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Kenneth P. Klaasen Brian Carcich Gemma Carcich Edwin J. Grayzeck Stephanie Mclaughlin 《Space Science Reviews》2005,117(1-2):335-372
A comprehensive observational sequence using the Deep Impact (DI) spacecraft instruments (consisting of cameras with two different
focal lengths and an infrared spectrometer) will yield data that will permit characterization of the nucleus and coma of comet
Tempel 1, both before and after impact by the DI Impactor. Within the constraints of the mission system, the planned data
return has been optimized. A subset of the most valuable data is planned for return in near-real time to ensure that the DI
mission success criteria will be met even if the spacecraft should not survive the comet’s closest approach. The remaining
prime science data will be played back during the first day after the closest approach. The flight data set will include approach
observations spanning the 60 days prior to encounter, pre-impact data to characterize the comet at high resolution just prior
to impact, photos from the Impactor as it plunges toward the nucleus surface (including resolutions exceeding 1 m), sub-second
time sampling of the impact event itself from the Flyby spacecraft, monitoring of the crater formation process and ejecta
outflow for over 10 min after impact, observations of the interior of the fully formed crater at spatial resolutions down
to a few meters, and high-phase lookback observations of the nucleus and coma for 60 h after closest approach. An inflight
calibration data set to accurately characterize the instruments’ performance is also planned. A ground data processing pipeline
is under development at Cornell University that will efficiently convert the raw flight data files into calibrated images
and spectral maps as well as produce validated archival data sets for delivery to NASA’s Planetary Data System within 6 months
after the Earth receipt for use by researchers world-wide. 相似文献
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