Blazar的爆发携带着丰富的物理信息。凭借其较好的探测灵敏度和巡天观测模式，Fermi伽马射线望远镜为我们提供了高质量的、长达近十年的blazar的GeV伽马射线爆发的数据。尤其是Fermi望远镜最近探测到了最为剧烈和快速的blazar的伽马射线爆发，这些极端的爆发现象是研究相关物理的突破口。目前已有几种模型被提出来解释blazar的剧烈而快速的伽马射线爆发，但尚不能唯一确定这类大爆发的起源。我们将利用Fermi望远镜的公开数据来构建blazar的精细的伽马射线光变曲线，分析爆发态时观测量的统计特征（如爆发态峰值流量和爆发持续时间的分布等），与已有的爆发模型预言的统计特征进行对比分析，从而唯一得确认伽马射线爆发的起源。我们还将探索伽马射线爆发态时可观测量间是否存在有规律的演化行为；分能段构建光变曲线，分析爆发态时的观测量是否依赖光子能量，并分析不同能段爆发的时间延迟。

Blazar’s flare carries a wealth of physical information. Thanks to its good detection sensitivity and sky survey mode, the Fermi Gamma-Ray Telescope provides us with high-quality GeV gamma-ray data for nearly 10 years of blazar. In particular, the Fermi Gamma-Ray Telescope has detected the most violent and rapid blazar gamma-ray flares recently, and these extreme flares are breakthroughs in the study of related physics. At present, several models have been proposed to explain the violent and rapid gamma-ray flares of blazar, however the origin of such giant flares can not yet be uniquely identified. We will use the public data from the Fermi Gamma-Ray Telescope observations to construct refined gamma-ray light curves for blazar, and to analyze the statistical characteristics of the observations at the time of flares (e.g., the distribution of peak flux and flare duration). Through comparing these statistical characteristics with that the existing models predicted, we can determine the origin of flares uniquely. We will also explore whether there is a regular evolvement of the observables in gamma-ray flare states; and build light curves in different gamma-ray bands, to analyze whether the observations in flare states depend on photon energy. We will also analyze the time delays between flares in different gamma-ray bands.