Emergence Patterns of Small Subtidal Arthropods in Relation to Day/Night, Tidal, and Surface/Bottom Factors: Investigations in the Boreal Sea, Japan (Akkeshi, Hokkaido)     

Masayuki Saigusa  Kazushi Oishi  Akihiro Ikumoto  Hiroshi Iwasaki  Michihiro Terajima 《Journal of Oceanography》2000,56(3):295-310

The emergence of small arthropods was studied in the boreal sea, Japan (Akkeshi, Hokkaido). In the shallow subtidal zone, two impeller pumps were set in the surface and bottom waters. The pumps ran continuously for 25 days (22 August-16 September, 1998), and invertebrates were sampled using a nylon net (300 to 500 m in mesh size). The small arthropods collected with the net belonged to 16 orders comprising about 60 taxa. In the dominant 23 taxa, a two-way ANOVA was applied to determine whether there was any significant difference in abundance between day and night and between surface and bottom. While emergence of 15 taxa (65%) was significantly different with regard to the day/night factor, that of the other 8 taxa (35%) was not. As to the difference between the two depths, the distribution of 15 taxa (65%) was significantly different. Furthermore, in 25 taxa for which over 100 specimens were collected in each of the two depths of water, emergence patterns were examined with regard to the synchrony with day/night and tidal cycles. There were various nocturnal patterns, and the strength of the synchrony with the day/night cycle was different for each species or group. Within the same taxa, nocturnal patterns were more clearly manifested in the surface water than in the bottom water. A tidal rhythm of emergence was only seen in zoeas of shrimp. Variations of the emergence patterns of benthic crustaceans are accounted for by a hypothesis that the frequency of swimming during day versus at night is different in each species. On the other hand, the emergence patterns of some zooplankton reflect by the daily rhythm of vertical migration or dispersal in the water column.  相似文献   

The ocean/continent transition along a profile through the Lofoten basin,Northern Norway     

Andreas Goldschmidt-Rokita  Knut J. F. Hansch  Hans B. Hirschleber  Takaya Iwasaki  Toshihiko Kanazawa  Hideki Shimamura  Markvard A. Sellevoll 《Marine Geophysical Researches》1994,16(3):201-224

The Cenozoic margins of the Norwegian-Greenland Sea offer ideal conditions for passive margin studies. A series of structural elements, first observed on these margins, led to the concept of volcanic passive margins. Questions still remain about the development of such features and the location of the boundary between oceanic and continental crust. Despite the thin sediment cover of the margins, seismic reflection data are not able to image the deeper structures due to the occurrence of igneous rocks at shallow depth.This paper presents a 320-km long profile perpendicular to the strike of the main structural units of the Lofoten Margin in Northern Norway. A geological model is proposed, based on observations made with ocean bottom seismographs, which recorded seismic refraction data and wide angle reflections, along with a seismic reflection profile covering the same area. Ray-tracing was used to calculate a geophysical model from the shelf area into the Lofoten basin. The structures typical of a volcanic passive margin were found, showing that the Lofoten Margin was influenced by increased volcanic activity during its evolution. The ocean/continent transition is located in a 30-km wide zone landwards of the Vøring Plateau escarpment.The whole margin is underlain by a possibly underplated, high velocity layer. Evidence for a pre-rift sediment basin landwards of the escarpment, overlain by basalt flows, was seen. These structural features, related to extensive volcanism on the Lofoten Margin, are not as distinct as further south along the Norwegian Margin. Viewed in the light of the hot-spot theory of White and McKenzie (1989) the Lofoten Margin can be interpreted as a transitional type between volcanic and non-volcanic passive margin.  相似文献   

