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MISSION PLAN - PDS Small Bodies Node

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Several imaging calibration activities will be performed on approach to the comet and<br />

after comet flyby. These activities are required to ensure proper performance from the<br />

camera and interpretability of the images acquired during encounter. Table 6.2-2<br />

summarizes the required calibration activities during the encounter phase.<br />

Table 6.2-2 Encounter Imaging Calibrations<br />

Time<br />

(days) Image Description<br />

no. of<br />

images<br />

bits /<br />

pixel<br />

no. of<br />

filters Comments<br />

E-60 Mini cal sequence 7 16 7 windowed about center (100x100?)<br />

Mirror pointing, align &<br />

sensitivity cal<br />

20 16 1<br />

(nav)<br />

pattern matched, windowed<br />

(10x10), nominal attitude, tight<br />

deadband<br />

E ±30<br />

1 Standard solar analog<br />

1 Flux standard (star<br />

TBD)<br />

28 /ea 16 7 /ea 4 exp / 7 filters, windowed (15x15),<br />

yaw turn, mirror, tight deadband<br />

Zero exposure 3 16 1 windowed (20x20), determine<br />

camera bias (~400 DN).<br />

E-30, ±15 Photocal w/ lamp ‘on’ 21 16, 8 7 3 exposures / image, windowed<br />

6.2.3 CIDA and DFMI Encounter Experiments<br />

At E-5 hours, communications will be continuous and CIDA and DFMI data included in<br />

the telemetry to Earth. It is after this time, that most, if not all, dust related activity is<br />

expected to occur. This configuration will continue through to approximately E-3<br />

minutes at which time the telemetry link is interrupted if the roll maneuver is required.<br />

Data from CIDA events will be compressed and stored on board. Any free memory left<br />

from the encounter period will be used for imaging after the primary encounter period.<br />

6.2.4 Delivery Accuracy and Science Implications<br />

If navigation targeting is perfect, Wild-2 will be located at z=150 km, y=0 km and x=0<br />

km in the spacecraft fixed coordinate system at the closest approach to the comet. Table<br />

6.2-3, however, shows the potential delivery error after the E-18 h and E-6 h TCMs.<br />

Remember that the E-6 h TCM will be performed only in the event of an anomaly.<br />

However, the knowledge improvement will be used to initialize the nucleus tracking<br />

algorithm and to update the start of the encounter sequence block, if necessary, thus<br />

keeping the navigation delivery in line with the spacecraft and sequencing capabilities.<br />

Table 6.2-3 Encounter Delivery Accuracy (1-sigma)<br />

TCM Cross-track (km) Time-of-Flight (sec)<br />

E-18 h 10 29<br />

E-6 h 7 29<br />

77

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