Evapotranspiration and water source of a tropical rainforest in peninsular Malaysia          下载免费PDF全文

Marryanna Lion  Yoshiko Kosugi  Satoru Takanashi  Shoji Noguchi  Masayuki Itoh  Masanori Katsuyama  Naoko Matsuo  Siti‐Aisah Shamsuddin 《水文研究》2017,31(24):4338-4353

To evaluate water use and the supporting water source of a tropical rainforest, a 4‐year assessment of evapotranspiration (ET) was conducted in Pasoh Forest Reserve, a lowland dipterocarp forest in Peninsular Malaysia. The eddy covariance method and isotope signals of rain, plant, soil, and stream waters were used to determine forest water sources under different moisture conditions. Four sampling events were conducted to collect soil and plant twig samples in wet, moderate, dry, and very dry conditions for the identification of isotopic signals. Annual ET from 2012 to 2015 was quite stable with an average of 1,182 ± 26 mm, and a substantial daily ET was observed even during drought periods, although some decline was observed, corresponding with volumetric soil water content. During the wet period, water for ET was supplied from the surface soil layer between 0 and 0.5 m, whereas in the dry period, approximately 50% to 90% was supplied from the deeper soil layer below 0.5‐m depth, originating from water precipitated several months previously at this forest. Isotope signatures demonstrated that the water sources of the plants, soil, and stream were all different. Water in plants was often different from soil water, probably because plant water came from a different source than water that was strongly bound to the soil particles. Plants showed no preference for soil depth with their size, whereas the existence of storage water in the xylem was suggested. The evapotranspiration at this forest is balanced and maintained using most of the available water sources except for a proportion of rapid response run‐off.  相似文献   

临夏盆地新生代沉积物高分辨率岩石磁学记录与亚洲内陆干旱化过程及原因   总被引：4，自引：0，他引：4       下载免费PDF全文

方小敏  徐先海  宋春晖  韩文霞  孟庆泉  鸟居雅之 《第四纪研究》2007,27(6):989-1000

亚洲内陆干旱化是全球新生代大陆环境变化中最引人瞩目的重大事件,与新生代全球变冷和青藏高原隆升密切相关.文章通过对甘肃临夏盆地几乎连续的新生代沉积物系统岩石磁学性质研究,获取了高分辨率磁化率和非磁滞剩磁记录,揭示在29.0～8.6 Ma的漫长的以湖相粉砂岩和泥岩为主的渐新世晚期和中新世早、中期没有明显的长期变化,从8.6Ma开始持续增加,尤其从6.4Ma和5.3Ma开始表现出两次快速持续增加.同时,以8.6Ma为界磁性矿物相对含量发生明显变化,此前以赤铁矿为主,磁铁矿和磁赤铁矿次之,此后以磁铁矿和磁赤铁矿为主,赤铁矿次之,磁性矿物类型和性质类似于风成红粘土和黄土.因此,我们将这种沉积物中磁性矿物组合、性质和含量的长期变化解释为流域外风成物质的加入,指示我国西北内陆现代干旱气候可能从8.6Ma开始,7.4～6.4 Ma后急剧加速变干,5.3Ma后再次加速变干,并最终形成今天的干旱区的过程.9～8 Ma开始的青藏高原阶段性快速隆升和随后的全球变冷可能是驱动亚洲内陆干旱化进程的动力.  相似文献   

Wind Fields over Funka Bay and Their Effect on Water Circulation in the Bay     

Jun Inoue  Masayuki Kawashima  Kay I. Ohshima  Yasushi Fujiyoshi  Ken-ichi Maruyama 《Journal of Oceanography》2000,56(5):507-515

