Runoff generation processes estimated from hydrological observations on a steep forested hillslope with a thin soil layer   总被引：4，自引：0，他引：4  

Makoto Tani 《Journal of Hydrology》1997,200(1-4):84-109

In order to understand runoff generation processes on a forested hillslope involving large heterogeneities, this study monitored runoff from a steep hillslope with a thin soil layer as well as matric potential within it and analyzed their responses to storm rainfall. A comparison of storm runoff responses from the study slope with those from two adjacent catchments, one of which includes it, showed that physical properties of the slope reflected the runoff characteristics: although no responses occurred in very dry conditions because of the absence of wet zones near the stream, the area contributing to storm runoff more rapidly extended to the whole slope due to its topographic properties. They also caused its steep hydrographs produced in the wettest condition where almost all the rainfall contributed to storm runoff. In this wettest condition, tensiometric responses near bedrock showed the vertical quick propagation of the rainfall pulse, and a good agreement of storm hydrograph simulated through a kinematic wave runoff model suggested that runoff from the slope was produced by a lateral flow on the bedrock receiving the quick propagation. In a transition process from dry to the wettest conditions, the development of the lateral flow producing smaller responses at the downslope end was estimated from decreasing of matric potential near bedrock from high negative to low values with increasing cumulative rainfall.  相似文献   

Dynamics of Lithosphere Convergence     

Makoto Yamano  Manik Tulwuni  Kensaku Turnuki 《Island Arc》1997,6(3):233-233

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Long-term temperature monitoring in a borehole drilled into the Nojima Fault, southwest Japan   总被引：2，自引：0，他引：2  

Makoto Yamano  Shusaku Goto 《Island Arc》2001,10(3-4):326-335

Abstract Long-term monitoring of temperature distribution in an active fault zone was carried out using the optical fiber temperature-sensing technique. An optical fiber cable was installed in a borehole drilled into the Nojima Fault in Awaji Island, south-west Japan, and the temperature profile to a depth of 1460 m had been measured for 2.5 years (July 1997–January 2000). Although the obtained temperature records showed small temporal variations due to drifts of the measurement system all along the cable, local temperature anomalies were detected at two depths. One at around 80 m seems to correspond to a fracture zone and may be attributed to groundwater flow in the fracture zone. This anomaly had been stable throughout the monitoring period, whereas the other anomaly at around 500 m was a transient one. The water level in the borehole could be estimated from the diurnal temperature variations in the uppermost part of the borehole and may provide information on the hydrological characteristics of the fault zone, which is connected to the borehole through perforations on the casing pipe. Except for these minor variations, the temperature profile had been very stable for 2.5 years. The conductive heat flow calculated from this profile and the thermal conductivity measured on core samples increases with depth, probably resulting from errors in thermal conductivity due to sampling problems and/or from advective heat transfer by regional groundwater flow. Assuming that the middle part of the borehole (less fractured granite layer) is least affected by these factors, heat flow at this site is estimated to be approximately 70 mW/m².  相似文献   

The Fourier transform of controlled-source time-domain electromagnetic data by smooth spectrum inversion   总被引：1，自引：0，他引：1  

Yuji Mitsuhata  Toshihiro Uchida  Yutaka Murakami  Hiroshi Amano 《Geophysical Journal International》2001,144(1):123-135

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Rotating eruption of an untwisting filament triggered by the 3B flare of 25 April, 1984     

Hiroki Kurokawa  Yoichiro Hanaoka  Kazunari Shibata  Yutaka Uchida 《Solar physics》1987,108(2):251-264

A great 3B flare, whose X-ray class was X13, occurred over a delta-sunspot at 00: 01 UT on April 25, 1984. Before the flare, a strong magnetic shear was found to be formed along the neutral line in the delta-sunspot with shear motions of umbrae. The shear motions of the umbrae were caused by the successive emergence of a magnetic flux rope.Before the flare, several groups of sheared H threads and filaments were found to merge into an elongated filament along the neutral line through the delta-sunspot. In the merging process the helical twists were formed in the filament by the reconnection as in the Pneuman's (1983) model.At the post-maximum phase of the flare, the helically twisted filament spouted out with an untwisting rotation. Examining the morphological and dynamical features of the filament eruption, we concluded that it has some typical features of the flare spray and that it seems to be accelerated by the sweeping-magnetictwist mechanism proposed by Shibata and Uchida (1986).Contributions from the Kwasan and Hida Observatories, University of Kyoto, No. 276.  相似文献   

The Bragg Crystal Spectrometer for SOLAR-A     

J. L. Culhane  E. Hiei  G. A. Doschek  A. M. Cruise  Y. Ogawara  Y. Uchida  R. D. Bentley  C. M. Brown  J. Lang  T. Watanabe  J. A. Bowles  R. D. Deslattes  U. Feldman  A. Fludra  P. Guttridge  A. Henins  J. Lapington  J. Magraw  J. T. Mariska  J. Payne  K. J. H. Phillips  P. Sheather  K. Slater  K. Tanaka  E. Towndrow  M. W. Trow  A. Yamaguchi 《Solar physics》1991,136(1):89-104

