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Fig. 2

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The evolution of the PUI distribution with increasing heliocentric distance for negligible velocity diffusion. As in Fig. 1 the normalized distribution ℱ is shown at the given heliocentric distances vs. normalized speed with w = U. With increasing heliocentric distance the initial (delta-)distribution is more strongly broadening towards lower velocities for magnetic cooling (right panel) as compared to adiabatic cooling (left panel).

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