Group Leader: Albert Shih
Co-Leader: Alec MacKinnon
The Presentations
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We will focus on what RHESSI and other instruments can tell us about accelerated ions and relativistic electrons, primarily using gamma-ray observations. We will also discuss other types of observations (e.g., neutrons or ENAs) that may provide new avenues of investigation. Participants’ interests will shape the group; likely topics include:
- the role of energetic ions in the flare process
- relative elemental abundances in the various populations
- diagnostics of deep-atmosphere conditions
- the relationship between accelerated ions and electrons
- the contribution of pion-decay products to high-energy emission
- the connection between energetic particles in flares and CMEs
Working Group 3 Draft Schedule (subject to change)
Google calendar: View in browser or import it into your favorite calendar software with this XML Calendar file (or iCal).
Figure: An image of the WG 3 schedule. Use the google calendar links to access the live calendar.
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