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Landslide Hazard and Risk Assessment on the Northern Slope of Mt. Changbai, China 被引量:3
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作者 LIU Zhenghua ZHANG Yanbin +1 位作者 Yoshiharu ISHIKAWA Hiroyuki NAKAMURA 《Acta Geologica Sinica(English Edition)》 SCIE CAS CSCD 2008年第1期214-224,共11页
Landslide hazard and risk assessment on the northern slope of Mt. Changbai, a well-known tourist attraction near the North Korean-Chinese border, are assessed. This study is divided into two parts, namely, landslide h... Landslide hazard and risk assessment on the northern slope of Mt. Changbai, a well-known tourist attraction near the North Korean-Chinese border, are assessed. This study is divided into two parts, namely, landslide hazard zonation and risk assessment. The 1992 Anbalagan and Singh method of landslide hazard zonation (LHZ) was modified and used in this area. In this way, an Associative Analysis Method was used in representative areas to get a measure for controlling factors (slope gradient, relative relief, vegetation, geology, discontinuity development, weak layer thickness and ground water). For the membership degree of factor to slope failure, the middle range of limited values was used to calculate LHZ. Based on an estimation of the potential damage from slope failure, a reasonable risk assessment map was obtained using the relationship of potential damage and probable hazard to aid future planning and prediction and to avert loss of life. 展开更多
关键词 Landslide Hazard Zonation (LHZ) controlling factor Associative Analysis method membership degree risk assessment TOURISM China
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Mass segregation of embedded clusters in the Milky Way
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作者 Xin-Yue Er Zhi-Bo Jiang Yan-Ning Fu 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2013年第3期277-289,共13页
Embedded clusters are ideal laboratories for understanding the early phase of the dynamical evolution of clusters as well as massive star formation. An interesting observational phenomenon is that some of the embedded... Embedded clusters are ideal laboratories for understanding the early phase of the dynamical evolution of clusters as well as massive star formation. An interesting observational phenomenon is that some of the embedded clusters show mass segregation, i.e., the most massive stars are preferentially found near the cluster center. We develop a new approach to describe mass segregation. Using this approach and the Two Micron All Sky Survey Point Source Catalog (2MASS PSC), we analyze 18 embedded clusters in the Galaxy. We find that 11 of them are mass-segregated and that the others are not mass-segregated. No inversely mass-segregated cluster is found. 展开更多
关键词 open clusters and associations: general -- stars: formation -- methods:data analysis
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