![]() ![]() Organization of plasma and magnetic field structures in the solar atmosphere As ADAHELI Associated Scientist, I have been also involved in the scientific definition of the mission and contributed both to the design of Ground Segment and to the definition of observation strategies. In this context, I am involved in the study of the structures associated with convective motion of plasma and I have actively participated in: several projects funded within the FP7 and H2020 frameworks (EST, SOLARNET, GREST, PRE-EST, SOLARNET2 and ESCAPE) the ASI (Italian Space Agency) feasibility study for the ADAHELI satellite and several PRIN (Italian National Research Grants) projects financed by MIUR or INAF. Such movements organize the topology of the field from the photospheric to the coronal layers determining many of the physical properties of the solar atmosphere. The solar magnetic fields are produced and often organized by the motions of the solar plasma. The dynamics of the solar surface and the interaction with the magnetic structures control the external structure of the solar atmosphere, and more generally the entire heliosphere. In the following, I list some research interests of mine and the activities I personally undertook.ĭynamics of the lower solar atmosphere (photosphere and chromosphere) My scientific activity is testified by > 100 entries in the ORCID database (iD: 0000-0003-2500-5054) or SAO/NASA Astrophysics Data System (ADS), the 77 entries in the Scopus database and by the numerous congress and meeting participations. ![]()
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