Horizontal wind fields over Funka Bay during cold air outbreaks were simulated using a 3-D meso-scale atmospheric model. The simulated wind fields over the bay have a positive curl in the north and a negative curl in the south. These wind fields were used to simulate the current in Funka Bay using a barotropic ocean model. The simulated current pattern was composed of two vortices—one with anti-clockwise vorticity in the north and the other with clockwise vorticity in the south—and was in the opposite direction to that simulated by the uniform wind fields. This is because the wind stress curl effect on the vorticity production in Funka Bay opposes and overwhelms the bathymetry torque effect during cold air outbreaks. These results show that the non-uniformity of the wind fields caused by the land topography around a shallow lake or bay cannot be neglected in simulating its currents.  相似文献   

Diurnal Cycle of Sound Scatterers and Measurements of Turbidity Using ADCP in Beppu Bay   总被引：2，自引：0，他引：2  

Xiao-Hua Zhu  Yoshio Takasugi  Masayuki Nagao  Eisuke Hashimoto 《Journal of Oceanography》2000,56(5):559-565

From September 20 to 22 in 1994, the vertical profiles of echo intensity and three-component velocities were measured with a bottom-mounted 300 kHz broadband acoustic Doppler current profiler (ADCP) in Beppu Bay in the Seto Inland Sea of Japan. A very strong thermocline was observed from 50 to 60 m. A pronounced diurnal cycle of backscatter strength (BS) was found above the thermocline. However, it was not found under the thermocline where there was a lack of dissolved oxygen. We suggest that the diurnal cycle of BS is caused by the vertical migration of zooplankton. The downward and upward migration occurred in early morning and late afternoon, respectively. The migration speeds estimated from BS isopleth displacements were about 1 cm s^–1. Further, the contribution of turbidity (Tur) to BS was examined by separating out the effect of migrating zooplankton. There was a significant correlation between BS and turbidity under the thermocline. The maximum contributions of the Tur, migrating zooplankton and non-migrating plankton on BS were estimated at 3, 12, 25 dB, respectively. These data suggest that when using an ADCP to estimate Tur, it is very important to consider carefully the backscatter signal from zooplankton.  相似文献   

A Late Holocene geomagnetic secular variation record from Erhai Lake, southwest China   总被引：1，自引：0，他引：1  

Masayuki Hyodo  Arata Yoshihara  Kenji Kashiwaya  Takashi Okimura  Toshiyuki Masuzawa  Ryotaro Nomura  Shingo Tanaka  Tang Bang Xing  Liu Su Qing  & Liu Shi Jian 《Geophysical Journal International》1999,136(3):784-790

A secular variation record of the geomagnetic field direction for the last 6.5  kyr has been obtained from the magnetization of sediment cores from Erhai Lake, southwest China. In order to make a comparison with this record, secular variation in east-central China was investigated by combining available magnetic field data from historical records and archaeomagnetic measurements since about 350 bc . The secular variation in Erhai Lake shows features consistent with the combined record, except for the oldest three observed declination swings in Sian from 720 to 900 ad . Many features of declination and inclination in China also occur in Japan. From 500 to 1000 ad , declination was westerly ranging from about −20° to −5° in Erhai Lake, east-central China, and Japan.  相似文献   

Similarity solution for the interaction of the stellar wind with surrounding interstellar medium     

Shiro Sakashita  Hitoshi Hanami  Masayuki Umemura 《Astrophysics and Space Science》1984,98(2):315-321

Similarity solution for the interaction of stellar wind with surrounding interstellar medium is obtained on the base of momentum conservation. The conversion efficiency of kinetic energy of stellar wind into the kinetic energy of expanding shell is derived. The results are compared with the observations on the ring nebulae associated with the Wolf-Rayet star and it is shown that the observed values of energy conversion are in good agreement with the momentum conserving model.  相似文献   

The first confirmed Perseid lunar impact flash     

Masahisa Yanagisawa  Kouji Ohnishi  Hiroshi Masuda  Miyoshi Ida  Masayuki Ishida 《Icarus》2006,182(2):489-495

