On the surface distribution of chemical anomalies of Ap stars in spectroscopic binary systems     

M. Kitamura 《Astrophysics and Space Science》1980,68(2):283-294

By estimating the orbital inclinations of non-eclipsing Ap spectroscopic binaries with periods less than 13 days, we can obtain a marked statistical result on the frequency distribution of the inclinations which strongly suggests that the abundance anomalies of Ap components tend to concentrate towards the stellar polar region. This would provide a critical test for models of Ap stars.  相似文献   

Phase diagrams describing solid-gas equilibria in the system Fe-Mg-Si-O-C-H,and its bearing on redox states of chondrites     

Akira Tsuchiyama  Masao Kitamura 《Meteoritics & planetary science》1995,30(4):423-429

Abstract— Phase diagrams describing solid-gas equilibria in the system Fe-Mg-Si-O-C-H under H-rich conditions (～700–2000 K and 10^?2–10^?20 atm of Ph ₂), including solar nebula conditions, were constructed based on thermochemical calculations. Boundaries of vaporous phases, which are the first phases to condense from a gas, can be obtained without calculating condensation temperatures of individual gas compositions because the numbers of major gaseous species are the same as those of components in the concerned systems. Fractionations by condensation and/or evaporation can be discussed easily in such phase diagrams. A thermal divide, which is a barrier that vapors cannot cross by a single cooling process, was recognized in the phase diagrams. This is present on the Fe-MgO-SiO₂-CO-H plane at high temperatures (≥500–700 K) and plays an important role in fractionations. Oxidizing states of ordinary chondrites and carbonaceous chondrites before aqueous alteration are located at the O-rich side of the thermal divide. Such oxidizing states can be formed from the solar gas by fractionation in the primordial solar nebula because the solar composition is located on the O-rich side. On the other hand, the reducing states of enstatite chondrites, located at the O-poor side, cannot be formed as long as the thermal divide is present. The reducing states can be obtained by CO to CH₄ molecular reaction at low temperatures (≤500–700 K), where the high-temperature thermal divide is absent. Addition of H₂O-rich and CH₄-rich ice can explain establishment of the redox states of ordinary and enstatite chondrites, respectively.  相似文献   

基于CMIP5模拟的中国区域陆气耦合强度评估及未来情景预估     

曾毓金  谢正辉 《气候与环境研究》2015,20(3):337-346

基于第五次国际耦合模式比较计划(CMIP5)11个模式历史情景的模拟结果计算得到了中国区域夏季的陆气耦合强度并进行集合平均,结果表明,位于半干旱区的华北和内蒙古地区陆气耦合强度相对较强,西部干旱区的陆气耦合强度相对较弱,位于湿润区的中国东北地区东部、长江中下游和西南地区陆气耦合强度最弱。利用上述模式集合平均结果与由NCEP再分析资料和欧洲中心的中期气象预报40年再分析资料(ERA40)计算得到的陆气耦合强度相比较,结果显示这些模式的集合平均与再分析资料NCEP和ERA40的计算结果有较好的一致性。利用历史情景模拟和不同的典型排放路径(RCP),即低排放情景RCP2.6、中排放情景RCP4.5和高排放情景RCP8.5下的模拟结果预估陆气耦合强度未来变化。结果显示:与历史情景相比较,位于湿润区的中国南方地区蒸散发的主要控制因子是温度,在3种排放情景下随着温度上升引起蒸散发增加所导致陆气耦合强度升高;位于青藏高原以及半干旱区的内蒙古大部分地区蒸散发在未来的年际变化幅度减弱导致陆气耦合指数降低;位于西北干旱区陆气耦合强度在RCP2.6和RCP4.5情景上升,然而在RCP8.5情景下陆气耦合强度下降,其原因是在高排放情景下,水汽平流输送明显增强,局地蒸散发异常对空气湿度变化的贡献减弱,导致了陆气耦合强度降低。未来预估结果在中国南方可信度相对较高,从全国来看,在RCP4.5情景下可信度相对较高。  相似文献   

