Fig. 5

Probability distribution, ,
of the location angle (λ) as derived from the magnetic data of MCs
observed at 1 AU and fitted by the Lundquist model (Lepping et al. 1990). The data are grouped into a histogram having 10 bins
of |λ| and
is normalized so that the sum of the bins is unity. A least square fit of the
histogram with a straight line and a cosinus function are shown in black and blue,
respectively.
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