Fig. 7
From: Sub-ion-gyro scale magnetic field compressions generated by the solar wind interaction with the moon
Kaguya position and magnetic field vectors produced by a hot flow anomaly on 5 August 2008. The format is the same as in Fig. 2. Red bars represent directions of the 1-s averaged magnetic field vectors of the short-period magnetic enhancement at approximately its maximum intensity at 3:28:41, while green bars represent ambient magnetic field vectors plotted every 60 s during the period from 3:25 to 3:30