Data Set Overview  :   This data set contains Calibrated data taken by New Horizons  Multispectral Visible Imaging Camera  instrument during the PLUTO mission phase.   MVIC is a visible and near-infrared imager. MVIC comprises seven  separate CCD two-dimensional arrays; all rows are 5024 pixels across  with twelve pixels at either end of each row optically inactive. The  single Pan Frame array is a panchromatic frame-transfer imager, 5024x128 pixels, that typically takes multiple frames in each observation. The  common Pan Frame data product is an image cube in three dimensions:  spatial; spatial; image frame, equivalent to time. Of the remaining six  arrays, 5024x32 pixels each, two are panchromatic (unfiltered), and the  remaining four are under filters and called the color arrays:  Near-InfraRed (NIR); methane (CH4); Red; Blue. All six are operated in  Time-Delay Integration (TDI) mode; the TDI arrays are in some ways  similar to line cameras. In TDI mode, the spacecraft and MVIC boresight  are scanned across the target at a rate that matches the charge transfer clock rate across the rows of the CCDs. Ideally the rates are matched,  so as the charges are read by the analog-to-digital converter off the  last line of the array, each pixel reading is near-proportional to the  brightness of the same piece of the target as its image moved across the array, accumulating charge on each row. In TDI mode it is the product of the per-row charge clock rate and the duration of the observation that  determines the number of rows each the image, and the image can be  arbitrarily long; the number of rows (32) in each array is not relevant  in determining the size of the image. The common data product for each  of the TDI arrays is a 2-D image, of arbitrary length as noted earlier.   During the Pluto Charon Encounter mission phase starting in January,  2015, there were several sub-phases: three Approach sub-phases, (AP1,  AP2 and AP3); a CORE sequence for the Pluto flyby on 14.July, 2015  (Day Of Year 195), sometimes also referred to as NEP (Near-Encounter  Phase); three Departure sub-phases (DP1, DP2, DP3); a Transition  sub-phase ending in late October, 2016 and closing out the Pluto  Encounter mission phase. For this final Ralph-MVIC delivery for the  Pluto mission phase, this data set includes the Approach data plus  plus all CORE and Departure sequences' data, including observations of  a low-resolution Pluto ring search taken in November, 2015, and  finally Transition sequence data covering functional tests and star  calibrations performed in mid-2016.   On Approach during April, May and June of 2015, MVIC operations  included the following: functional tests; full color observations of  the Pluto, Charon and the other Plutonian satellites; Critical and  Non-critical Optical Navication (OpNav or NAV) observations. The  color observations were grouped over several 6-day periods to obtain a  full rotation of Pluto and Charon.   This dataset includes the first PC_VISUV_MAP for MVIC at about 19 days  before encounter, a color TDI observation looking for changes in color  and composition over multiple rotations, to meet the goal of  understanding the time variability of Pluto's surface. These  observations were repeated daily over that week leading up to  encounter. From the day of encounter, this data set includes data from  three CORE observations: (1) Pluto/Charon color map (PC_MULTI_MAP)  about a day before the Time of Closest Approach (P-1d); (2) Pluto and  Charon color scan at P-5h (PC_COLOR_1); (3) Nix color scan  (N_COLOR_2).   The PC_MULTI_MAP observation, the last one of which is included in  this dataset, met multiple goals including imaging for color and  surface composition maps of the Pluto and Charon hemispheres, Pluto  and Charon phase integrals with resolved whole-disk images near 15  degrees, and imaging Pluto hazes on approach. Secondary goals are  Pluto and Charon color high and low phase imaging to enable  integrating over wavelength to determine the bolometric Bond albedo,  and also to investigate the surface microphysics of Pluto and Charon,  studying compositional and textural stratification in the surface as a  function of terrain type. The N_COLOR series provided Nix  high-resolution resolved color images.   