 Fig.1
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 Fig.2
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 Fig.3
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- Fig.1
- Compressed magnetic field data from IMAP-3 through BNS-M. In the middle - the perigee crossing.
- Fig.2
- Solar detectors data. Area with zero signal corresponds to the part of the orbit where SC was in shade.
- Fig.3
- 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