利用卫星遥感数据监测莱州湾海冰     

赵玉金  赵红 《山东气象》2008,28(3)

主要介绍了利用NOAA和EOS卫星遥感监测莱州湾海冰的方法,简要分析了海冰对不同光谱的反应及海冰和水体在可见光、近红外通道反射率的差异等,对2008年莱州湾海面结冰状况进行了监测,利用国家卫星气象中心提供的海冰厚度计算经验模式,估算了海冰厚度分布及面积。为了使海冰分布更加清晰,对NOAA卫星监测海冰图像进行了彩色增强处理。  相似文献   

Monitoring of Sea Ice Distribution Based on Satellite Remote Sensing Data in Laizhou Bay     

Zhao Yujin  Zhao Hong 《山东气象》2008,28(3)

  相似文献   

Long-term precipitation and stream discharge records at seven forested experimental watersheds along a latitudinal transect in Japan: Jozankei,Kamabuchi, Takaragawa,Tsukuba, Tatsunokuchi-yama,Kahoku and Sarukawa     

Takanori Shimizu  Koji Tamai  Ikuhiro Hosoda  Shoji Noguchi  Yuji Kominami  Toshio Abe  Kenzo Kitamura  Ushio Kurokawa  Delphis F. Levia  Tayoko Kubota  Naoki Kabeya  Shin'ichi Iida  Tatsuhiko Nobuhiro  Shinji Sawano  Sho Iwagami  Akira Shimizu  Yoshio Tsuboyama 《水文研究》2021,35(10):e14376

This data note introduces a database of long-term daily total precipitation and stream discharge data for seven forested watersheds in Japan that have been continuously monitored by the Forestry and Forest Products Research Institute. Three of the watersheds started data collection in the 1930s. Forest cover across the sites ranges from cool to warm temperate regions with the latitude spanning from 31 to 44° N and annual precipitation ranging from 1200 to 3000 mm yr⁻¹. The effects of vegetation change via clearcutting, thinning and forest fire (among other stressors) on stream discharge can be analysed from the long-term observation sites. Moreover, this multi-site dataset allows for inter- and intra-site comparisons of annual water loss (difference of annual precipitation and stream discharge). These long-term datasets can provide comprehensive insights into the effects of climate change and other stressors on forested ecosystems, not only in Japan but across a spectrum of forest types, if combined with other long-term records from other forested watersheds across the world.  相似文献   

福建政和地区"稻香组"问题的探讨   总被引：1，自引：0，他引：1  

揭育金 《福建地质》2004,23(3):124-130

在野外实际调研成果并结合前人资料的基础上,从岩石组合、岩石地球化学特征及构造组合特征等方面分析,认为原“稻香组”建组剖面(政和稻香-高堀剖面),可划分为三套分属不同时代的岩性组合,且将稻香组的定义重新修订。其下部为细砂岩、粉砂岩、硅质岩、泥岩组合,时代暂置晚古生代。三套岩石组合间为构造拼接关系,其性质为逆冲推覆．运动方向由南东向北西,推测逆冲推覆事件发生在晚侏罗世。  相似文献   

The anisotropy of cosmic ray arrival directions around 10 eV     

N. Hayashida  M. Nagano  D. Nishikawa  H. Ohoka  N. Sakaki  M. Sasaki  M. Takeda  M. Teshima  R. Torii  T. Yamamoto  S. Yoshida  K. Honda  N. Kawasumi  I. Tsushima  N. Inoue  E. Kusano  K. Shinozaki  N. Souma  K. Kadota  F. Kakimoto  K. Kamata  S. Kawaguchi  Y. Kawasaki  H. Kitamura  Y. Matsubara  K. Murakami  Y. Uchihori  H. Yoshii 《Astroparticle Physics》1999,10(4):125-311

