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the mantle
The mantle upwelling originates from the core-mantle boundary and mostly occurs in the middle mantle and the lower part of the upper mantle.
      
The mantle flow has an effect on controlling the movement of plates and the distributions of ocean ridges, subduction zones and collision zones.
      
The mantle upwelling regions are clearly related with the locations of hotspots on the earth's surface.
      
As the volcanism prograded to the northwest, the depth of fault penetration into the mantle changed.
      
In Peter the Great Bay, Sea of Japan, this species repeatedly reproduces during the entire spring-autumn period; externae with developing embryos in the mantle cavity occur from May to September, and planktonic larvae occur from June to October.
      
grayanus: 8 from the muscles, 8 from the hepatopancreas, 6 from the female gonads, 4 from the mantle, 3 from the kidneys and male gonads, and 1 from the gills.
      
Twenty-one species of filamentous fungi were isolated from the internal organs of Modiolus modiolus: 10 from the muscles, 6 from the hepatopancreas, 5 from the female gonads, 3 from the kidneys, 3 from the mantle, and 1 from the gills.
      
This source is probably a diapir fold involving the upward movement of the mantle.
      
The latter can be a model for the relationship between the lithosphere thickness and the cross-sectional sizes of the mantle diapir that form a corona.
      
The densities of mineral assemblages in the mantle and the iron concentration in the core, calculated on the basis of the L- and LL-chondritic models, meet the geophysical constraints on the mass and the moment of inertia of Io.
      
The mean thickness of the mantle of dark material (~40 m) is estimated from the sizes of the craters ejecting the blocks of the basement ice material.
      
Large craters, knobs, and the mantle of dark material were formed mostly at the end of the period of heavy meteorite bombardment.
      
Here, effects of the inhomogeneity, compressibility, and viscosity of the liquid core are considered, along with those of electromagnetic coupling of the liquid core with the mantle and solid inner core.
      
This opens up new avenues for astrometric studies of the mechanical properties and electrical conductivity of the mantle and solid inner core at very low frequencies.
      
Here, effects of the inhomogeneity, compressibility, and viscosity of the liquid core are considered, along with those of electromagnetic coupling of the liquid core with the mantle and solid inner core.
      
This opens up new avenues for astrometric studies of the mechanical properties and electrical conductivity of the mantle and solid inner core at very low frequencies.
      
The constraints on the density distribution in the mantle and the size of the rock-iron core were derived.
      
The following parameters were varied while constructing the models: the ferric number of the mantle (Fe#) and the sulfur and hydrogen content in the core.
      
In this case, such an important parameter as the mantle silicate iron saturation is Fe# = 0.265.
      
On the possible enhancement of the magnetic field by neutrino reemission processes in the mantle of a supernova
      
 

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