- 5.10.1 What is the temporal variability of 3D thermal particle distributions?
- 5.10.2 How are proton and helium temperatures related to their relative drift, is there any evidence for resonant heating?
- 5.10.3 How common are proton beams, where do they come from and what impact do they have on ambient conditions (wave generation, heating)?
- 5.10.4 Identify and characterise the various forms of free energy in the particle distribution functions
- 5.10.5 Fully characterise the radial and latitudinal variability of 3D thermal particle distributions under different solar wind conditions
- 5.10.6 Electron halo population
- 5.10.7 How do the combined electron strahl and composition signatures vary across reconnecting solar wind current sheets?