An inner boundary condition for solar wind models based on coronal density | Journal of Space Weather and Space Climate

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Fig. 2

Coronal electron density (blue, right axis) taken from the tomographical map of Figure 1c at Earth’s latitude, and solar wind velocity at 8 R_⊙ (black, left axis) gained from the density using the simple inverse relationship of equation (1). For this example, V_max = 480 km s⁻¹ and V_min = 220 km s⁻¹.

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