摘要: Geomagnetic substorm is an essential process that releases plasma and energy from the magnetotail to the inner magnetosphere and high latitude ionosphere. In this study, we investigate the substorms with different time durations based on the SME index during the years 1982-2012. Our results demonstrate that substorms with longer durations often occur during solar maximum years and from May to July, likely due to the higher polar ionospheric conductivity and more sunward geomagnetic pole directions during summer in the northern hemisphere. Additionally, longer substorms more frequently occur under stronger, longer-lasting southward IMF and are accompanied by slower solar winds, suggesting that extended magnetic reconnection is required to drive longer substorms. Substorm durations are not significantly related to the minimum SML index, but longer substorms usually have higher SMU and continuous rising PC indices. The SME indices of long-duration substorms show a bimodal MLT distribution located near midnight and dusk after substorm onset, with the peak originally at midnight moving eastward to the morning side during the late recovery phase. Longer duration substorms have a stronger effect on the overall ring current at all the MLT sectors except dawnside. Our results provide new insights into the development process and influencing factors of substorms from the expansion to recovery phases.