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Abstract
We statistically investigate the spectral scalings of magnetic fluctuations at the upstream and downstream regions near the Venusian bow shock and perform a differentiation by shock geometry. Based on the Venus Express data, 115 quasi-parallel (
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Details
1 Harbin Institute of Technology, Shenzhen, China (GRID:grid.19373.3f) (ISNI:0000 0001 0193 3564)
2 University of Science and Technology of China, CAS Key Laboratory of Geospace Environment, Hefei, China (GRID:grid.59053.3a) (ISNI:0000000121679639)
3 Harbin Institute of Technology, Shenzhen, China (GRID:grid.19373.3f) (ISNI:0000 0001 0193 3564); Austrian Academy of Sciences, Space Research Institute, Graz, Austria (GRID:grid.4299.6) (ISNI:0000 0001 2169 3852)