Weakening of the solar EUV line emission near the Sun's limb     

Mitsuo Kanno 《Solar physics》1983,89(2):253-259

The weakening of the EUV line emission near the Sun's limb is studied to acquire information about the absorbers causing the weakening. The equivalent optical thickness of the absorbers for the Lyman continuum is determined as a function of the distance from the center of the solar disk by use of Skylab spectroheliograms in Oiv λ554 and Ovi λ1032. It is found that (1) the weakening cannot be explained by shielding of EUV emitting sources in terms of completely opaque spicules and (2) the distribution of the equivalent optical thickness on the solar disk is extremely flat with a maximum at a position of ～ 5″ above the white-light limb. The results imply that the absorbers are a number of mass blobs consisting of cool chromospheric material which overlies the EUV emitting sources. It is suggested that both the EUV emitting sources and the absorbers are the remnants of Hα-emitting spicules which are diffused into the corona.  相似文献   

Seasonal and areal variation of continental aerosol in the surface air over the western North Pacific region   总被引：1，自引：0，他引：1  

Shizuo Tsunogai  Toshitaka Suzuki  Takayoshi Kurata  Mitsuo Uematsu 《Journal of Oceanography》1985,41(6):427-434

Weekly aerosol samples were collected for two years from 1981 at six stations in the western North Pacific region. The samples were analyzed for aluminum to determine the mineral dust concentration in the air. By combining our data with observations in the central and eastern North Pacific by a US research group, the following results and conclusions have been obtained. Spring peaks in atmospheric mineral dust were observed at all the stations accompanied byKosa episodes (hazes due to mineral dust of Chinese origin). The spring peaks, however, varied from year to year. The mean concentration of mineral dust depends not only on the distance from the Asian coast but also on the latitude of the sampling station. The half-decrease distance of the atmospheric mineral dust turned out to be 500–600 km for all latitudes in the western North Pacific. This indicates that the rate of deposition of mineral dust in the western North Pacific is much larger than that in the central and eastern North Pacific.  相似文献   

Atmospheric inorganic nitrogen in marine aerosol and precipitation and its deposition to the North and South Pacific Oceans     

Jinyoung?JungEmail author  Hiroshi?Furutani  Mitsuo?Uematsu 《Journal of Atmospheric Chemistry》2011,68(2):157-181

Aerosol and rain samples were collected between 48°N and 55°S during the KH-08-2 and MR08-06 cruises conducted over the North and South Pacific Ocean in 2008 and 2009, to estimate dry and wet deposition fluxes of atmospheric inorganic nitrogen (N). Inorganic N in aerosols was composed of ~68% NH₄⁺ and ~32% NO₃^– (median values for all data), with ~81% and ~45% of each species being present on fine mode aerosol, respectively. Concentrations of NH₄⁺ and NO₃⁻ in rainwater ranged from 1.7–55 μmol L⁻¹ and 0.16–18 μmol L⁻¹, respectively, accounting for ~87% by NH₄⁺ and ~13% by NO₃⁻ of total inorganic N (median values for all data). A significant correlation (r = 0.74, p < 0.05, n = 10) between NH₄⁺ and methanesulfonic acid (MSA) was found in rainwater samples collected over the South Pacific, whereas no significant correlations were found between NH₄⁺ and MSA in rainwater collected over the subarctic (r = 0.42, p > 0.1, n = 6) and subtropical (r = 0.33, p > 0.5, n = 6) western North Pacific, suggesting that emissions of ammonia (NH₃) by marine biological activity from the ocean could become a significant source of NH₄⁺ over the South Pacific. While NO₃⁻ was the dominant inorganic N species in dry deposition, inorganic N supplied to surface waters by wet deposition was predominantly by NH₄⁺ (42–99% of the wet deposition fluxes for total inorganic N). We estimated mean total (dry + wet) deposition fluxes of atmospheric total inorganic N in the Pacific Ocean to be 32–64 μmol m⁻² d⁻¹, with 66–99% of this by wet deposition, indicating that wet deposition plays a more important role in the supply of atmospheric inorganic N than dry deposition.  相似文献   

A Study Of The Atmospheric Boundary Layer Using Radon And Air Pollutants As Tracers     

Toshio Kataoka  Eiji Yunoki  Mitsuo Shimizu  Tadashige Mori  Osamu Tsukamoto  Yukitaka Ohashi  Ken Sahashi  Toshihiko Maitani  Koh’ichi Miyashita  Toru Iwata  Yoko Fujikawa  Akira Kudo  Roger H. Shaw 《Boundary-Layer Meteorology》2001,101(2):131-156

