“…The solar wind interacts directly with the Venusian ionosphere, forming an induced magnetosphere above the ionosphere (e.g., Phillips & McComas, ; Zhang et al, , ), and the bow shock and the magnetosheath are also formed in this interaction (e.g., Luhmann, ). Prior studies suggested that the Venusian magnetosheath is filled with strong magnetic field fluctuations, which can be convected from the upstream foreshock or can be locally generated (e.g., Du et al, ; Luhmann et al, ; Xiao et al, ). The magnetic field fluctuations play an important role in the transfer of momentum and energy in the space plasma environment of the planet (e.g., Guicking et al, ; Luhmann, ).…”