The identified bow shock crossings based on Venus Express observations
<div>Bow shock locations and upstream parameters observed by Venus Express.</div> <div> </div> <div>The columns are structured as follows:</div> <div> 1: time of bow shock crossings dd-mmm-yyyy HH:MM:SS</div> <div> 2: X-VSE [Rv]</div> <div> 3: Y-VSE [Rv]</div> <div> 4: Z-VSE [Rv]</div> <div>5: Solar wind magnetosonic Mach number</div> <div> 6: EUV [mW/m^2]</div> <div> 7: IMF Bx in VSE [nT]</div> <div>8: IMF By in VSE [nT]</div> <div> 9: IMF intensity |B| [nT]</div> <div> 10: IMF cone angle [degree]</div> <div>11: Solar wind dynamic pressure [nPa]</div> <div>12: The angle between the IMF and the shock normal, thetaBn [degree]</div> <div> </div> <div>Please contact xuqi01@nssc.ac.cn if you have questions.</div>
ShareScore
36/100
Overall dataset sharing score
Score breakdown
These five areas show where the dataset supports — or may limit — practical reuse.
- Stewardship
- 4
- Harmonization
- 4
- Access
- 20
- Reuse readiness
- 8
- Engagement
- 0