Effects of flares on solar high-degree helioseismic acoustic mode amplitudes

TL;DR

This study investigates whether solar flares excite acoustic modes by analyzing mode amplitudes around flare events, finding no significant amplification beyond 10% uncertainty, and highlighting the influence of magnetic fields.

Contribution

It provides the first detailed analysis of flare impacts on solar acoustic mode amplitudes using ring-diagram analysis across multiple flare sizes.

Findings

No significant mode amplitude amplification detected during flares.

Magnetic field effects are significant in mode amplitude variations.

Analysis across different flare intensities shows consistent results.

Abstract

Several attempts have been made to observe whether solar flares excite acoustic modes since Charles Wolff suggested this possibility almost fifty years ago. We look for the impact of flares on the amplitude of solar acoustic modes and other effects that are also affecting the mode amplitude. Solar acoustic mode amplitudes are known to be sensitive to magnetic fields. As flares usually occur in the presence of strong magnetic fields and most likely are the by-product of magnetic reconnection, we show how the magnetic field in and around the flaring region affects the mode amplitude. The mode amplitudes were obtained using ring-diagram analysis, which was first applied to a single event, the largest flare in the space age (the `Halloween Flare', SOL2003-10-28T11:00), using MDI data. Then, using HMI data, the analysis was applied to the regions corresponding to the flares observed during the high activity phase of cycle 24 and that fall into two groups. These two groups consist of small (10-60 erg/cm^2/s) and large (>1200 erg/cm^2/s) peak-flux flares, based on the Heliophysics Event Knowledgebase (HEK). The first set is used as a comparison to the results of the strong flares in the second set. After applying several corrections in order to take into account several sources of bias, we did not find any amplification in the inferred mode amplitude due to flaring activity larger than a 10% uncertainty.