Table 1
Comparisons of the status of solar wind plasma and IMF and the Venusian magnetosphere before, during and after the ICME.
| Time | IMF (nT) | Pdyn (nPa) | Mf | Barrier Bmax (nT) | BS Loc. (RV) | IMB Loc. (RV) |
|---|---|---|---|---|---|---|
| 30 min (before ICME) | 8.68 | 2.66 | 6.07 | 90.36 | 1.33 | 1.107 |
| 39 min (ICME shock) | 18.60 | 2.66 | 5.31 | 117.23 | 1.21 | 1.092 |
| 42 min (during ICME) | 18.83 | 11.55 | 4.29 | 177.47 | 1.36 | 1.115 |
| 158 min (during ICME) | 23.77 | 14.59 | 4.48 | 203.58 | 1.34 | 1.140 |
Notes. The columns from left to right represent: Time, IMF strength, solar wind dynamic pressure (Pdyn), fast magnetosonic Mach number (Mf), maximum magnetic field strength in the magnetic barrier (Barrier Bmax), bow shock location (BS Loc.), and induced magnetosphere boundary location (IMB Loc.), respectively.
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