Anisotropy in the arrival directions of cosmic rays with energies above 10¹⁷ eV is studied using data from the Akeno 20 km² array and the Akeno Giant Air Shower Array (AGASA), using a total of about 114 000 showers observed over 11 years. In the first harmonic analysis, we have found a strong anisotropy of 4% around 10¹⁸ eV, corresponding to a chance probability of 0.2% after taking the number of independent trials into account. with two-dimensional analysis in right ascension and declination, this anisotropy is interpreted as an excess of showers near the directions of the Galactic Center and the Cygnus region.  相似文献   

Variation in the sediment deposition behind check‐dams under different soil erosion conditions on the Loess Plateau,China          下载免费PDF全文

Yanhong Wei  Zhong He  Juying Jiao  Yujin Li  Yixian Chen  Hengkang Zhao 《地球表面变化过程与地形》2018,43(9):1899-1912

To maintain a reasonable sediment regulation system in the middle reaches of the Yellow River, it is critical to determine the variation in sediment deposition behind check‐dams for different soil erosion conditions. Sediment samples were collected by using a drilling machine in the Fangta watershed of the loess hilly–gully region and the Manhonggou watershed of the weathered sandstone hilly–gully (pisha) region. On the basis of the check‐dam capacity curves, the soil bulk densities and the couplet thickness in these two small watersheds, the sediment yields were deduced at the watershed scale. The annual average sediment deposition rate in the Manhonggou watershed (702.0 mm/(km²·a)) from 1976 to 2009 was much higher than that in the Fangta watershed (171.6 mm/(km²·a)) from 1975 to 2013. The soil particle size distributions in these two small watersheds were generally centred on the silt and sand fractions, which were 42.4% and 50.7% in the Fangta watershed and 60.6% and 32.9% in the Manhonggou watershed, respectively. The annual sediment deposition yield exhibited a decreasing trend; the transition years were 1991 in the Fangta watershed and 1996 in the Manhonggou watershed (P < 0.05). In contrast, the annual average sediment deposition yield was much higher in the Manhonggou watershed (14011.1 t/(km²·a)) than in the Fangta watershed (3149.6 t/(km²·a)). In addition, the rainfalls that induced sediment deposition at the check‐dams were greater than 30 mm in the Fangta watershed and 20 mm in the Manhonggou watershed. The rainfall was not the main reason for the difference in the sediment yield between the two small watersheds. The conversion of farmland to forestland or grassland was the main reason for the decrease in the soil erosion in the Fangta watershed, while the weathered sandstone and bare land were the main factors driving the high sediment yield in the Manhonggou watershed. Knowledge of the sediment deposition process of check‐dams and the variation in the catchment sediment yield under different soil erosion conditions can serve as a basis for the implementation of improved soil erosion and sediment control strategies, particularly in semi‐arid hilly–gully regions. Copyright © 2018 John Wiley & Sons, Ltd.  相似文献   

Disruption of Sema3A expression causes abnormal neural projection in heavy oil exposed Japanese flounder larvae     

Kawaguchi M  Song JY  Irie K  Murakami Y  Nakayama K  Kitamura S 《Marine pollution bulletin》2011,63(5-12):356-361

It has been well known that oil spills cause serious problems in the aquatic organisms. In particular, some species of teleosts, which develop on the sea surface thought to be affected by heavy oil (HO). During the embryogenesis, the nervous system is constructed. Therefore, it is important to study the toxicological effects of HO on the developing neurons. We exposed HO to eggs of Japanese flounder (Paralichthys olivaceus) and investigated the neural disorder. In larvae exposed by HO at the concentration of 8.75 mg/L, the facial and lateral line nerves partially entered into the incorrect region and the bundle was defasciculated. Furthermore, in the HO-exposed larvae, Sema3A, a kind of axon guidance molecule, was broadly expressed in second pharyngeal arch, a target region of facial nerve. Taken together, we suggested the possibility that the abnormal expression of Sema3A affected by HO exposure causes disruption of facial nerve scaffolding.  相似文献