PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM LABEL_REVISION_NOTE = " 2004-08-25 S.McLaughlin Created 2005-02-10 S.McLaughlin Resolved liens from Oct 2004 thermal-vac review 2006-05-18 DI:S.McLaughlin Resolved liens from Apr 2006 peer review 2006-10-02 DI:S.McLaughlin Corrected FOV characteristics " OBJECT = INSTRUMENT INSTRUMENT_HOST_ID = "DIF" INSTRUMENT_ID = "MRI" OBJECT = INSTRUMENT_INFORMATION INSTRUMENT_NAME = " DEEP IMPACT MEDIUM RESOLUTION INSTRUMENT - VISIBLE CCD" INSTRUMENT_TYPE = "CCD CAMERA" INSTRUMENT_DESC = " Instrument Overview =================== The Medium Resolution Imager consisted of an f/17.5 Cassegrain telescope followed by a filter wheel feeding directly onto a CCD for direct, optical imaging. The MRI telescope was a classical Cassegrain design with the following parameters: Primary aperture : 12.0 cm diameter, round Primary focal ratio : 3.75 Secondary Obscuration : 6.6 cm diameter, round Secondary magnification : 4.75x (net Cassegrain focal length 210 cm) Back focal distance : 30.0 cm The filter wheel contained two clear apertures and eight filters. The filters included duplicates of some of the medium-band filters in the High Resolution Instrument, narrow-band filters that isolate OH, CN, and C2 as well as the green and violet continuum. These narrow-band filters were designed to match the Hale-Bopp filter sets used for ground-based programs since 1996. The longest wavelength filter was actually a long-pass filter that used the CCD response to define the long-wavelength cutoff at about 960 nanometers. The detector was a 1024 x 1024 split frame-transfer CCD with 21-micron-square pixels. The electronics allowed readout of centered sub-frames in multiples of 2, 64x64, 128x128, and so on, with or without rows of overscan. Transfer time, to move the two halves of the image from the exposing area to the two shielded areas, was about 5.2 milliseconds. There are readout amplifiers in each of the four quadrants. Readout time for a full frame was 1.8 seconds. Net pixel scale was 10 microradians/pixel (2 arcseconds/pixel). The MRI instrument in full-frame 1024 x 1024 mode had the following field-of-view characteristics: Pixel Size : 21 micrometers Pixel FOV : 10.0 microradians Instrument FOV : 10.0 milliradians or 0.587 degrees Surface Scale : 7 meters/pixel at 700 kilometers The three instruments on the flyby spacecraft, HRII, HRIV and MRI, were mounted on a separate instrument platform together with the star trackers. The three instruments were nominally co-aligned. For a detailed discussion of the instrument, see Hampton, et al. (2005) [HAMPTONETAL2005]. This instrument overview was provided by Dr. Michael A'Hearn, the principal investigator for the Deep Impact mission. Instrument Calibration ====================== The MRI instrument was calibrated by using in-flight data as well as pre-launch data taken during a thermal-vacuum test (TV4) performed in 2003. The calibration of the MRI instrument was discussed in the 'Deep Impact Instrument Calibration' paper by Klaasen, et al. (2006) [KLAASENETAL2006]. Flight Performance ================== The MRI instrument generally performed as expected during flight. " END_OBJECT = INSTRUMENT_INFORMATION OBJECT = INSTRUMENT_REFERENCE_INFO REFERENCE_KEY_ID = "HAMPTONETAL2005" END_OBJECT = INSTRUMENT_REFERENCE_INFO OBJECT = INSTRUMENT_REFERENCE_INFO REFERENCE_KEY_ID = "KLAASENETAL2006" END_OBJECT = INSTRUMENT_REFERENCE_INFO END_OBJECT = INSTRUMENT END