A possible current system associated with the S_q^p variation     

K. Kawasaki  S.-I. Akasofu 《Planetary and Space Science》1973,21(3):329-337

It is suggested that the quiet day daily magnetic variation in the polar cap region, S_q^p, results partly from the short-circuit effect of the magnetotail current by the polar ionosphere. This implies that there is an inward field-aligned current from the dawnside magnetopause to the forenoon sector of the auroral oval (positively charged) and an outward field-aligned current to the duskside magnetopause from the afternoon sector of the oval (negatively charged), together with the ionospheric (Pedersen and Hall) currents. The distribution of the magnetic field vectors of both combined current systems agrees with the observed S_q^pvector distribution. The space charges provide an electric field distribution which is similar to that which has been observed by polar orbiting satellites.  相似文献   

Influence of bedrock groundwater on streamflow characteristics in a volcanic catchment          下载免费PDF全文

Masamitsu Fujimoto  Nobuhito Ohte  Masatoshi Kawasaki  Ken'ichi Osaka  Masayuki Itoh  Izumi Ohtsuka  Masami Itoh 《水文研究》2016,30(4):558-572

Groundwater movements in volcanic mountains and their effects on streamflow discharge and representative elementary area (REA) have remained largely unclear. We surveyed the discharge and chemical composition of spring and stream water in two catchments: the Hontani river (NR) catchment (6.6 km²) and the Hosotani river (SR) catchment (4.0 km²) at the southern part of Daisen volcano, Japan. Daisen volcano is a young volcano (17 × 10³ years) at an early stage of erosion. Our study indicated that deep groundwater that moved through thick lava and pyroclastic flows and that could not be explained by shallow movements controlled by surface topography contributed dominantly to streamflow at larger catchment areas. At the NR catchment, the deep groundwater contribution clearly increased at a catchment boundary defined by an area of 3.0 km² and an elevation of 800 m. At the SR catchment, the contribution deep groundwater to the stream also increased suddenly at a boundary threshold of 2.0 and 700 m. Beyond these thresholds, the contributions of deep bedrock groundwater remained constant, indicating that the REA is between 2 and 3 km² at the observed area. These results indicate that the hydrological conditions of base flow were controlled mainly by the deep bedrock groundwater that moved through thick lava and pyroclastic flows in the undissected volcanic body of the upper part of the catchment. Our study demonstrates that deep and long groundwater movements via a deep bedrock layer including thick deposits of volcanic materials at the two catchments on Daisen volcano strongly determined streamflow discharge instead of the mixing of small‐scale hydrological conditions. Copyright © 2015 John Wiley & Sons, Ltd.  相似文献   

Experimental evaluation and parameterization of evaporation from soil surface     

Jidong Teng  Noriyuki Yasufuku  Qiang Liu  Shiyu Liu 《Natural Hazards》2014,73(3):1405-1418

Surface evaporation is one of the main processes in the soil–atmosphere interaction. Since it is highly related to meteorological factors and soil properties, determination of evaporation rate from soil surface remains a challenge. To investigate the evaporation from unsaturated soil, a climate control apparatus has been newly developed, which has a feature of completely controlling air temperature, relative humidity and wind speed. Twelve climatic conditions are applied to three kinds of soil specimens to carry out the evaporation tests. The results show that only water content cannot allow an accurate estimation, additional variables accounting for soil texture and wind speed must be included as well. Moreover, a simple approach to parameterize evaporation is presented by the soil moisture θ of top 1-cm layer with considering the effect of soil texture and wind speed. It is found that the new approach is able to accurately estimate the evaporation from unsaturated soil.  相似文献   

Characteristics of Beachrocks: A Review   总被引：1，自引：0，他引：1  

Takashi Danjo  Satoru Kawasaki 《Geotechnical and Geological Engineering》2014,32(2):215-246

Beachrocks are calcareous rocks that have been quite recently formed and are found in the intertidal zone on sandy beaches. The authors are developing an artificial rock with self-healing capabilities that can be used in coastal areas to repair the infrastructure of coastal walls. Because beachrocks are formed naturally on beaches, they merit study as a model for artificial rocks. We conducted a bibliographical study in order to gather information about the characteristics of beachrocks, which may aid in the manufacturing of artificial rocks. This study investigated their geographic distribution, formative periods, physical properties, and origins. The study found that over 90 % of beachrocks are found between the latitudes 40°N and the Tropic of Capricorn, and that their formative periods range from 26,000 years to just a few decades ago. We also learned that the cement component of beachrocks mainly consists of either calcium carbonate or silica. The dynamic characteristics of these components have been studied in only three papers, which note that their uniaxial compression strength ranges from as low as 6.0 to 42.0 MPa. Since very limited data are available on beachrocks in Japan where the artificial rock technology will first be deployed, there is a need for collecting additional data on their mechanical properties, elemental composition ratios, and mineral content.  相似文献   

