The Relation between Type III Radio Storms and CIR Energetic Particles

TL;DR

This study investigates the relationship between type III radio storms and energetic particles in corotating interaction regions, revealing that storms are associated with significantly higher particle fluxes and fluences.

Contribution

It provides the first comparative analysis of particle fluxes in CIRs with and without type III radio storms, highlighting the impact of storms on particle intensities.

Findings

Storm-associated CIRs have about 6 times higher proton fluence.

Storm-associated CIRs have about 8 times higher electron fluence.

Case studies show higher particle fluxes during storm events.

Abstract

We report on a study that compares energetic particle fluxes in corotating interaction regions (CIRs) associated with type III radio storm with those in nonstorm CIRs. In a case study, we compare the CIR particle events on 2010October 21 and 2005 November 2. The two events have similar solar and solar wind circumstances, except that the former is associated with a type III radio storm and has a higher CIR particle flux and fluence. We also perform a statistical study, which shows that the proton and electron fluences are higher in the storm associated CIRs by factor of about 6 and 8, respectively than those in the storm-free CIRs.