Multi-Instrument Observations and Tracking of a Coronal Mass Ejection Front From Low to Middle Corona

TL;DR

This study combines multi-instrument solar observations and advanced automated tracking to analyze the evolving shape and dynamics of a CME from the low to middle corona, providing new insights into EUV wave-CME relations.

Contribution

It introduces an updated multi-instrument tracking method for CMEs, enabling detailed analysis of their shape and kinematics across different solar regions.

Findings

Confirmed the connection between EUV waves and CMEs

Provided detailed observational insights into EUV wave-shock-CME relations

Enhanced tracking capabilities for CME features beyond the leading edge

Abstract

The shape and dynamics of coronal mass ejections (CMEs) vary significantly based on the instrument and wavelength used. This has led to significant debate about the proper definitions of CME/shock fronts, pile-up/compression regions, and cores observations in projection in optically thin vs. optically thick emission. Here we present an observational analysis of the evolving shape and kinematics of a large-scale CME that occurred on May 7, 2021 on the eastern limb of the Sun as seen from 1 au. The eruption was observed continuously, consecutively by the Atmospheric Imaging Assembly (AIA) telescope suite on the Solar Dynamics Observatory (SDO), the ground-based COronal Solar Magnetism Observatory (COSMO) K-coronagraph (K-Cor) on Mauna Loa, and the C2 and C3 telescopes of the Large Angle Solar Coronagraph (LASCO) on the Solar and Heliospheric Observatory (SoHO). We apply the updated multi-instument version of the recently developed Wavetrack Python suite for automated detection and tracking of coronal eruptive features to evaluate and compare the evolving shape of the CME front as it propagated from the solar surface out to 20 solar radii. Our tool allows tracking features beyond just the leading edge and is an important step towards semi-automatic manufacturing of training sets for training data-driven image segmentation models for solar imaging. Our findings confirm the expected strong connection between EUV waves and CMEs. Our novel, detailed analysis sheds observational light on the details of EUV wave-shock-CME relations that is lacking for the gap region between the low and middle corona.