Studies on the red tide flagellates—VI     

H. Iwasaki 《Journal of Oceanography》1971,27(4):152-157

Extensive bloom of red tide, accompanying mass mortality of fish and the other animals, occurred in Bingo-Nada, the Seto Inland Sea, in August, 1970. Two species of microorganisms,Eutreptiella sp. andExuviaella sp., were isolated from the water and were obtained in axenic culture by micropipette washings.These organisms are stimulated by trace metals. The highest growth resulted from the addition of chelated Fe (<3 mg/l) or/and Mn (<2 mg/l) to enriched sea water. The organisms prefer low salinity. The optimal salinities are Cl 8.0–17.0 forEutreptiella sp., Cl >11.0 forExuviaella sp. respectively. These organisms can tolerate a wide range of pH.Exuviaella sp. needs vitamin B₁₂ for growth. The pattern of specificity toward B₁₂ analogues²⁾ is similar to that ofEuglena gracilis. On the other hand,Eutreptiella sp. requires B₁₂, biotin, and thiamine. The B₁₂ specificity fits toEscherichia coli. Both organisms prefer NH₄-N in lower concentrations than 1 mg/l (optimal 0.3 mg/l) as nitrogen sources.Exuviaella sp. also likes urea. Inorganic and organic phosphates are utilized by the organisms:Eutreptiella sp. utilizes Na₂-glycerophosphate, guanylic acid,Exuviaella sp. utilizes Na₂-glycerophosphate, adenylic acid. KH₂PO₄ is the most favorable to the growth of both organisms. All the purines, pyrimidines, plant hormones tested increase the growth ofExuviaella sp. Especially, guanine, xanthine, thymine, indoleacetic acid, and gibberellic acid promote the growth remarkably.These organisms do not grow to high densities without Fe or/and Mn in high concentrations even under the conditions provided by optimal temperature, salinities, pH, and essential nutrients. On the other hand, the coastal area of Fukuyama where the red tide first occurred has been fertilized with the nutrients essential to the organisms, and also polluted with trace metals such as Fe (Iwasaki, Inoue unpublished data). From these results, it can be considered that the great increase of the organisms is caused principally by the high concentration of iron in the sea water.  相似文献   

Distribution of moon jellyfish Aurelia aurita in relation to summer hypoxia in Hiroshima Bay,Seto Inland Sea     

Jun Shoji  Takaya Kudoh  Hideyuki Takatsuji  Osamu Kawaguchi  Akihide Kasai 《Estuarine, Coastal and Shelf Science》2010,86(3):485-490

Biological and physical surveys were conducted in order to investigate the relationship between environmental conditions and the distribution of moon jellyfish Aurelia aurita in Hiroshima Bay, western Seto Inland Sea, Japan. Moon jellyfish and ichthyoplankton were collected at 13 stations in Hiroshima Bay during monthly surveys from July to September in 2006 and 2007. Surface temperature in 2006 was significantly lower during the August and September cruises and surface salinity was lower during all cruises than in 2007. Moon jellyfish was the most dominant gelatinous plankton collected, accounting for 89.7% in wet weight. Mean moon jellyfish abundance in 2006 was higher than that in 2007 from July through September, with significant inter-year differences for July and September. Variability in precipitation and nutritional input from the Ohta River, northernmost part of Hiroshima Bay, were suggested as possible factors affecting the inter-annual variability in moon jellyfish abundance in the coastal areas of northern Hiroshima Bay. Moon jellyfish were more abundant in the coastal areas of northern Hiroshima Bay, where the dissolved oxygen (DO) concentration was lower, while low in the central part of the bay. Japanese anchovy Engraulis japonicus eggs were most dominant (58.1% in number) among the ichthyoplankton and were abundant in the central area of Hiroshima Bay. Explanatory analysis was conducted to detect possible effects of environmental conditions on the abundance of moon jellyfish and Japanese anchovy eggs during the summer months in Hiroshima Bay. Of the environmental conditions tested (temperature, salinity and DO of surface and bottom layers at each sampling station), bottom DO had the most significant effect on the moon jellyfish abundance: there was a negative correlation between the bottom DO and the moon jellyfish abundance in Hiroshima Bay during summer.  相似文献   

Temporal Variations of Seismic Wave Velocity Associated with 1998 M6.1 Shizukuishi Earthquake     

