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Fig. 2
Color-coded range of the derived B1 AU (nT) as a function of the near-Sun CME magnetic field B0 at 10 R⊙ (abscissa) and of the power-law exponent αB of the radial CME-ICME falloff (ordinate). The color scale is saturated such that white and black areas lie outside the observed MC magnetic fields by WIND observations at L1.
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