Quantifying the latitudinal representivity of in situ solar wind observations | Journal of Space Weather and Space Climate

Topical Issue - Space Weather research in the Digital Age and across the full data lifecycle

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Fig. 6

V₀−V_θ, solar wind speed difference between the equator and other latitudes, as a function of solar cycle phase and latitude. Left: the median of V₀−V_θ. Centre: the inter-quartile range of V₀−V_θ. Right: the 5–95-percentile range of V₀−V_θ.

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