Mean shape of interplanetary shocks deduced from in situ observations and its relation with interplanetary CMEs

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Fig. 11

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a) Probability distributions for three sets of shocks (drawn as curves rather than histograms as in Fig. 4). b) Corresponding deduced shock shapes from Eqs. (15) and (16) with the apex distance normalized to 1 and ϕ_max = 35°.

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