Abstract Details

Name: Krishna Prasad Sayamanthula
Affiliation: Aryabhatta Research Institute of Observational Sciences (ARIES)
Conference ID: ASI2024_1021
Title : Coronal signatures of transition region downflows within a sunspot
Authors and Co-Authors : S. Krishna Prasad1, C. J. Nelson2, M. Mathioudakis3, D. B. Jess3, and T. Van Doorsselaere4
Abstract Type : Oral
Abstract Category : Sun, Solar System, Exoplanets, and Astrobiology
Abstract : Recent observations have revealed that intermittent plasma downflows are commonly observed in sunspots. These flows can be observed either in the umbra or penumbra of a sunspot. The flow speeds are often supersonic, with the corresponding spectra displaying a steady redshifted component that appears as a separate new line. For this reason, these flows are often referred to as "dual flows". High-resolution observations suggest that these flows are colocated with the foot point of coronal loops. Although their origin is still unclear, they are usually explained either in terms of siphon flows or coronal rain. In this study, we analyse the spectroscopic data of a sunspot from IRIS along with the corresponding imaging data from SDO/AIA to study the observational characteristics of these downflows.