SH004-03
High Resolution Observations of the Low Atmospheric Response to Small Heating Events in Active Regions

Monday, 7 December 2020: 07:16
Virtual
Paola Testa, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, Luc Rouppe van der Voort, University of Oslo, Oslo, Norway, Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States and Helle Bakke, Institute of Theoretical Astrophysics, University of Oslo, Oslo, Norway
Abstract:
We investigate the low atmospheric response to small heating events (nano/micro-flares) by analyzing coordinated active region observations with IRIS and SST, and also using the simultaneous SDO/AIA observations to study the coronal emission. The events we observe as intense brightenings in the chromosphere and transition region are clearly associated with heating of the overlying loops to high temperatures (5-10MK), as is clear from the strong Fe XVIII emission observed in the 94A SDO/AIA passband. Some of the chromospheric brightenings have been observed with the SST with the CRISP instrument in Ca II 8542 and H-alpha, as well as with the new CHROMIS instrument in Ca II K, which provides unprecedented resolution. We will present the rich spectral diagnostics offered by IRIS and SST for these events, including insights we obtained by applying a k-means clustering analysis to the SST and IRIS spectra during the heating events. Our observations will help provide more stringent constraints on the properties of non-thermal particles in nanoflares and microflares.