Analytic modeling of recurrent Forbush decreases caused by corotating interaction regions
Analytic modeling of recurrent Forbush decreases caused by corotating interaction regions
复制标题
由共旋转相互作用区域引起的循环 Forbush 减少的分析模型
DOI:
10.1051/0004-6361/202140846
复制
发表时间:
2022
影响因子:
6.5
通讯作者:
M. Heber
中科院分区:
文献类型:
--
作者:
Vršnak;Dumbović ;M. Heber
ContextOn scales of days, the galactic cosmic ray (GCR) flux is affected by coronal mass ejections and corotating interaction regions (CIRs), causing so-called Forbush decreases and recurrent Forbush decreases (RFDs), respectively.AimsWe explain the properties and behavior of RFDs recorded at about 1 au that are caused by CIRs generated by solar wind high-speed streams (HSSs) that emanate from coronal holes.MethodsWe employed a convection-diffusion GCR propagation model based on the Fokker-Planck equation and applied it to solar wind and interplanetary magnetic field properties at 1 au.ResultsOur analysis shows that the only two effects that are relevant for a plausible overall explanation of the observations are the enhanced convection effect caused by the increased velocity of the HSS and the reduced diffusion effect caused by the enhanced magnetic field and its fluctuations within the CIR and HSS structure. These two effects that we considered in the model are sufficient to explain not only the main signatures of RFDs, but also the sometimes observed “over-recovery” and secondary dips in RFD profiles. The explanation in terms of the convection-diffusion GCR propagation hypothesis is tested by applying our model to the observations of a long-lived CIR that recurred over 27 rotations in 2007–2008.ConclusionsOur analysis demonstrates a very good match of the model results and observations.