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91.
Surface solar radiation over the Pacific Ocean off the Sanriku coast has been estimated using Visible and Infrared Spin Scan
Radiometer data supplied by the Geostationary Meteorological Satellite 5 for September, 1996 to June, 1997, when the Ocean
Color and Temperature Scanner was functioning. The hourly and daily insolation is estimated with a spatial resolution of 0.01-degree
grid. Thein situ surface short wave radiation obtained by the research vessel,Kofu-Maru belonging to the Japan Meteorological Agency is used for validation of the estimated insolation. It is shown that the estimated
hourly and daily insolation has an rms (root mean square) error of 17.05% and 8.13%, respectively, which are the ratios between
the rms error (W/m2) and the mean insolation (W/m2). 相似文献
92.
Qinghuan Luo Shinpei Shibata Donald B. Melrose 《Monthly notices of the Royal Astronomical Society》2000,318(3):943-951
The viability of polar cap models for high-energy emission from millisecond pulsars is discussed. It is shown that in millisecond pulsars, polar gap acceleration along the last open field lines is radiation-reaction limited, that is, the maximum energy to which particles can be accelerated is determined by balancing the energy-loss rate (due to curvature radiation) with the gap-acceleration rate. The maximum Lorentz factor is limited by curvature radiation and is not sensitive to the specific acceleration model. However, the distance (from the polar cap) at which the Lorentz factor achieves the limit is model dependent, and can be between one-hundredth (for the vacuum gap) and above one-tenth (for the space-charge limited gap) of a stellar radius distant from the polar cap for a pulsar period P =2 ms and a surface magnetic field B =7.5104 T. Because of the radiation reaction constraint and the relatively weak magnetic field, both the expected multiplicity (number of pairs per primary particle) and the Lorentz factor of the outflowing one-dimensional magnetospheric e± plasma from the polar gap are considerably lower than those for normal pulsars. Assuming space-charge limited flow, the location of the pair production front (PPF) is estimated to occur at about one stellar radius above the polar cap, which is significantly higher than that for normal pulsars. If the observed X-ray emission originates in the region near or above the PPF, the wide hollow-cone can reproduce the observed wide double-peaked feature of the light curves without using the aligned rotator assumption. 相似文献
93.
Geochronological and geochemical studies reveal the possible origin of the restricted body of mylonite rocks occurring at the eastern edge of Kyushu Island, Japan, just in contact with the Sashu Fault, a part of the Paleo‐Median Tectonic Line (Paleo‐MTL). The LA‐ICP‐MS zircon U–Pb dating of the quartz diorite mylonite in this mylonitic body indicates a crystallization age of 114.0 ±1.7 Ma. Moreover, the two tonalite samples appear as thin layers within the Permian fine‐grained mafic mylonite; a part of the same body yields the age of 113.7 ±2.3 Ma and 116.9 ±1.3 Ma, with extremely low Th/U ratio. These quartz diorite mylonite and tonalite are consistent with the late Early Cretaceous magmatism and coeval metamorphism similar to those in the Higo Plutono‐metamorphic Complex in western Kyushu, Japan. This newly characterized complex occurs just south of the Cretaceous Sambagawa metamorphic rocks. The newly characterized mylonitic rocks are lying structurally above the Sambagawa Metamorphic Complex and are distributed along the Paleo‐MTL. The extension of the Higo Plutonometamorphic Complex, as well as the structural relationship between this complex and the Sambagawa Metamorphic Complex, is still controversial but holds a key to reconstruct the tectonic evolution of Southwest Japan during the Late Mesozoic to Early Cenozoic period. Hence, this article provides new insight into the reconstruction of the evolution history of East Asia as an active convergent margin. 相似文献
94.
95.