Cross-sectional profiles of Baltis Vallis channel on Venus: Reconstructions from Magellan SAR brightness data     

Shoko Oshigami  Noriyuki Namiki 《Icarus》2007,190(1):1-14

Baltis Vallis is a 6800-km long canali-type channel on Venus. Canali have a unique combination of morphological characteristics: extraordinary length, a single main conduit, and a degree of similarity to terrestrial rivers. These characteristics have given rise to intensive discussions on whether the origin of canali is erosional or constructional. Cross-sectional profiles of such channels reveal the detailed morphology of the structure and enable us to distinguish between these two possible origins; however, canali are just several kilometers wide and are therefore too small for the construction of cross-sectional profiles from Magellan altimetry data. Instead, we propose a new method for reconstructing short-wavelength topography using brightness data from Synthetic Aperture Radar images. We apply Muhleman's backscattering function to the backscatter intensity calculated from the brightness of Magellan Full-Resolution SAR Map images. The estimated vertical error of this new method is less than 5 m for a distance of 1 km across the channel. We studied 120 sites along an approximately 6000 km extent of Baltis Vallis. The channel profiles reveal that in nearly 90% of these sites, the bottom surface of the channel is lower than the surrounding plains by 20-100 m. Clear levee structures and intra-channel ridges are recognized in about 30 and 25%, respectively, of the sites analyzed within Baltis Vallis. Most of the levees occur in the upper segment of Baltis Vallis, while intra-channel ridges are mostly confined to the region between 1500 and 3000 km downstream from the probable source. The average depth and width of the channel are 46 m (standard deviation: 16 m) and 2.2 km (standard deviation: 0.4 km), respectively, and the depth profile along the channel is highly undulatory. The groove-like morphology and paucity of levee structures indicates an erosional origin. Furthermore, the observed undulations in depth along the channel indicate that Baltis Vallis most likely formed by mechanical erosion. The observed morphological transition from levees to intra-channel ridges suggests that the channel-forming processes changed across an area located approximately 1500 km from the source. Carbonatite is the most likely candidate material for the low-viscosity fluid that formed Baltis Vallis.  相似文献   

Mira variables in the Galactic bulge with OGLE-II data     

Noriyuki Matsunaga  Hinako Fukushi  Yoshikazu Nakada 《Monthly notices of the Royal Astronomical Society》2005,364(1):117-125

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Paleomagnetism of the Cu�CZn�CPb-bearing Kupferschiefer black shale (Upper Permian) at Sangerhausen, Germany     

David T. A. Symons  Kazuo Kawasaki  Sabine Walther  Gregor Borg 《Mineralium Deposita》2011,46(2):137-152

Syngenetic, diagenetic and epigenetic models have been proposed for the Cu?CZn?CPb Kupferschiefer mineralization at Sangerhausen, Germany. Paleomagnetic and rock magnetic measurements have been made on 205 specimens from mine workings on the margin of the Sangerhausen Syncline. The mineralization is richest in the ??0.5-m-thick Upper Permian (258?±?2?Ma) Kupferschiefer black marly shale (nine sites) and dies out over ??0.2?m in the underlying Weisliegend sandstones (three sites) and overlying Zechstein carbonates (two sites). Except for one site of fault zone gypsum, characteristic remanent magnetization directions were isolated for all 14 sites using alternating field and thermal step demagnetization. These directions provide a negative fold test, indicating that the remanence postdates Jurassic fault block tilting. Rock magnetic measurements show that the Kupferschiefer shale marks a redox front between the oxidized Weissliegend sandstones and non-oxidized Zechstein carbonates. The 14 site directions give a Late Jurassic paleopole at 149?±?3?Ma. It is significantly different from the paleopole reported by E.C. Jowett and others for primary or early diagenetic Rote F?ule alteration that gives an age of 254?±?6?Ma on the current apparent polar wander path and is associated with Kupferschiefer mineralization. We suggest that the Late Jurassic extensional tectonic event that formed the nearby North German Basin also reactivated Variscan basement faults and extended them up through the overlying strata, thereby allowing hydrothermal basement fluids to ascend and epigenetically mineralize the Kupferschiefer shale. The possibility of a 53?±?3?Ma mineralization age is also considered.  相似文献   

