增生杂岩的构造解析，对研究俯冲带构造构造演化过程具有重要的意义。通过将其拆分为系列构造岩片，逐一研究其形成-就位时序，可为理解俯冲带构造演化过程提供支撑。然而对比现代活动俯冲带，古老造山带中增生楔精细生长序列研究稍显薄弱，制约了对增生型造山带生长过程及机理的理解。西准噶尔北缘塔尔巴哈台增生杂带分为南北两部分，南部额敏蛇绿岩带就位于晚石炭世，且自北向南存在数百万年尺度的变年轻生长序列；北部珠万托别混杂岩带被早石炭世岩体钉合，但其增生时序尚未得到解析。故塔尔巴哈台增生杂岩带南北两部分是否存在数十百万年的生长，北部珠万托别混杂带是否同样存在数百万年的生长，需进一步研究。. 本课题拟在珠万托别混杂带进行大比例尺构造填图、岩片形成-就位时序分析，从而还原不同时间尺度上塔尔巴哈台增生杂岩带生长时序，为探讨该地区晚古生代构造演化提供制约，也为理解古老增生型造山带生长过程及机理提供窗口。

The structural anatomy of accretionary complex is of great importance to the understanding of the evolutionary history of subduction tectonics. It can help to restore the subduction zone evolutionary history by structurally dividing the accretionary complex into tectonic slices and studying their individual formation – accretion time sequence. However, it is less focused for the accretion sequence anatomy of the ancient accretionary orogeny when it is compared with the modern subduction zone, which becomes a major obstacle for the understanding of the process and mechanism of accretionary type orogenic belt. The Northern West Junggar develops the Tarbagatay complex, which can be tectonically divided two major parts: the southern part, represented as the late Carboniferous accreted E’min ophiolite, which develops several million years’ southward younging; and the northern part, represented as the Zhuwantuobie complex, stitched by early Carboniferous plutons, of which the accretion sequence remains unclear. Thus it is important to figure out: 1. Is there a dozens of million years’ accretion sequence on the whole Tarbagatay accretionary complex, from the northern part Zhuwantuobie complex that is stitched by early Carboniferous pluton, to the southern part E’min ophiolite that is stitched by late Carboniferous dike? 2. Is there a several million years’ accretion sequence on the Zhuwantuobie complex, like the E’min ophiolite? . Thus, this study carry out large scale structural mapping, the formation – accretion sequence analyzing on the Zhuwantuobie complex of West Junggar, in order to add new constrains on late Paleozoic evolutionary history of this area, and helps to understand the process and mechanism on the growth of ancient accretionary type orogeny.