L. Mestel P. Panagi S. Shibata 《Monthly notices of the Royal Astronomical Society》1999,309(2):388-394
The simplest model illustrating the effect of the magnetospheric charge-current field on the structure of a pulsar magnetic field has the region within the light-cylinder filled with the GoldreichJulian charge density which corotates with the neutron star, but has no electric currents along the magnetic field lines. This model has previously been studied for the axisymmetric case, with the rotation and magnetic dipolar axes aligned. The analogous problem is now solved with the two axes mutually perpendicular, so that not only the material current arising from the rotating charges but also the displacement current contributes. Again, the constructed magnetic field B 0 crosses the light-cylinder normally, and there is no energy flux to infinity. However, in a more realistic model there is a flow of current along B 0 , generating a field B 1 which has a non-vanishing toroidal component at the light-cylinder, so yielding a finite integrated Poynting flux. 相似文献
96.
Tetsuya Takahashi Hideaki Nakata Keiji Hirano Kazumi Matsuoka Mitsunori Iwataki Hitoshi Yamaguchi Tomoyuki Kasuya 《Journal of Oceanography》2009,65(1):113-120
Wind-induced circulation and the distribution of hypoxia corresponding to the upwelling of oxygen-depleted water (called “Aoshio”
in Japan and “Sumishio” locally in Omura Bay) in Omura Bay, Japan, was examined field observations and by three-dimensional
modeling. During the calm weather in summer, well-mixed strait water, in rich oxygen at the mouth of the bay intruded into
the middle layer of the bay, southward and northward along the west and east coast, respectively, forming basin-scale cyclonic
circulation. A stagnant water mass was formed below the center of this cyclonic circulation, and it became hypoxic water.
As a result of the prevailing strong southeast (northeast) wind, the bottom hypoxia moved in a southeasterly (northeasterly)
direction. This induces the upwelling of hypoxic water, accompanied by mass mortality of marine organisms. 相似文献
97.
Underwater light environment and photosynthetic accessory pigments were investigated in Ariake Bay in order to understand
how change of the pigments occurs in response to the tidal-induced changes in underwater light conditions. We hypothesize
that phytoplankton increases photo-protective pigments and decreases light-harvesting pigments under higher light condition
in the mixed layer caused by tidal cycle. Contribution rates of non-phytoplankton particles (a
nph
(400–700)) for light attenuation coefficient (K
d
) was highest (32–85%), and those of phytoplankton particles (a
ph
(400–700)), dissolved organic matter (a
g
(400–700)) and water were 6–32, 6–21 and 5–23%, respectively. Mean K
d
was higher during the spring tide (0.55 ± 0.23 m−1) than the neap tide (0.44 ± 0.16 m−1), and the K
d
difference was caused by the substances resuspension due to the tidal current. In contrast, ratios of photo-protective pigments
(diadinoxanthin and diatoxanthin) per chlorophyll a ((DD+DT)/Chl a) were higher during the neap tide (0.10 ± 0.03 mg mg-Chl a
−1) than the spring tide (0.08 ± 0.03 mg mg-Chl a
−1). And there was significant positive correlation between (DD+DT)/Chl a and mean relative PAR in the mixed layer ($
\overline {I_{mix} }
$
\overline {I_{mix} }
). Moreover, there was significant negative correlation between ratios of light-harvesting pigments (fucoxanthin) per Chl
a (Fuco/Chl a) and $
\overline {I_{mix} }
$
\overline {I_{mix} }
. These results suggested that phytoplankton in Ariake Bay increase photo-protective pigments and decrease light-harvesting
pigments in the higher light condition of less turbid, shallower mixed layer during neap tide than spring tide. 相似文献
98.
