At Venus, the bow shock is driven chiefly by IMF intensity/Mach number and θbn, while the ion composition boundary is driven chiefly by solar EUV flux.
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Ranking the drivers of the Venusian bow shock and ion composition boundary locations
At Venus, the bow shock is driven chiefly by IMF intensity/Mach number and θbn, while the ion composition boundary is driven chiefly by solar EUV flux.