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71.
Peng K. Hong Seiji Sugita Yasuhito Sekine Naruhisa Takatoh Tetsuharu Fuse Hideyo Kawakita Eliot F. Young Kosuke Kurosawa Junichi Haruyama Toshihiko Kadono Shunichi Kamata Tomohiko Sekiguchi Hirotomo Noda 《Icarus》2011,214(1):21-29
The Lunar Crater Observation and Sensing Satellite (LCROSS) mission was an impact exploration searching for a volatile deposit in a permanently shadowed region (PSR) by excavating near-surface material. We conducted infrared spectral and imaging observations of the LCROSS impacts from 15 min before the first collision through 2 min after the second collision using the Subaru Telescope in order to measure ejecta dust and water. Such a ground-based observation is important because the viewing geometry and wavelength coverage are very different from the LCROSS spacecraft. We used the Echelle spectrograph with spectral resolution λ/Δλ ∼ 10,000 to observe the non-resonant H2O rotational emission lines near 2.9 μm and the slit viewer with a K′ filter for imaging observation of ejecta plumes. Pre-impact calculations using a homogeneous projectile predicted that 2000 kg of ejecta and 10 kg of H2O were excavated and thrown into the analyzed area immediately above the slit within the field of view (FOV) of the K′ imager and the FOV of spectrometer slit, respectively. However, no unambiguous emission line of H2O or dust was detected. The estimated upper limits of the amount of dust and H2O from the main Centaur impact were 800 kg and 40 kg for the 3σ of noise in the analyzed area within the imager FOV and in the slit FOV, respectively. If we take 1σ as detection limit, the upper limits are 300 kg and 14 kg, respectively. Although the upper limit for water mass is comparable to a prediction by a standard theoretical prediction, that for dust mass is significantly smaller than that predicted by a standard impact theory. This discrepancy in ejecta dust mass between a theoretical prediction and our observation result suggests that the cratering process induced by the LCROSS impacts may have been substantially different from the standard cratering theory, possibly because of its hollow projectile structure. 相似文献
72.
从20世纪50年代到80年代长江宜昌水文站观测的泥沙输送量逐年增加,但是到了90年代却出现了逐渐减少的趋势。泥沙量增加的原因主要是乱伐森林和土地利用方式的快速改变,而减少的原因则可能是采取了一系列防止水土流失的对策和在上游修建了许多大坝而造成的。嘉陵江流域是长江泥沙的主要源区之一,90年代每年从嘉陵江流域到长江的输沙量减少到1988年前的约36%。因此,分析该流域每年泥沙输送动态及其变化原因,对制定减小水土流失的森林规划,防止三峡水库的淤积以及保护长江流域的生存环境和生态系统等具有重大意义。本研究开发并改进了一个流域集水坡面上的侵蚀模型,并将它应用到1987年的嘉陵江流域,以对其适用性进行了研究。结果表明,该模式可被用于月度泥沙生产量的评估中。 相似文献
73.
M. Lutfi Firdaus Kazuhiro Norisuye Yusuke Nakagawa Seiji Nakatsuka Yoshiki Sohrin 《Journal of Oceanography》2008,64(2):247-257
Dissolved and labile particulate Zr, Hf, Nb, Ta, Mo and W were determined at stations K1 (51°N, 165°E), K2 (47°N, 160°E),
KNOT (44°N, 155°E) and 35N (35°N, 160°E) in the western North Pacific Ocean. A portion of seawater for dissolved species (D)
was passed through a 0.2 μm Nuclepore filter and acidified to pH 2.2 with HCl and HF. A portion of seawater for acid-dissolvable species (AD) was acidified
without filtration. Labile particulate (LP) species is defined as AD minus D, which represents a chemically labile fraction
of particulate species. D-Zr, Hf and Ta increase with depth, Nb shows a slight depletion in surface water, whereas Mo and
W have a conservative vertical profile. The concentration range of D-Zr, Hf, Nb, Ta and W is 31–275, 0.14–0.95, 4.0–7.2, 0.08–0.29
and 40–51 pmol kg−1, respectively, whereas that of Mo is 97–105 nmol kg−1. LP-species of Zr, Hf and Ta account for 10–14% of AD in average and increase up to 25% below 4000 m, whereas those for Mo
and W are negligible. In contrast, LP-Nb shows maxima (up to 27%) in surface water. We also found that D-Zr/Hf, Nb/Ta and
Mo/W mole ratios generally increase in the order continental crust < river water < coastal sea < open ocean. 相似文献