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A Non-Extensive Statistical Physics View in the Spatiotemporal Properties of the 2003 (Mw6.2) Lefkada, Ionian Island Greece, Aftershock Sequence

机译:2003(Mw6.2)莱夫卡达,爱奥尼亚岛希腊,余震序列的时空特性的非广义统计物理视图

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Investigation of the spatiotemporal properties of the 2003 Lefkada seismic sequence is performed through non-extensive statistical physics. Information on highly accurate aftershock source parameters became feasible from the recordings of a portable digital seismological network that was installed and operated in the study area, during the evolution of the seismic sequence. Thus, the spatiotemporal distribution of aftershocks onto the main and neighboring fault segments was investigated in detail, enabling the recognition of four distinctive seismicity clusters separated by less active patches. The aftershock spatiotemporal properties are studied here, using the ideas of non-extensive statistical physics (NESP). The cumulative distribution functions of the inter-event times and the inter-event distances are presented using the data set in each seismicity cluster, and the analysis results in values for the statistical thermodynamic q_T and q_D parameters for each cluster, where q_T varies from 1.16 to 1.47 and q_D from 0.42 to 0.77 for the inter-event times and distances distributions, respectively. These values confirm the complexity and non-additivity of the spatiotemporal evolution of seismicity, and the applicability of the NESP approach in investigating aftershocks sequence. The temporal pattern is discussed using the closely connected to NESP approach of superstatistics, which is based on a superposition of ordinary local equilibrium statistical mechanics. The result indicates that the temporal evolution of the Lefkada aftershock sequence in clusters A, B and C is governed by very low number of degrees of freedom, while D is a less organized seismicity structure with a much higher number of degrees of freedom.
机译:通过非广泛的统计物理学方法对2003年莱夫卡达地震序列的时空特性进行了研究。在地震序列演变过程中,从便携式数字地震网络的记录中获得了关于高精度余震源参数的信息,该便携式数字地震网络已安装在研究区域并在研究区域中运行。因此,详细研究了余震在主断层段和邻近断层段上的时空分布,从而能够识别由活动性较弱的斑块分隔开的四个独特的地震活动群。余震时空特性在本文中使用非广义统计物理学(NESP)的思想进行了研究。使用每个地震活动度群集中的数据集来显示事件间时间和事件间距离的累积分布函数,并且分析得出每个群集的统计热力学q_T和q_D参数的值,其中q_T从1.16变化事件间隔时间和距离分布分别从0.42到0.77的1.47和q_D从0.42到0.77。这些值证实了地震活动的时空演变的复杂性和非可加性,以及NESP方法在研究余震序列中的适用性。使用与超级统计的NESP方法紧密联系的方法来讨论时间模式,该方法基于普通局部均衡统计机制的叠加。结果表明,星团A,B和C的莱夫卡达余震序列的时间演化受非常低的自由度支配,而D是组织性较差的地震活动结构,具有更高的自由度。

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