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On the evolution of a sub-C class flare: a showcase for the capabilities of the revamped Catania Solar Telescope View all abstracts by submitter

Paolo Romano   Submitted: 2021-11-18 00:36

Solar flares are occasionally responsible for severe Space Weather events, which can affect space-borne and ground-based infrastructures, endangering anthropic technological activities and even human health and safety. Thus, an essential activity in the framework of Space Weather monitoring is devoted to the observation of the activity level of the Sun. In this context, the acquisition system of the Catania Solar Telescope has been recently upgraded in order to improve its contribution to the European Space Agency (ESA) - Space Weather Service Network through the ESA Portal, which represents the main asset for Space Weather in Europe. Here, we describe the hardware and software upgrades of the Catania Solar Telescope and the main data products provided by this facility, which include full-disc images of the photosphere and chromosphere, together with a detailed characterization of the sunspot groups. As a showcase of the observational capabilities of the revamped Catania Solar Telescope, we report the analysis of a B5.4 class flare occurred on 2020 December 7, simultaneously observed by the IRIS and SDO satellites.

Authors: Paolo Romano, Salvo L. Guglielmino, Pierfrancesco Costa, Mariachiara Falco, Salvatore Buttaccio, Alessandro Costa, Eugenio Martinetti, Giovanni Occhipinti, Daniele Spadaro, Rita Ventura, Giuseppe E. Capuano, Francesca Zuccarello
Projects: None

Publication Status: Solar Physics (in press)
Last Modified: 2021-11-20 20:08
Go to main E-Print page  The Magnetic Origin of Solar Campfires  Direct evidence that twisted flux tube emergence creates solar active regions  Edit Entry  Download Preprint  Delete Entry 

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