Fig. 8
From: Sub-ion-gyro scale magnetic field compressions generated by the solar wind interaction with the moon
High time resolution magnetic field of a hot flow anomaly on August 5, 2008. a–d The magnitude and the \(x_{{SSE}}\), \(y_{{SSE}}\), \(z_{{SSE}}\) components of the magnetic field in SSE coordinates, e the azimuth and f the latitude angles observed by Kaguya at a sampling rate of 32 Hz. g Magnetic connection between Kaguya and the nightside surface of the moon