Energetic Ions: The Elusive Component of Solar Flares
First Team Meeting, 1 - 5 February, 2016
Illustration: comparison of spherical (Highland) cow observation and theory (R Vainio)
Meeting schedule
Monday, 1 February
- Introduction to the Team; planning for the week (Alec MacKinnon)
- Gamma-ray lines: example of a well-observed flare (Paulo Simoes)
- Non-parametric inversion of a set of gamma-ray lines (Federico Benvenuto)
- Introduction to Fermi and the LAT (Melissa Pesce-Rollins)
Tuesday, 2 February
- Search for Doppler-shifted spectrum lines from energetic ion charge-exchange reactions (Hugh Hudson)
- Charge exchange reactions: theory (Luis Fernandez Menchero)
- Solar Energetic Particles (Christina Cohen)
- Theoretical modelling of SEP acceleration and transport (Rami Vainio)
Wednesday, 3 February
- Energetic Neutral Atoms (Christina Cohen)
- A well-observed flare (continued) (Säm Krucker)
- FLUKA calculations of fast ion secondaries and observable radiation (Alec MacKinnon)
- Solar flares observed by Fermi LAT (Melissa Pesce-Rollins)
Thursday, 4 February
- Radio conterparts of some Fermi LAT events (Nicole Vilmer)
- Selection of events and topics for further study
Friday, 5 February
- Team working on specific events and topics