磁化“冠层”模型中的相关耀斑
Correlated flares in models of a magnetized "canopy"
摘要：
本文用Lu-Hamilton模型研究了磁化太阳大气的临界行为。主要的新颖之处在于，它的驱动是通过源进行扩散。这模仿了虚拟湍流基底迫使系统的效果。该系统表现出幂律统计不仅在耀斑的大小，而且在等待时间的分布。
英文摘要：
A model of the Lu-Hamilton kind is applied to the study of critical behavior of the magnetized solar atmosphere. The main novelty is that its driving is done via sources undergoing a diffusion. This mimics the effect of a virtual turbulent substrate forcing the system. The system exhibits power-law statistics not only in the size of the flares, but also in the distribution of the waiting times.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
