First comparison of wave observations from CoMP and AIA/SDO

TL;DR

This study compares wave observations from CoMP and AIA/SDO in the solar corona, revealing consistent signatures of transverse and longitudinal oscillations that contribute to understanding coronal dynamics and heating.

Contribution

It is the first direct comparison of wave signatures from CoMP and AIA/SDO in the same active region, linking on-disk and off-limb observations of coronal waves.

Findings

Transverse wave signatures observed with CoMP and AIA/SDO show similar phase speeds and periods.

Quasi-periodic intensity features travel along coronal loops with consistent properties.

Correlated wave features are identified across different instruments and observation angles.

Abstract

Waves have long been thought to contribute to the heating of the solar corona and the generation of the solar wind. Recent observations have demonstrated evidence of quasi-periodic longitudinal disturbances and ubiquitous transverse wave propagation in many different coronal environments. This paper investigates signatures of different types of oscillatory behaviour, both above the solar limb and on-disk, by comparing findings from the Coronal Multi-channel Polarimeter (CoMP) and the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory (SDO) for the same active region. We study both transverse and longitudinal motion by comparing and contrasting time-distance images of parallel and perpendicular cuts along/across active region fan loops. Comparisons between parallel space-time features in CoMP Doppler velocity and transverse oscillations in AIA images are made, together with space-time analysis of propagating quasi-periodic intensity features seen near the base of loops in AIA. Signatures of transverse motions are observed along the same magnetic structure using CoMP Doppler velocity (Vphase=600-750km/s, P=3-6mins) and in AIA/SDO above the limb (P=3-8mins). Quasi-periodic intensity features (Vphase=100-200km/s, P=6-11mins) also travel along the base of the same structure. On the disk, signatures of both transverse and longitudinal intensity features were observed by AIA; both show similar properties to signatures found along structures anchored in the same active region three days earlier above the limb. Correlated features are recovered by space-time analysis of neighbouring tracks over perpendicular distances of <2.6Mm.