A. Nakamura  A. Hasegawa  N. Hirata  T. Iwasaki  H. Hamaguchi 《Pure and Applied Geophysics》2002,159(6):1183-1204

—?We attempt to detect temporal variations of seismic wave velocity before and after 1998 M6.1 Shizukuishi, northeastern Japan, earthquake by using waveform data from explosions and earthquake doublets spanning the period immediately before and after the earthquake. Direct P waves of the second explosion are delayed by ～20 ms at observation stations with epicentral distances less than 15 km. This tendency does not change if the analysis frequency band is changed. Our result suggests that the P-wave velocity decreased by at least 1% in the extremely shallow region of the hanging wall of the M6.1 thrust event after its occurrence. On the other hand, there was the frequency dependence of the coda wave delays for both artificial sources and for natural events. At 5–10 Hz, immediate sharp increases by more than 20 ms in time delays and lower coherency were observed at several stations. We estimated the region in which P-wave velocity might have decreased after the M6.1 earthquake. Maximum depth of the region is 13 km. The region includes the aftershock area of the M6.1 earthquake, but is eccentric to the earthquake in the west. Considering the frequency band analyzed (5–10 Hz), the scale of the spatial inhomogeneity which led to the coda wave delay is several hundreds meters. We investigated candidates for the cause of the direct P-wave and coda wave delay. Observed direct P-wave delay can be partly explained by the stress changes caused by coseismic fault slip. However, the coda wave delay cannot be explained by the stress changes that are limited to the superficial area. Crustal heterogeneity should have changed at coseismic time in the deeper area where aftershocks of the M6.1 earthquake occurred.  相似文献   

S-wave anisotropy off Lofoten, Norway, indicative of fluids in the lower continental crust?   总被引：2，自引：0，他引：2  

Rolf Mjelde  Markvard A. Sellevoll  Hideki Shimamura  Takaya Iwasaki  Toshihiko Kanazawa 《Geophysical Journal International》1995,120(1):87-96

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Groundwater microtemperature in earthquake regions     

Hideki Shimamura  Morio Ino  Hisayoshi Hikawa  Takaya Iwasaki 《Pure and Applied Geophysics》1984,122(6):933-946

Microtemperature measurements of groundwater with a relative precision better than 1/1000°C have been made in several seismically active areas in Japan. The measured temperatures show clear coseismic signals as well as a correlation with atmospheric pressure. Simultaneous observations at various depths have shown that these temperature changes were not induced by simple groundwater level changes. Also, distinctive signals occurred before several earthquakes and seem to be caused by a different mechanism than the coseismic signals. The microtemperature at some observation sites shows excellent correlation with records of nearby sensitive borehole strainmeters. Simultaneous recording of microtemperature and strain has been initiated in some boreholes.  相似文献   

Structural factors controlling the rupture process of a megathrust earthquake at the Nankai trough seismogenic zone   总被引：7，自引：0，他引：7  

S. Kodaira  E. Kurashimo  J.-O. Park  N. Takahashi  A. Nakanishi  S. Miura  T. Iwasaki  N. Hirata  K. Ito  Y. Kaneda 《Geophysical Journal International》2002,149(3):815-835

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Dynamical behaviour of planetesimals temporarily captured by a planet from heliocentric orbits: basic formulation and the case of low random velocity     

Kazunori Iwasaki  Keiji Ohtsuki 《Monthly notices of the Royal Astronomical Society》2007,377(4):1763-1771

Planetesimals encountering with a planet cannot be captured permanently unless energy dissipation is taken into account, but some of them can be temporarily captured in the vicinity of the planet for an extended period of time. Such a process would be important for the origin and dynamical evolution of irregular satellites, short-period comets, and Kuiper-belt binaries. In this paper, we describe the basic formulation for the study of temporary capture of planetesimals from heliocentric orbits using three-body orbital integration, such as the definition of the duration and rate of temporary capture, and present results in the case of low random velocity of planetesimals. In the case of planetesimals initially on circular orbits, we find that planetesimals undergo a close encounter with the planet before they become temporarily captured. When planetesimals are scattered by the planet into the vicinity of one of periodic orbits around the planet, the duration of temporary capture tends to be extended. Typically, these capture orbits are in the retrograde direction around the planet. We evaluate the rate of temporary capture of planetesimals, and find that the ratio of this rate to their collision rate on to the planet increases with increasing semimajor axis of the planet. Similar results are obtained for planetesimals with non-zero but small random velocities, as long as Kepler shear dominates the relative velocity between the planet and planetesimals. For larger initial random velocities of planetesimals, temporary capture in both prograde and retrograde directions with much longer duration becomes possible.  相似文献   

Geochemical indicators and seismic phenomena     

Iwasaki  I. 《Bulletin of Volcanology》1975,39(1):82-90

Bulletin of Volcanology - The results obtained from the study of the Atami Geyser. of Hakone Volcano fumaroles, and of Kagai hot springs can be used for the geochemical prediction of ‘great...  相似文献