Concentrations of radon ²²²Rn andair pollutants, meteorological parametersnear the surface and vertical profiles of meteorological elements were measured atUchio (Okayama City, Okayama Prefecture, Japan) 12 km north from the coast ofthe Inland Sea of Japan. In the nighttime, the ²²²Rn concentration increased in the case of weak winds, but did not increase as much in the case of moderate or strong winds, as had been expected. In the daytime, the ²²²Rn concentrationheld at a slightly higher than average level for the period from sunrise to about 1100 JST. It is considered that this phenomenon is due to a period of morning calm, that is, a transition period from land breeze to sea breeze.NO, which is sensitive to traffic volume,brought information concerning advection.Oxidant concentrations,which reflect the availability of sunlight,acted in the reverse manner to ²²²Rnconcentrations. Thus, a set of ²²²Rn and air pollutants could provide useful information regarding the local conditions of the atmospheric boundary layer.  相似文献   

A note on stilpnomelane mineralogy     

Mitsuo Hashimoto 《Contributions to Mineralogy and Petrology》1969,23(1):86-88

Stilpnomelane analyses are classified into two separate groups of ferro- and ferristilpnomelanes on the H₂O(+)-Fe₂O₃/(Fe₂O₃+FeO) diagram. The relation is not comparable with that of oxyhornblende.  相似文献   

Petroloy of the Taga Volcano Group,Izu Peninsula,Central Japan     

Dr. Mitsuo Shimazu  Dr. Kazuhiro Kurihara 《Mineralogy and Petrology》1989,41(1):11-24

The Taga Volcano Group of the Izu Peninsula is divided into four volcanoes: Older Taga, Atami, Shimo-Taga and Himenosawa. Each volcano consists of basalt-andesite lavas and volcaniclastic sediments, mainly of low alkali tholeiite composition.The activity of the Shimo-Taga Volcano is divided into three stages (early, middle and later). Rocks of the first two stages consist of lavas and volcaniclastic sediments of olivine basalt, phyric and aphyric basaltic andesite. The later stage rocks consist of volcaniclastic sediments which were erupted as mudflow deposits.Basalts and andesites of the first two stages are considered to have been derived from a zoned magma chamber. They were produced by fractional crystallization, which involved the gravitational separation of plagioclase, olivine and/or pyroxene crystals. Eruption of aphyric and phyric basaltic andesite from the upper part of the chamber occurred first, followed by olivine basalt from lower parts of the chamber.

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Zusammenfassung Die Taga-Vulkan Gruppe besteht aus dem älteren Taga, dem Atami, dem Shimo-Taga und dem Himenosawa Vulkan. Jeder dieser Vulkane wird aus basaltisch-andesitischen Laven und vulkano-klastischen Sedimenten, hauptsächlich subalkalisch tholeiitischer Zusammensetzung, aufgebaut.Die Eruptionstätigkeit des Shimo-Taga Vulkans läßt sich in drei Phasen, eine Früh-, Mittel- und Spätphase untergliedern. Laven und vulkanoklastische Sedimente der ersten beiden Phasen bestehen aus Olivinbasalten, sowie aus basaltischen Andesiten mit porphyrischem und nichtporphyrischem Gefüge. Während des letzten Stadiums wurden vulkanoklastische Sedimente in Form von vulkanoklastischen Schlammströmen eruptiert.Die Basalte und Andesite der ersten beiden Stadien werden als Produkte einer zonierten Magmenkammer gedeutet. Sie entstanden durch fraktionierte Kristallisation und durch die gravitative Abtrennung von Plagioklas, Olivin und/oder Pyroxenkristallen. Der Eruption der porphyrischen und nichtporphyrischen basaltischen Andesite aus dem obersten Teil der Magmakammer folgte die Eruption von Olivinbasalten aus dem tieferen Teil der Magmakammer.

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Phytoplankton chlorophyll stocks in the Antarctic Ocean   总被引：5，自引：0，他引：5  