The Bragg Crystal Spectrometer (BCS) is one of the instruments which makes up the scientific payload of the SOLAR-A mission. The spectrometer employs four bent germanium crystals, views the whole Sun and observes the resonance line complexes of H-like Fexxvi and He-like Fexxv, Caxix, and Sxv in four narrow wavelength ranges with a resolving power (/) of between 3000 and 6000. The spectrometer has approaching ten times better sensitivity than that of previous instruments thus permitting a time resolution of better than 1 s to be achieved. The principal aim is the measurement of the properties of the 10 to 50 million K plasma created in solar flares with special emphasis on the heating and dynamics of the plasma during the impulsive phase. This paper summarizes the scientific objectives of the BCS and describes the design, characteristics, and performance of the spectrometers.After the launch the name of SOLAR-A has been changed to YOHKOH.Tragically Professor K. Tanaka died on January 2, 1990.  相似文献   

Large-Scale Active Coronal Phenomena in YOHKOH SXT Images. III. Enhanced Post-Flare Streamer     

Švestka  Zdeněk  Fárník  František  Hick  Paul  Hudson  Hugh S.  Uchida  Yutaka 《Solar physics》1997,176(2):355-371

We demonstrate several events where an eruptive flare close to the limb gave rise to a transient coronal streamer visible in X-rays in Yohkoh SXT images, and analyze one of these events, on 28–29 October 1992, in detail. A coronal helmet streamer began to appear 2 hours after the flare, high above rising post-flare loops; the streamer became progressively narrower, reaching its minimum width 7–12 hours after the flare, and widened again thereafter, until it eventually disappeared. Several other events behaved in a similar way. We suggest that the minimum width indicates the time when the streamer became fully developed. All the time the temperature in the helmet streamer structure was decreasing, which can explain the subsequent fictitious widening of the X-ray streamer. It is suggested that we may see here two systems of reconnection on widely different altitudes, one giving rise to the post-flare loops while the other creates (or re-forms) the coronal helmet streamer. A similar interpretation was suggested in 1990 by Kopp and Polettofor post-flare giant arches observed on board the SMM; indeed, there are some similarities between these post-flare helmet streamers and giant arches and, with the low spatial resolution of SMM instruments, it is possible that some helmet streamers could have been considered to be a kind of a giant arch.  相似文献   

Zooplankton investigations in Yatsushiro-kai,western Kyushu,I     

Reiichiro Hirota  Makoto Hara 《Journal of Oceanography》1975,31(3):115-123

The occurrence of the zooplankton at 21 stations in Yatsushiro-kai, western Kyushu, was investigated in June, September and November of 1968, and March of 1969. Copepods formed the most predominant constituent among the collected Zooplankton. AlthoughParacalanus parvus was abundant in most of the surveyed region, other copepods occurred dominantly in the following order when going from the northeastern area toward the southwest: Oithona nana→Acartia clausi→Microsetella norvegica→Oithona similis→Corycaeus spp. Yatsushiro-kai can be characterized biologically by dividing it into two main regions. The northern half is more embaymental and the southern half is more oceanic, bordered by an area whereMicrosetella norvegica occurred as the dominant. The area whereAcartia clausi occurred dominantly is the most embaymental in the northern half, and the area whereCorycaeus spp. occurred dominantly is the most oceanic in the southern half.  相似文献   

Effect of dietary docosahexaenoic acid on lipogenesis and lipolysis in black sea bream, Acanthopagrus schlegeli   总被引：2，自引：0，他引：2  

JI Hong  OM Ahamd Dau  YOSHIMATSU Takao  UMINO Testuy  NAKAGAWA Heisuke  FURUHASHI Makoto  SAKAMOTO Shuichi 《海洋学报(英文版)》2007,26(1):112-121

1 IntroductionIt is well known that varying dietary fatty acidprofile affects the tissue fatty acid composition and e-ven the growth performance in fish ( Bell et al.,2002; Figueiredo -Silva et al., 2005; Harel andPlace, 2003; Schulz et al., 2005; Tocher et al.,2003). Docosahexaenoic acid (DHA), an importantessential fatty acid for marine species, has the effectnot only on the fatty acid profile of fish body tissue,but also on biological and physiological conditions(Ishizaki et al., 2000; …  相似文献   

Growth characteristics ofChattonella antiqua     

Yasuo Nakamura  Makoto M. Watanabe 《Journal of Oceanography》1983,39(4):151-155

Nutrient requirements of a red tide flagellate,Chattonella antiqua, were investigated in a laboratory culture experiment. Growth ofC. antiqua was supported by nitrate and ammonium, and by urea to a limited extent, but not by glycine, alanine and glutamate. Orthophosphate served as a good phosphorus source but glycerophosphate did not. Fe³⁺ (1µM) fully promoted the flagellate's growth in the presence of 80µM of EDTA. The addition of Mn²⁺ (0–20µM), Zn²⁺ (0–10µM) and Co²⁺ (0–0.4µM) did not show any effect. Among three vitamins tested, only B₁₂ (6 ng 1^?1) served as a growth factor. Glucose, acetate and glycolate did not improve growth in the light nor did they support growth in darkness. The minimum cell quotas for nitrogen, phosphorus, iron and B₁₂ were estimated to be 11 pmoles ce^?1, 1.0, ～0.09 and 1.1 fg cell^?1, respectively.  相似文献