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81.
Toshio Uchida 《Monthly notices of the Royal Astronomical Society》1998,297(1):315-322
The force-free magnetosphere around an obliquely rotating pulsar is studied. The basic equations reduce to two equations for two Euler potentials. One of the Euler potentials is regarded as a generalization of the stream function of the poloidal magnetic field lines in an axisymmetric rotator. Two divergence-free vectors become tangential to the surface on which this Euler potential is constant. 相似文献
82.
83.
Toshio Fukushima Masa-Katsu Fujimoto Hiroshi Kinoshita Shinko Aoki 《Celestial Mechanics and Dynamical Astronomy》1986,38(3):215-230
The relation between the units and readings of time and space coordinates of terrestrial and barycentric reference frames is discussed from the viewpoint of general relativity. Attention is paid to the unit of space coordinates since the International Astronomical Union (IAU) regulates only the unit of time in the above two frames. Two definitions of unit of length are examined and their effects on the numerical expression of coordinate transformation, equations of planetary motions, and those for light propagation time are discussed. A clear conflict is found between the IAU (1976) recommendation on the definition of the time-scales in different frames of reference and the statement that all constants in the IAU (1976) new system of astronomical constants are defined in terms of the Internationsl System of units (SI units). One of the above two definitions is proposed to resolve this conflict by the least alteration to current procedures for analysing the recent astrometric observations such as the radar/laser rangings, the range and range-rate, and the very long baseline interferometric observations. Also, an interpretation of numerical values in the IAU (1976) new system of astronomical constants is presented. It is stressed that the definition proposed in this paper requires that a formula slightly different from that in current use be employed in the numerical transformation of readings of coordinates between the terrestrial and barycentric reference frames. 相似文献
84.
A one-dimensional numerical model with a level-2.5 turbulent closure scheme to provide vertical mixing coefficients has been
used to investigate the process by which the dichothermal water is formed in the Bering Sea, the density of which is about
26.6 sigma-theta. The water column to be simulated is assumed to move along a predetermined path. That is, the present model
is of the Lagrangian-type. Surface boundary conditions are given using the climatologies of heat, freshwater and momentum
fluxes. In order to obtain a plausible moving speed of the water column along the path, pre-liminary experiments were done
using the surface fluxes in the central part of the Bering Sea for the initial temperature and salinity profiles at the entrance
of the Sea. As a result, it was found that the temperature minimum layer, i.e., the dichothermal water with temperature similar
to the climatology at the exit of the Bering Sea, was formed after about two years of integration. Based on the result, the
movement speed of the water column along the path was set as 4.5 cm/s in the standard run. It was found that this model could
plausibly reproduce the subsurface temperature minimum layer. That is, the dichothermal water was formed in the winter mixed
layer process in the Bering Sea. The existence of the subsurface halocline (pycnocline) prohibited the deeper penetration
of the winter mixed layer, and therefore water with a temperature colder than that under the mixed layer was formed in the
mixed layer due to wintertime surface cooling. In the warming season this water remains as the subsurface temperature minimum
layer between the upper seasonal thermocline and the lower halocline.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
85.
The clay minerals in the 18 core samples collected from the northern, equatorial and southeastern Indian Ocean are illite, chlorite, montmorillonite and kaolinite. In the fraction finer than 2 in the surface layer (top to 5 cm deep) of each core, the relative abundance of clay minerals varies widely from area to area. Kaolinite possesses the maximum proportion of the clay mineral composition and chlorite has the minimum proportion.Kaolinite is particularly dominant in sediments near off the northwestern coast of Australia. In the factions finer and coarser than 2 of the surface layer, montmorillonite and kaolinite tend to be abundant in the fraction finer than 2, and chlorite and illite tend to be abundant in the fraction coarser than 2. In some cores, kaolinite-rich layers in sediments which are considered to have been transported by turbidity currents from the Bay of Bengal are found. Turbidity currents appear partly a role in transport of sediments to the equatorial Indian Ocean.As to the relation between the vertical change of clay mineral composition and geochronological data, montmorillonite and kaolinite tend to be more abundant in interglacial ages than in glacial ages, while illite and chlorite tend to exhibit opposite trend.Muscovite and biotite highly concentrated in the cores Ka-9 and Ka-15 collected from the equatorial Indian Ocean seem to originate from granite or gneiss of Ceylon and/or India. 相似文献
86.
Toshio Yamagata 《Journal of Oceanography》1981,37(4):219-225
This article reviews the author's study on waves in planetary fluids for which the Okada Prize of the Oceanographical Society
of Japan was awarded in 1981. The contents of the review are i) some connections of planetary waves with the large-scale ocean
circulation, ii) stability of planetary waves, iii) the relationship between mean currents and planetary waves, iv) the influence
of topography on the mean current, v) a simple relationship between wave dissipation and viscous boundary layers and vi) some
ageostrophic effects on large-scale phenomena. Studies now in progress and related suggestions are also described and discussed
in the article 相似文献
87.
Clay minerals in the <2 fraction of the four deep-sea cores collected from the northeast and central North Pacific are studied. In the surface layers of the cores, illite is more dominant in the pelagic samples than in the near-shore ones, and montmorillonite is vice versa. Chlorite in the near-shore sample is relatively abundant in the areas of higher latitude than in those of lower latitude. Kaolinite content is less than 10 percent in all samples. The presence of particles of amphibole in the clay-size was confirmed by X-ray analysis in the whole of the core-st. 18 taken from the northeastern portion of the area. This fact suggests that, for a long time probably since the Tertiary age, particles of amphibole have been supplied from source areas. In the three cores except the core-st. 18 it is shown that montmorillonite clearly increases downward. It is suggested that montmorillonite has been derived from volcanic glassy material by a diagenetic change. Montmorillonite in the bottom layer (400–405 cm) of the core-st. 9 is particularly rich in iron. 相似文献
88.
Responding to the recommendation at the first Meeting of the International Coordination Group for the Cooperative Study of the Kuroshio and Adjacent Regions (CSK) 1965, a series of nitrate standard solutions consisting of eight different concentrations ranging from 0 to 50g-at NO3-N/l in 30.5 sodium chloride solution with the highest purity was prepared for nitrate-N determination in seawater. The solutions have been proved to be stable at least 520 days after preparation.The best way of handling and conditioning the copper-cadmium column was studied for securing the perfect and reproducible conversion of nitrate to nitrite for the procedure as proposed byWood
et al. (1967).It was also shown that the method can be applied to freshwater samples by the addition of sodium chloride and adjusting pH properly. 相似文献
89.
Toshio Yamagata 《Journal of Oceanography》1976,32(4):162-168
The problem of reflexion and critical level absorption of barotropic non-divergent Rossby waves in a lateral shear flow is considered with a ray tracing method. The results are compared with those of a normal mode approach. Some oceanographical applications are suggested. 相似文献
90.
Toshio Yamagata 《Journal of Oceanography》1976,32(4):155-161
The flow induced by the two-dimensional line vortex moving in a rotating fluid is discussed. The governing vorticity equation is linearized adopting the Oseen approximation.First, the problem is considered on a constantf-plane. The solution shows that the Stewartson E1/4 layer is transformed into the Oseen wake as the role of the advection becomes important.Second, the problem is considered on a-plane. When the line vortex moves westward, the solution shows a pattern of Rossby lee waves decaying downstream of the vortex and alternating flows far upstream. When the line vortex moves eastward, the inviscid solution shows definite alternating jets downstream. In a viscous case, however, the jets become less definite and identical with the above mentioned alternating flows in the far field. Far upstream, there are no disturbances because of the special propagation characteristics of Rossby waves. 相似文献