Hard X-Ray Imaging of Solar Flares

lt;p>Michele Piana is full professor of Numerical Analysis at the Dipartimento di Matematica of the Università di Genova, research associate at CNR - SPIN Genova and Principal Investigator of the Methods for Image and Data Analysis (MIDA) Group. He was Visiting Scholar at the Department of Mathematical Sciences at the University of Delaware, researcher at the Istituto Nazionale di Fisica della Materia (INFM), Associate Professor of Computer Science at the Dipartimento di Informatica of the Università di Verona. He spent visiting periods at the Brain Research Unit, Low Temperature Laboratory, Helsinki University of Technology; Department of Physics and Astronomy, University of Glasgow; NASA Goddard Space Flight Center; and Institute for Data Science, Fachhochschule Nordwestschweiz. He has authored and co-authored more than 100 papers in refereed journals on solar physics, medical imaging, computational neuroscience, and applied mathematics. He has been a member of the Data Analysis Team of the NASA RHESSI mission and is currently co-Investigator for STIX on the Solar Orbiter and HXI on ASO-S. He has been Unit Coordinator for the FLARECAST project in Horizon 2020 and Coordinator of the HESPE project in FP7. He has been Deputy Rector for International Affairs and Deputy Rector for Research and Technological Transfer at the Università di Genova. He is currently Scientific Director of the Life Science Computational Laboratory, jointly established by the Università di Genova and the Ospedale Policlinico San Martino IRCCS Genova.

Brian Dennis has been actively involved in designing, building, and operating X-ray and gamma-ray spectrometers and imaging spectrometers during his over 50-year career as an astrophysicist at NASA's Goddard Space Flight Center. These include spectrometers on the 5th and 8th Orbiting Solar Observatories in the 1960s and `70s and on the Solar Maximum Mission in the 1980's, and the Ramaty High Energy Solar Spectroscopic Imager (RHESSI) from 2002 to 2018.  He is the RHESSI Mission Scientist and lead coinvestigator at Goddard, and has participated in this mission from the development of the original concept in the 1990s through to the final archiving of the data that is currently in progress. He is also an unfunded co-investigator for STIX on the Solar Orbiter. He is the author or co-author of over 200 refereed papers on these instruments and on the scientific analysis of observations made with them.

Gordon Emslie is a Professor of Physics & Astronomy at Western Kentucky University, having previously held a variety of positions at The University of Alabama in Huntsville and Oklahoma State University.  With over 200 refereed articles published, his research focuses on mechanisms for energy release and transport in solar eruptive events, with particular emphasis on developing models that are driven by the observed properties of the high-energy radiation produced during the energy release. He was a co-Investigator on the NASA RHESSI mission.

Anna Maria Massone is Associate Professor of Numerical Analysis at the Dipartimento di Matematica, Università di Genova and Research Associate at CNR - SPIN Genova. She has been researcher at CNR - SPIN and at the Istituto Nazionale di Fisica della Materia (INFM), and Assistante Diplômée at the Université de Lausanne. She spent visiting periods at the Institut für Data Science, Fachhochschule Nordwestschweiz, Trinity College, University of Dublin, Institut für Kernphysik, Universitaet Mainz, Department of Physics and Astronomy, University of Glasgow, Low Temperature Laboratory, Brain Research Unit, Helsinki University of Technology, Helsinki, NASA Goddard Space Flight Center, Greenbelt (MD), USA, and Leibniz-Institut für Astrophysik Potsdam. She has been Honorary Research Associate at the School of Physics and Astronomy, University of Glasgow. She ha

1. Hard X-ray Emission in Solar Flares.- 2. X-Ray Imaging Methods.- 3. RHESSI and STIX.- 4. Image Reconstruction Methods.- 5. Count-based Imaging Methods.- 6. Visibility-based Imaging Methods.- 7. Application to Solar Flares.- 8. Future Possibilities.