Period–luminosity relations for type II Cepheids and their application     

Noriyuki Matsunaga †‡  Michael W. Feast  John W. Menzies 《Monthly notices of the Royal Astronomical Society》2009,397(2):933-942

JHK _s magnitudes corrected to mean intensity are estimated for Large Magellanic Cloud (LMC) type II Cepheids in the OGLE-III survey the third phase of the Optical Gravitational Lensing Experiment (OGLE). Period–luminosity (PL) relations are derived in JHK _s as well as in a reddening-free VI parameter. Within the uncertainties, the BL Her stars  ( P < 4 d)  and the W Vir stars (   P = 4  to 20 d) are colinear in these PL relations. The slopes of the infrared relations agree with those found previously for type II Cepheids in globular clusters within the uncertainties. Using the pulsation parallaxes of V553 Cen and SW Tau, the data lead to an LMC modulus uncorrected for any metallicity effects of  18.46 ± 0.10  mag. The type II Cepheids in the second-parameter globular cluster, NGC 6441, show a PL( VI ) relation of the same slope as that in the LMC, and this leads to a cluster distance modulus of  15.46 ± 0.11  mag, confirming the hypothesis that the RR Lyrae variables in this cluster are overluminous for their metallicity. It is suggested that the Galactic variable κ Pavonis is a member of the peculiar W Vir class found by the OGLE-III group in the LMC. Low-resolution spectra of OGLE-III type II Cepheids with   P > 20  d (RV Tau stars) show that a high proportion have TiO bands; only one has been found showing C₂. The LMC RV Tau stars, as a group, are not colinear with the shorter period type II Cepheids in the infrared PL relations in marked contrast to such stars in globular clusters. Other differences between LMC, globular cluster and Galactic field type II Cepheids are noted in period distribution and infrared colours.  相似文献   

Monthly variations of hydrographic structures and water mass distribution off the Doto area, Japan   总被引：2，自引：2，他引：0  

Akira Kusaka  Tomonori Azumaya  Yasuhiro Kawasaki 《Journal of Oceanography》2013,69(3):295-312

Monthly variations of hydrographic structures and water mass distributions were investigated over a nearly 30-year period (January 1982–March 2011) off the Doto area, Japan, to examine temporal evolutions and devolutions of representative water masses in this area. In the continental shelf area, the Coastal Oyashio Water (COW) was distributed along the coast during January–May, when COW has been modified by relatively higher salinity water, which may have originated from the Oyashio Water (OW) off the Kuril Islands. On the other hand, the Surface COW (S-COW) may have formed with COW heated by solar radiation, simultaneously mixing with the Tokachi River freshwater and OW in the continental shelf area, and the area of this S-COW spread offshoreward during June and July, and stayed in the offshore area during June and October. Although coastal density current structures, probably due to the Modified Soya Warm Current Water (M-SWCW) inflows, were conspicuous in the continental shelf area during August–October, those structures were weak after November. These weakening structures may be due to developed surface mixed layer caused by surface cooling, and decay of volume transport of the Soya Warm Current in the Okhotsk Sea, and such weakening accordingly may lead to weakening of higher salinity water inflows from the upstream regions. M-SWCW was radically replaced by COW during December and January with rapid salinity decreases, which suggest extremely lower salinity water inflows, probably due to influences of the East Sakhalin Current Water.  相似文献   

The Reocín zinc–lead deposit,Spain: paleomagnetic dating of a late Tertiary ore body     

David T. A. Symons  Michael T. Lewchuk  Kazuo Kawasaki  Francisco Velasco  David L. Leach 《Mineralium Deposita》2009,44(8):867-880

The Reocín mine in northern Spain’s Basque–Cantabrian basin exploited a world-class Mississippi Valley-type Zn–Pb deposit. Its epigenetic mineralization is in Urgonian 116 ± 1 Ma dolomitized limestones of the Santillana syncline, which was formed by Oligocene and mid Miocene pulses of the Pyrenean orogeny. Paleomagnetic results (22 sites, 274 specimens) in mineralization isolated a stable remanence (ChRM) in pyrrhotite and minor magnetite inclusions in ore specimens, Zn concentrate, and tailings. A fold test shows that the ChRM is substantially post-folding. The mineralization’s paleopole lies on the European apparent polar wander path and indicates that the mineralization was formed at 15 ± 10 Ma. We postulate that brines originated in underlying Triassic and Lower Cretaceous sedimentary rocks and were driven upward into the host rocks by the hydraulic gradient created by the nearby Asturian massif.  相似文献