So the new knowledge that we are gathering from this new data and new
observations are going to help us understand the whole heliosphere, and
also some processes even close to the Sun. For example, what I mentioned earlier,
about the acceleration of particles. The fact that particles may be not as simple as
going through a shock and accelerating particles.
Maybe you have them accelerated in the sides of shocks or maybe in sheaths
in coronal mass ejections. This knowledge we are gathering at the edge of the
solar system probably will influence the edge but also other ionized matter.