Contra evolution revolution torrent torrent#
Based on data from the Austrian Alps, we extended a vulnerability curve for residential buildings affected by fluvial sediment transport processes to other torrent processes and other building types.
The vulnerability of buildings affected by torrent processes can be quantified by vulnerability functions that express a mathematical relationship between the degree of loss of individual elements at risk and the intensity of the impacting process. Vulnerability assessment for elements at risk is an important component in the framework of risk assessment. Mountain torrents: Quantifying vulnerability and assessing uncertainties Further efforts are discussed for improving torrent hazard mapping and prediction. The results are useful for engineering planning support and resource protection in the Hexi Corridor. The torrent hazard map shows that there is high potential torrent hazard in the central and southeastern Hexi Corridor. The results show that the capability of the proposed method is satisfactory. A torrent hazard map for the Hexi Corridor was generated by integrating the driving factors of mountain torrent disasters including precipitation, terrain, flow concentration processes, and the vegetation fraction. In this study, an evidential reasoning approach based on Dempster-Shafer theory is proposed for mapping mountain torrent hazards in the Hexi Corridor. The frequent torrent disasters greatly impact the security of infrastructure and human safety. Many important national engineering projects pass through the corridor, such as highways, railways, and the West-to-East Gas Pipeline. The Hexi Corridor is an important part of the Silk Road Economic Belt and a crucial channel for westward development in China. Ran, Youhua Liu, Jinpeng Tian, Feng Wang, Dekai Mapping mountain torrent hazards in the Hexi Corridor using an evidential reasoning approach Also given is the cross-identification of stars in common with the astrometry ( Balaguer-Nunez et al. We mark the selection of probable members of NGC 1817, combining this photometric study with the previous astrometric analysis ( Balaguer-Nunez et al.
VizieR Online Data Catalog: ubvyH and J2000 coordinates for 7842 stars in an area of 65'x40' around NGC 1817.
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