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Fig. 9

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Parameter correlation lines, shown pairwise for the polar data subsets illustrated in Fig. 1, with reduced-χ2(λ) shown in Fig. 7. The small gray cross with error bars is the solution found by Witte (2004). The large black cross marks the LIC flow parameters found from analysis of interstellar absorption lines by Redfield & Linsky (2008), the black line is the acceptable parameter line obtained from IBEX by Bzowski et al. (2012), with the dark spot marking the best solution. In addition to the correlation lines from the polar arcs (north NP and south SP), parameter correlation lines from the fit to the three CP scans together are shown. The color dots mark the best-fit parameter sets found for individual arcs.

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