Fig. 14
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Spatial distribution of EMLHB. Regions with EMLHB uncertainty < 5 × 10−5 cm−6 pc were also masked. The solid black line indicates the position of the ecliptic, and the two dashed lines represent a range of ±25° around it in ecliptic latitude where the solar wind density is expected to be high. The extent of the LHB under the assumption of ne = 4 × 10−3 cm−3 is also shown.
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