derived from salt‐marsh sediment preserved beneath Eurasian sub‐Arctic peatlands can provide valuable insight into the spatio‐temporal evolution of the Fennoscandian and Eurasian ice sheets. 相似文献
99.
R. Presura V. V. Ivanov Y. Sentoku V. I. Sotnikov P. J. Laca N. Le Galloudec A. Kemp R. Mancini H. Ruhl A. L. Astanovitskiy T. E. Cowan T. Ditmire C. Chiu W. Horton P. Valanju S. Keely 《Astrophysics and Space Science》2005,298(1-2):299-303
An experimental simulation of planetary magnetospheres is being developed to investigate the formation of collisionless shocks
and their effects. Two experimental situations are considered. In both, the solar wind is simulated by laser ablation plasmas.
In one case, the “solar wind” flows across the magnetic field of a high-current discharge. In the other, a transverse magnetic
field is embedded in the plasma flow, which interacts with a conductive obstacle. The ablation plasma is created using the
“Tomcat” laser, currently emitting 5 J in a 6 ns pulse at 1 μm wavelength and irradiance above 1013 W/cm2. The “Zebra” z-pinch generator, with load current up to 1 MA and voltage up to 3.5 MV produces the magnetic fields. Hydrodynamic modeling
is used to estimate the plasma parameters achievable at the front of the plasma flow and to optimize the experiment design.
Particle-in-cell simulations reveal details of the interaction of the “solar wind” with an external magnetic field, including
flow collimation and heating effects at the stopping point. Hybrid simulations show the formation of a bow shock at the interaction
of a magnetized plasma flow with a conductor. The plasma density and the embedded field have characteristic spatial modulations
in the shock region, with abrupt jumps and fine structure on the skin depth scale. 相似文献
100.
A. De Kemp 《Astrophysics and Space Science》1997,247(1-2):11-16
This contribution can only be a small collection of ideas and experiences from my (personal) publishing point of view. The
subject area assigned is very generic and there are indeed many developments going on, so I had to be very selective and restrictive,
while avoiding redundancies as much as I could. I have included some metaphors and paradigms, such as the shift from print
publications to electronic information. The traditional role of publishers in the information chain is compared with the new
opportunities that electronic publishing is offering now and may offer in the foreseeable future. From DTP to DTD, unplugged
and unbundled information, linearity, appropriateness, packaging and customizing, filters, intelligent agents, quality, integrity
and authenticity are some of the items hidden in the text. The overall conclusion is: the Internet still can learn a lot from
print...!
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献