An Analytical Diffusion-Expansion Model for Forbush Decreases Caused by Flux Ropes
Mateja Dumbovi\'c, Bernd Heber, Bojan Vr\v{s}nak, Manuela Temmer and, Anamarija Kirin

TL;DR
This paper introduces an analytical model for Forbush decreases caused by flux ropes, incorporating CME expansion and diffusion, and demonstrates its effectiveness through a case study matching observed data.
Contribution
The paper presents a new diffusion-expansion model for Forbush decreases that accounts for CME flux rope evolution and validates it with observational data.
Findings
Model qualitatively agrees with observations
Quantitative fit depends on diffusion coefficient and expansion mode
Diffusion coefficient aligns with expected physical values
Abstract
We present an analytical diffusion-expansion Forbush decrease (FD) model ForbMod which is based on the widely used approach of the initially empty, closed magnetic structure (i.e. flux rope) which fills up slowly with particles by perpendicular diffusion. The model is restricted to explain only the depression caused by the magnetic structure of the interplanetary coronal mass ejection (ICME). We use remote CME observations and a 3D reconstruction method (the Graduated Cylindrical Shell method) to constrain initial boundary conditions of the FD model and take into account CME evolutionary properties by incorporating flux rope expansion. Several flux rope expansion modes are considered, which can lead to different FD characteristics. In general, the model is qualitatively in agreement with observations, whereas quantitative agreement depends on the diffusion coefficient and the expansion…
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Taxonomy
TopicsMetallurgy and Material Forming · Fatigue and fracture mechanics