The first confirmed lunar impact flash due to a non-Leonid meteoroid is reported. The observed Perseid meteoroid impact occurred at 18^h28^m27^s on August 11, 2004 (UT). The selenographic coordinates of the lunar impact flash are 48±1° N and 72±2° E, and the flash had a visual magnitude of ca. 9.5 with duration of about 1/30 s. The mass of the impactor is estimated to have been 12 g based on a nominal model with conversion efficiency from kinetic to optical energy of 2×¹⁰⁻³. Extrapolation of a power law size-frequency distribution fitting the sub-centimeter Perseid meteoric particles to large meteoroids suggests that several flashes should have been observed at this optical efficiency. The detection of only one flash may indicate that the optical efficiency for Perseid lunar impact is much lower, or that the slope of the size distribution differs between large meteoroids and typical sub-centimeter meteoric particles.  相似文献   

南极中山站午后极光强度与太阳风参数的关系          下载免费PDF全文

胡红桥  刘瑞源  杨惠根  王敬芳  Natsuo Sato  Masayu kiKikuchi  李升贵 《极地研究》2001,13(3):151-158

本文利用1997年和1998年南极中山站多通道扫描光度计的地面观测数据和WIND卫星在弓激波上游对太阳风参数的观测数据，对午后高纬极光强度与太阳风等离子体密度、动压以及太阳风速度之间的相关性进行了定量研究。研究表明，午后极光630．0nm的强度与太阳风等离子体参数之间有较好的相关，630．0nm的强度表现出随太阳风等离子体密度、动压和速度的增大而增加的趋势，其相关系数分别为0．84、0．88和0．61；而557．7nm极光的强度与太阳风等离子体参数之间的相关较差。午后557．7nm极光的强度与太阳风等离子体参数之间的相关较差。午后557．7nm和630．0nm对太阳风参数的不同响应表明太阳风对630．0nm影响更直接，而557．7nm受到了磁层动力学过程的影响。  相似文献   

Long-term features of drifting and standing non-dipole fields as determined from Holocene palaeomagnetic secular variations     

Chizu Itota  Masayuki Hyodo  Katsumi Yaskawa 《Geophysical Journal International》1997,130(2):390-404

Geomagnetic field motions of Holocene secular variations are investigated using a separation method. The palaeomagnetic secular variations from Britain, North America and Australia have been subjected to maximum-entropy method analyses. Based on the results of spectral analyses, the secular variations are separated by band-pass filters into low-frequency components, generally including the period band 1800-3600 yr, and high-frequency components, generally including the period band 1000-1200 yr. There is an interval, from 4200 to 1700 yr BP, which shows clockwise rotational motions in the low-frequency components of all three sites. Westward drifting of geomagnetic fields may be globally dominant. Swinging or elliptical looping motions constrained to a certain direction were observed in the low-frequency components of the British data. The time duration for the persistence of the swinging motion constrained to a certain direction was 3500 years or so, which could be the lifetime of an oscillating stationary field. The duration of the transitional motion was 1000-1300 years, which may indicate the recurrence time of a stationary field.  相似文献   

The distribution of chlorophylla,protein, RNA and DNA in the North Pacific Ocean     

Masayuki Takahashi  Hiroko Nagai  Yukuya Yamaguchi  Shun-ei Ichimura 《Journal of Oceanography》1974,30(3):137-150

Chla, protein, RNA and DNA were measured in 400 samples taken from the surface down to 5,000 m at 27 oceanographical stations in the North Pacific Ocean. Two section diagrams of these cellular constituents were given along 155°E and 155°W meridians, and several vertical profiles of the four constituents were also given at some stations near Japan. The average concentration ranges of Chla, protein, RNA and DNA obtained in this study area were 0.025–0.862, 11.4–88.1, 1.36–35.3 and 0.13–5.24g/l, respectively. Chla was distributed mostly in the photic zone as we would expect. However protein, RNA were in high concentrations within the photic zone and sometimes extremely high concentrations in the deep aphotic zone.  相似文献