BNS Magnetometer And Solar Detectors Data

Compressed magnetic field data from IMAP-3 through BNS-M. In the middle - the perigee crossing.
Solar detectors data. Area with zero signal corresponds to the part of the orbit where SC was in shade.
Expanded part of Fig.2. From this data one could get an idea about orientation quality: the curve must be a sine wave if orientation is good.
Fig.1 Fig.2 Fig.3