Unambiguous Evidence of Coronal Implosions During Solar Eruptions and Flares

TL;DR

This study provides clear observational evidence of coronal loop contractions during solar eruptions and flares, confirming the implosion conjecture and identifying two physical categories of implosion based on event properties.

Contribution

The paper presents four edge-on observed events demonstrating true coronal loop contractions, validating the implosion conjecture and distinguishing two types of implosion phenomena.

Findings

Confirmed the reality of coronal loop contractions during eruptions.

Identified two physical categories of implosion based on event characteristics.

Suggested suppression of implosions in heavily-mass-loaded filaments.

Abstract

In the implosion conjecture, coronal loops contract as the result of magnetic energy release in solar eruptions and flares. However, after almost two decades, observations of this phenomenon are still rare, and most of previous reports are plagued by projection effects so that loop contraction could be either true implosion or just a change in loop inclination. In this paper, to demonstrate the reality of loop contractions in the global coronal dynamics, we present four events with the continuously contracting loops in an almost edge-on geometry from the perspective of SDO/AIA, which are free from the ambiguity caused by the projection effects, also supplemented by contemporary observations from STEREO for examination. In the wider context of observations, simulations and theories, we argue that the implosion conjecture is valid in interpreting these events. Furthermore, distinct properties of the events allow us to identify two physical categories of implosion. One type demonstrates a rapid contraction at the beginning of the flare impulsive phase, as magnetic free energy is removed rapidly by a filament eruption. The other type, which has no visible eruption, shows a continuous loop shrinkage during the entire flare impulsive phase which we suggest manifests the ongoing conversion of magnetic free energy in a coronal volume. Corresponding scenarios are described, which can provide reasonable explanations for the observations. We also point out that implosions may be suppressed in cases when a heavily-mass-loaded filament is involved, possibly serving as an alternative account for their observational rarity.