And 1-day summaries for greater detail:
Spectrum Analyzer Mode:
Wideband Mode: (This is mostly irrelevant since little or no wideband data will be obtained in the Magnetospheric Survey--only occasional fill data)
Spectrum Analyzer Mode:
Wideband Mode: (This is mostly irrelevant since little or no wideband data will be obtained in the Survey--only occasional fill data and data which is automatically recorded with remote sensing recorded observations)
Record for ~150 minutes beginning at about 23:30 on day 126 (6 May) 1997 at a distance of ~ 21 Rj. This interval begins 2.44 Rj below the magnetic equator and ends when the spacecraft is about 2.49 Rj above (north) of the magnetic equator. Here is the location of Galileo at the center of this observation.
Spectrum Analyzer Mode:
Wideband Mode:
Playback Strategy:
Return LPW (Golay) wideband data at a rate of 2:1 by returning every other waveform snapshot for 105 minutes of the interval centered on the magnetic equator; return LPW Golay wideband data at a rate of 4:1 by returning every 4th waveform snapshot for the remaining 45 minutes of the interval at the highest latitudes at the beginning and end of the interval. This plan may be modified upon analysis of RTS data.
Record LPW for ~45 minutes beginning at about 15:35 on day 127 (7 May) 1997.
Spectrum Analyzer Mode:
Wideband Mode:
Playback Strategy:
Return LPW (Golay) wideband data at a rate of 2:1 by sending back every other waveform snapshot.