Mitsuo Fukuchi 《Journal of Oceanography》1980,36(1):73-84

Phytoplankton chlorophyll stocks in the Indian sector of the Antarctic Ocean were estimated on the basis of published data collected from nine cruises of the Icebreaker,Fuji in 1965–1976, during routine observations of the Japanese Antarctic Research Expedition (JARE). Surface chlorophylla concentration, measured at 631 stations in waters south of 35°S, ranged from 0.01 to 3.01 mg m^–3, At about half of the stations the values were less than 0.24 mg and at only 29 stations were high values more than 1.00 mg m^–3 recorded. The levels of surface chlorophylla stocks were estimated in three groups; (1) data obtained on the southward leg through the eastern Indian sector (middle-late December), (2) those on the northward leg through the western Indian sector (late February–early March) and (3) those on the northward leg through the eastern Atlantic sector (late February–early March). Furthermore, mean values and standard deviations were calculated for each of six different water masses from north to south,i. e., subtropical water between 35°S and the Subtropical Convergence (STC) zone, water within the STC zone, Subantarctic Upper Water, water within the Antarctic Convergence (AC) zone, Antarctic Surface Water between the AC zone and 63°S, and Antarctic Surface Water south of 63°S. Mean values of surface chlorophylla concentrations for each of the six water masses on the three legs ranged from 0.15 to 0.58 mg m^–3 and were comparable to those reported by other workers previously. Seasonal periodicity of phytoplankton chlorophyll stock is discussed. The surface chlorophyll stock in the oceanic water of the Antarctic Ocean does not seem to be so high as previously believed.  相似文献   

Rejuvenated extension of the Philippine Sea plate and its effect on subduction dynamics in the Nankai Trough     

Gaku Kimura  Yasuyuki Nakamura  Kazuya Shiraishi  Gou Fujie  Shuichi Kodaira  Asuka Yamaguchi  Rina Fukuchi  Yoshitaka Hashimoto 《Island Arc》2021,30(1):e12402

The Nankai Trough, Japan, is a subduction zone characterized by the recurrence of disastrous earthquakes and tsunamis. Slow earthquakes and associated tremor also occur intermittently and locally in the Nankai Trough and the causal relationship between slow earthquakes and large earthquakes is important to understanding subduction zone dynamics. The Nankai Trough off Muroto, Shikoku Island, near the southeast margin of the rupture segment of the 1946 Nankai earthquake, is one of three regions where slow earthquakes and tremor cluster in the Nankai Trough. On the Philippine Sea plate, the rifting of the central domain of the Shikoku Basin was aborted at ~15 Ma and underthrust the Nankai forearc off Muroto. Here, the Tosa-Bae seamount and other high-relief features, which are northern extension of the Kinan Seamount chain, have collided with and indented the forearc wedge. In this study, we analyzed seismic reflection profiles around the deformation front of accretionary wedge and stratigraphically correlated them to drilling sites off Muroto. Our results show that the previously aborted horst-and-graben structures, which were formed around the spreading center of the Shikoku Basin at ~15 Ma, were rejuvenated locally at ~6 Ma and more regionally at ~3.3 Ma and have remained active since. The reactivated normal faulting has enhanced seafloor roughness and appears to affect the locations of slow earthquakes and tremors. Rejuvenated normal faulting is not limited to areas near the Nankai Trough, and extends more than 200 km into the Shikoku Basin to the south. This extension might be due to extensional forces applied to the Philippine Sea plate, which appear to be driven by slab-pull in the Ryukyu and Philippine trenches along the western margin of the Philippine Sea plate.  相似文献   

Observations of a compact solar flare on 1981 September 7 in Hα, X-ray,and microwave radiations     

Mitsuo Kanno  Hiroki Kurokawa  The Hinotori Group 《Solar physics》1983,86(1-2):193-194

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The innermost corona observed at the 1973 June 30 eclipse     

Yoichiro Hanaoka  Mitsuo Kanno  Hiroki Kurokawa  Tokio Tsubaki 《Solar physics》1986,106(1):95-106

Slitless flash spectrograms in heights below 8000 km above the solar limb were obtained by the University of Kyoto Expedition at Atar, Mauritania. The integrated intensities of Fexiv 5303, Fex 6374, Fexi 7892, and the continuum are measured as a function of height above the solar limb at eleven points (P.A. = 284–300°) around the third contact point. It is found that a significant amount of the emission in Fex 6374 originates in chromospheric levels well below 8000 km. This implies that the interspicular region of the chromosphere is occupied by coronal material. The average values of the electron temperature and the electron density in the interspicular region are derived from the Fex 6374 and the Fexi 7892 intensities on the assumption of spherical symmetry: T _e = 0.9–1.1 × 10⁶ K and N _e = 9–10 × 10⁸ cm^–3. The intensity variations of the coronal lines and the continuum with position angle are also studied. Strong correlations between Fexiv 5303 and the continuum and between Fex 6374 and Fexi 7892 are found. From the Fex 6374 intensities it is inferred that there is a density fluctuation in the innermost corona by at least a factor of two.Contributions from the Kwasan and Hida Observatories, University of Kyoto, No. 271.  相似文献