28 September 2020 to 2 October 2020
Pisa, Italy
Europe/Rome timezone

Launched in 2002, the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) was a NASA Small Explorer Mission designed to explore the basic physics of particle acceleration and explosive energy release in solar flares by making pioneering imaging spectroscopy observations of the X-ray and gamma-ray emissions of these energetic events. Decommissioned in October 2018, RHESSI covered more than a complete solar cycle in its 16-year lifetime and tremendously advanced the understanding of high energy phenomena at the Sun.

This workshop is the 19th in a series of workshops to explore current topics in high-energy in solar flare physics. It will have a format similar to previous workshops, with a balance of plenary sessions, invited and contributed talks, and working groups focused on specific topics.  The workshop will feature results from ongoing analysis and interpretation of archival RHESSI data, and will also emphasize coordinated observations of high-energy solar eruptive events using instruments/facilities such as EOVSA, NuSTAR, PSP, Fermi, and MinXSS.  It will also include sessions on preparing for future missions such as STIX/Solar Orbiter and FIERCE.

Starts
Ends
Europe/Rome
Pisa, Italy
Aula Magna
Building E, Polo Fibonacci Largo Pontecorvo, 3 Pisa
The call for abstracts is open
You can submit an abstract for reviewing.
Registration
Registration for this event is currently open.