Energetics of small electron acceleration episodes in the solar corona from radio noise storm observations

TL;DR

This study uses radio observations from GMRT and NRH to analyze small-scale electron acceleration events in the solar corona, revealing their energy contributions and implications for coronal heating.

Contribution

It provides the first detailed quantification of the energetics of small electron acceleration episodes in the solar corona using combined radio data.

Findings

Electrons involved carry $10^{21}$ to $10^{24}$ erg/s.

Energy in electrons per burst ranges from $10^{20}$ to $10^{23}$ ergs.

Results support the role of small-scale events in coronal heating.

Abstract

Observations of radio noise storms can act as sensitive probes of nonthermal electrons produced in small acceleration events in the solar corona. We use data from noise storm episodes observed jointly by the Giant Metrewave Radio Telescope (GMRT) and the Nancay Radioheliograph (NRH) to study characteristics of the nonthermal electrons involved in the emission. We find that the electrons carry $10^{21}$ to $10^{24}$ erg/s, and that the energy contained in the electrons producing a representative noise storm burst ranges from $10^{20}$ to $10^{23}$ ergs. These results are a direct probe of the energetics involved in ubiquitous, small-scale electron acceleration episodes in the corona, and could be relevant to a nanoflare-like scenario for coronal heating.