Open Access

Table A.3

Table containing information regarding the dual-spacecraft bow shock crossings where one spacecraft was located over a region of strong crustal fields, and one spacecraft over a region of weak crustal fields.

Event number dHiɡhCF [RM] dLowCF [RM] dHiɡhCF-dLowCF [RM] scHiɡhCF t [Min] MA Pdyn [nPa] EUV [mWm−2
7 -0.113 0.163 -0.275 mex 3.1 3.4 0.43 21.1
26 -0.095 0.017 -0.112 mex 4.0 1.8 0.92 19.7
30 0.137 0.238 -0.101 mex 18.7 1.3 2.47 19.6
41 0.173 0.049 0.123 mav 1.9 6.4 1.13 27.4
51 0.085 0.109 -0.023 mex 4.9 2.7 0.80 27.4
74 0.220 0.175 0.044 mav 18.5 1.9 1.52 27.7
83 -0.036 -0.141 0.105 mav 7.6 10.3 0.38 27.8
91 0.020 0.173 -0.153 mav 4.5 4.2 0.46 27.9
113 0.159 -0.215 0.374 mex 7.0 3.9 0.32 22.4
144 0.045 0.272 -0.228 mav 9.5 4.1 0.45 26.9
176 0.104 0.031 0.072 mav 15.0 3.2 0.36 26.3

Mean 0.063 0.079 -0.016 8.6

1σ 0.110 0.152 0.186

Notes. The first column shows event ID. The second and third columns show the distance from the bow shock model to the observed bow shock crossing by the spacecraft over strong and weak crustal field region, respectively. The fourth column shows the difference between these two distances. The fifth column shows which spacecraft crossed the bow shock over a region of strong crustal fields. The sixth column shows the time difference between the crossings. The seventh to ninth column shows upstream values of Alfvénic Mach number, dynamic pressure, and solar EUV, respectively. At the bottom two rows the mean and one standard deviation for the distances, and for the difference, is given.

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