The failures of surface vertical wells (SVWs) for methane extraction during mining are known to be the main causes of the shortening of the highly efficient drainage periods of the SVWs. Therefore, in order to improve the stability of the SVWs, it is of great significance to accurately investigate the failure characteristics when SVWs are severely destroyed and can no longer extract methane. In this research, a physical simulation experiment was carried out for the purpose of investigating the most possible failure periods, as well as the highest possible failure locations and failure modes of SVWs. This study’s results showed that the displacements of the SVW were constantly changing under the influences of mining stress. After the mine working faces had past the SVWs by more than 157 m, the total displacements reached the maximum, and the SVWs were in the most possible failure periods. During those periods, failure positions of the SVWs are prone to occur at the interfaces between the hard and soft strata; within the thick rock layers; and within the thick-thin-thick strata combination. Among these, the SVWs may suffer from shear slippage at the interface of the hard-soft combined rock layers with relatively large thickness differences; the SVWs may suffer from horizontal shear at the interfaces of the hard-soft combined rock layers with small thickness differences; the SVWs within the thick rock layers may become destroyed by shear slippage actions; and the SVWs in the thick-thin-thick combined rock layers may become distorted by shearing at the interface between the rock layers or blocking within the intermediate thin rock. The results of this research study were verified through the field tests which were conducted in China’s Sihe Coal Mine.
Coronal Mass Ejections (CMEs) are important sources of Solar Proton Events (SPEs). Their speeds and source region locations have significant effects on the occurrence of SPEs. In this paper, all the halo CMEs observed in recent five years are statistically analyzed. The results show that the fast halo CMEs with small angular distances are more likely to produce SPEs, especially, those halo CMEs with a speed greater than 1200 km s?1 and an angular distance less than 60°. Three fast halo CMEs with no SPEs caused are elaborately studied. The results show that the ejection direction of the CME's main body and the variation of interplanetary magnetic field also have important impacts on the occurrence of SPEs. Consequently, in the practical daily space environment forecasts, an accurate forecast for SPEs must take various factors into account, such as the eruption speed, source region location, the main-body ejection direction of CMEs, and the interplanetary environment, etc. 相似文献
