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So the new knowledge that we are gathering from this new data and new

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observations are going to help us understand the whole heliosphere, and

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also some processes even close to the Sun. For example, what I mentioned earlier,

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about the acceleration of particles. The fact that particles may be not as simple as

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going through a shock and accelerating particles.

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Maybe you have them accelerated in the sides of shocks or maybe in sheaths

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in coronal mass ejections. This knowledge we are gathering at the edge of the

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solar system probably will influence the edge but also other ionized matter.