Fig. 4
From: Sub-ion-gyro scale magnetic field compressions generated by the solar wind interaction with the moon
Energy time spectra of plasma particles obtained by MAP/PACE onboard Kaguya on January 1, 2008. a Electrons detected by ESA2 sensor (on zenith-looking panel), b electrons detected by ESA1 sensor (on nadir-looking panel), c ions detected by IEA sensor (on zenith-looking panel), d ions detected by IMA sensor (on nadir-looking panel), e magnitude and f directions of magnetic field measured by LMAG, g solar zenith angle of Kaguya, and h longitude and the latitude of Kaguya in SSE and ME coordinate systems