Pavel Trávníček

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We present a comparison between WIND/SWE observations [Kasper et al., 2006] of β p and T ⊥p /T p (where β p is the proton parallel beta and T ⊥p and T p are the perpendicular and parallel proton temperatures, respectively; here parallel and perpendicular indicate directions with respect to the ambient magnetic field) and predictions of the Vlasov linear(More)
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