Tomoyuki Shikata Sou Nagasoe Tadashi Matsubara Yasuhiro Yamasaki Yohei Shimasaki Yuji Oshima Takuji Uchida Ian R. Jenkinson Tsuneo Honjo 《Journal of Oceanography》2008,64(3):355-365
In the present study, we have investigated the conditions influencing encystment and excystment in the dinoflagellate Gyrodinium instriatum under laboratory conditions. We incubated G. instriatum in modified whole SWM-3 culture medium and in versions of modified SWM-3 from which NO3
−, PO4
3−, NO3
− + PO4
3−, or Si had been omitted and observed encystment. Percentage encystment was high in the media without N and without P, while
the percentage encystment in the medium lacking both N and P was highest. Moreover, to investigate N or P concentration which
induced the encystment, Gyrodinium instriatum was also incubated in media with different concentrations of inorganic N and P; the concentrations of NO2
− + NO3
− and PO4
3− were measured over time. The precursors of cysts appeared within 2 or 3 days of a decrease in NO2
− + NO3
− or PO4
3− concentration to values lower than 1 μM or 0.2 μM, respectively. When cysts produced in the laboratory were incubated, we observed excystment after 8–37 days, without a mandatory
period of darkness or low temperature. We incubated cysts collected from nature at different temperatures or in the dark or
light and observed excystments. Natural cysts excysted at temperatures from 10 to 30°C, in both light and dark, but excystment
was delayed at low temperatures. These studies indicate that G. instriatum encysts in low N or P concentration and excysts over a wide temperature range, regardless of light conditions, after short
dormancy periods. 相似文献
99.
Yuichiro Kumamoto Takafumi Aramaki Shuichi Watanabe Minoru Yoneda Yasuyuki Shibata Orihiko Togawa Masatoshi Morita Kiminori Shitashima 《Journal of Oceanography》2008,64(3):429-441
In 1995 and 2000, the radiocarbon ratio (Δ14C) of total dissolved inorganic carbon was measured in the Japan Sea where deep and bottom waters are formed within the sea
itself. We found that (1) since 1979, the Δ14C in bottom water below about 2000-m depth in the western Japan Basin (WJB) had increased by about 30‰ by 1995, and (2) the
bottom Δ14C in the WJB did not change between 1995 and 2000. The former finding was due to penetration of surface bomb-produced radiocarbon
into the bottom water owing to bottom ventilation, whereas the latter was caused by stagnation of the bottom ventilation there.
In the eastern Japan Basin (EJB), the bottom Δ14C also increased by about 30‰ between 1979 and 2002. Recent stagnation of the bottom ventilation in the EJB is also suggested
from analyses of constant bomb-produced tritium between 1984 and 1999. The temporal variations of Δ14C, tritium, and dissolved oxygen in the bottom waters indicate that: (1) new bottom water is formed south of Vladivostok in
the WJB only in severe winters; and (2) the new bottom water then follows the path of a cyclonic abyssal circulation of the
Japan Sea, which results in the increases in dissolved oxygen and the transient tracers in the bottom waters in the EJB and
Yamato Basin with an approximate 3-to 6-year time lag. This process is consistent with the spatial variations of Δ14C, bomb-produced 137Cs, and chlorofluorocarbon-11 in the bottom waters of the Japan Sea. 相似文献
100.
Baator Has Tomoyuki Noro Kiyoteru Maruyama Akira Nakamura Kiichiro Ogawa Satoshi Onoda 《Landslides》2012,9(4):539-546
The northern Nagano Prefecture earthquake, MJMA?6.7 (Mw?6.2), which is inferred to have been triggered by the huge (Mw?9.0) March 11, 2011 Tohoku earthquake, occurred on March 12, 2011, in northern Nagano Prefecture, an area in Japan famous for heavy snowfall. A large number of landslides were triggered by the 12 March earthquake, and it caused building damage in the area of the epicenter. To clarify characteristics of the distribution and dynamic behavior of these landslides, we analyzed aerial photographs and conducted field surveys in and around the epicentral area. Large-scale landslides with long distance run-outs are a remarkable characteristic of the landslides induced by this earthquake. The long travel distance is considered to be related to the thick snowpack at the time the earthquake occurred. Moderate scale deep-seated landslides and shallow landslides were also observed in the study area. Based on an analysis of landslides with the active fault on which the earthquake is believed to have occurred, most of these landslides were distributed on the hanging wall of the active fault, within a distance of 12?km from the fault. 相似文献