On the Response of the Transition Region and the Corona to Rapid Excursions in the Chromosphere

• Published in: The Astrophysical journal 2024-08, Vol.970 (2), p.179
• Main Authors: Chaurasiya, Ravi, Bayanna, A. Raja, Louis, R. E., Pereira, T. M. D., Mathew, S. K.
• Format: Article
• Language: English
• Subjects: Chromosphere; Corona; H alpha line; Solar activity; Solar chromosphere; Solar chromospheric heating; Solar coronal heating; Solar limb; Solar observatories; Solar spicules; Solar transition region; Spectra; Spectral signatures; Spicules; Temperature spectra; The Sun; Trajectories; Upper atmosphere
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/1538-4357/ad50d5

Spicules are the thin hair/grass-like structures that are prominently observed at the chromospheric solar limb. It is believed that fibrils and rapid blueshifted and redshifted excursions (RBEs and RREs; collectively referred to as REs) correspond to on-disk counterparts of type I spicules and type II spicules, respectively. Our investigation focuses on observing the response of these REs alongside similar spectral features in the chromosphere, transition region (TR), and corona, utilizing space–time plots derived from coordinated observations from the Swedish 1 m Solar Telescope/H α , Interface Region Imaging Spectrograph (IRIS), and Solar Dynamics Observatory. Our analysis reveals upflowing REs, promptly reaching temperatures characteristic of the TR and corona, indicating a multithermal nature. Similarly, downflowing features exhibiting similar spectral signatures over the disk display plasma motion from the corona to chromospheric temperatures, demonstrating a multithermal nature. In addition to distinct upflows and downflows, we observe sequential upflow and downflow along the same path, depicting a distinctive parabolic trajectory in space–time plots of observations sampling TR and various coronal passbands. Similar to isolated upflows and downflows, these REs also exhibit a multithermal nature throughout their trajectory. Furthermore, our results reveal a more intricate motion of the REs in which both upflow and downflow coexist at the same spatial location. On a different note, our analysis, utilizing coordinated IRIS spectral observations, shows spatiotemporal redshifts/downflows in both the TR and chromosphere, suggesting that at least subsets of the strong redshifts/downflows observed in TR temperature spectra result from the return from the upper atmosphere flow of plasma in the form of bundles of spicules or features exhibiting similar spectra.