Simulations show that spherical solar-wind expansion drives radial growth of magnetic clouds, with the ratio of internal to propagation timescales controlling the effect, and turbulence leaving radial expansion coherent.
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The effects of expansion and turbulence on the interplanetary evolution of a magnetic cloud
Simulations show that spherical solar-wind expansion drives radial growth of magnetic clouds, with the ratio of internal to propagation timescales controlling the effect, and turbulence leaving radial expansion coherent.