Formation and Thermodynamic Evolution of plasmoids in active region jets
Sargam M. Mulay, Durgesh Tripathi, Helen Mason, Giulio Del Zanna,, Vasilis Archontis

TL;DR
This study investigates the temperature structure and evolution of plasmoids in active region jets using multi-wavelength EUV/UV and X-ray imaging, revealing their thermodynamic behavior and possible formation mechanisms.
Contribution
It provides a detailed analysis of the temperature and density evolution of plasmoids in active region jets, highlighting their formation via tearing-mode instability.
Findings
Plasmoids exhibit systematic brightness and temperature variations during propagation.
Footpoint plasmoids have higher DEM-weighted temperatures than spire plasmoids.
Electron densities of plasmoids are estimated to be in the range of 10^8 cm^-3.
Abstract
We have carried out a comprehensive study of the temperature structure of plasmoids, which successively occurred in recurrent active region jets. The multithermal plasmoids were seen to be travelling along the multi-threaded spire as well as at the footpoint region in the EUV/UV images recorded by the Atmospheric Imaging Assembly (AIA). The Differential Emission Measure (DEM) analysis was performed using EUV AIA images, and the high-temperature part of the DEM was constrained by combining X-ray images from the X-ray telescope (XRT/Hinode). We observed a systematic rise and fall in brightness, electron number densities and the peak temperatures of the spire plasmoid during its propagation along the jet. The plasmoids at the footpoint (FPs) (1.0-2.5 MK) and plasmoids at the spire (SPs) (1.0-2.24 MK) were found to have similar peak temperatures, whereas the FPs have higher DEM weighted…
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Taxonomy
TopicsIonosphere and magnetosphere dynamics · Atmospheric aerosols and clouds · Atmospheric chemistry and aerosols