Every observation provided in this data set was taken as a part of a  particular sequence. A list of these sequences has been provided in  file DOCUMENT/SEQ_MVIC_PLUTO.TAB.  N.B. Some sequences provided may have no corresponding observations.   For a list of observations, refer to the data set index table. This  is typically INDEX.TAB initially in the INDEX/ area of the data set.  There is also a file SLIMINDX.TAB in INDEX/ that summarizes key  information relevant to each observation, including which sequence  was in effect and what target was likely intended for the  observation.    Version  :   This is VERSION 3.0 of this data set.   The TARGET_NAME values were expanded and made more consistent across  all instruments with version 3.0 of the data set.   General statement about data set versions after V1.0  ----------------------------------------------------  The pipeline (see Processing below) was re-run on these data for each  version since the first (V1.0). That will typically change only the  FITS headers but not the FITS data of raw data sets. In some cases  this may change the calibration because the calculated geometry of an  observation has changed. See data set version-specific sections below  for significant exceptions to this general statement, i.e. changes to  pipeline processing, calibration processing, and data delivered.   An all-instrument Calibration Campaign occurred in July 2016. For all  instruments, calibrations were updated as of April 2017 which changed  the data in the calibrated data sets. Calibration changes are described  in the data set version-specific sections.   Note that even if this is not a calibrated data set, calibration  changes are listed as the data will have been re-run and there will be  updates to the calibration files, to the documentation (Science  Operations Center - Instrument Interface Control Document:  SOC_INST_ICD) and to the steps required to calibrate the data.     MVIC updates for Pluto Encounter  Data Sets V3.0  :   This P3 Pluto Encounter dataset release includes all data from the  previous two Pluto deliveries and adds data that was downlinked from  1/31/2016 through 10/31/2016. This dataset completes delivery of all  data covering the Pluto Encounter and subsequent Calibration Campaign.  It includes the additional observations below for MVIC:   PEMV_01_PC_Multi_Map_A_18 2015-188_16:44:09 2016-097T18:02:21 Pluto, Charon PEMV_01_PC_Multi_Map_B_2 2015-189_09:04:09 2016-260T03:34:44 Pluto, Charon PEMV_01_PC_Multi_Map_B_3 2015-189_17:06:14 2016-095T20:48:31 Pluto, Charon PEMV_01_PC_Multi_Map_B_5 2015-190_03:40:28 2016-260T11:35:23 Pluto, Charon PEMV_01_PC_Multi_Map_B_6 2015-190_16:55:29 2016-095T22:56:44 Pluto, Charon PEMV_01_PC_Multi_Map_B_8 2015-191_08:54:53 2016-267T09:59:05 Pluto, Charon PEMV_01_PC_Multi_Map_B_9 2015-191_16:51:38 2016-266T11:36:17 Pluto, Charon PEMV_02_PC_Multi_Map_B_9 2015-191_16:54:28 2016-098T05:33:45 Pluto, Charon PEMV_01_PC_Multi_Map_B_11 2015-192_03:33:58 2016-267T09:18:50 Pluto, Charon PEMV_01_PC_Multi_Map_B_12 2015-192_16:46:18 2016-267T12:43:06 Pluto, Charon PEMV_02_PC_Multi_Map_B_12 2015-192_16:49:08 2016-268T06:19:29 Pluto, Charon PEMV_01_PC_Multi_Map_B_14 2015-193_08:22:29 2016-260T14:53:02 Pluto, Charon PEMV_01_PC_Multi_Map_B_15 2015-193_16:51:03 2016-175T13:40:09 Pluto, Charon PEMV_01_PC_Multi_Map_B_17 2015-194_03:37:27 2016-261T12:54:18 Pluto, Charon PEMV_01_PC_Multi_Map_B_18 2015-194_07:37:55 2016-178T17:49:36 Pluto, Charon PEMV_02_PCNH_Multi_Long_1d1 2015-194_14:45:27 2016-072T10:19:11 P,C, Nix, Hydra PEMV_01_PCNH_Multi_Long_1d1 2015-194_14:49:49 2016-073T00:27:20 P,C, Nix, Hydra PEMV_01_PC_LyMap 2015-194_16:23:01 2016-165T17:29:13 Pluto, Charon PEMV_01_PC_Multi_Long_1d2 2015-194_21:07:43 2016-192T07:45:52 Pluto, Charon PEMV_01_U_TBD_1 2015-194_23:53:45 2016-183T06:40:41 Styx PEMV_01_PC_Color_TimeRes 2015-195_02:47:02 2016-094T06:50:27 Pluto, Charon PEMV_01_N_Color_1 2015-195_04:36:05 2016-073T19:27:17 Nix PEMV_01_H_Color_1 2015-195_04:53:26 2016-187T08:25:21 Hydra PEMV_01_PC_Color_1 2015-195_06:49:08 2016-065T07:41:45 Pluto, Charon PEMV_01_H_Color_Best 2015-195_07:36:05 2016-185T21:21:57 Hydra PEMV_01_N_Color_2 2015-195_08:02:39 2016-075T07:20:33 Nix PEMV_01_N_Color_Best 2015-195_09:11:51 2016-180T12:05:01 Nix PEMV_01_P_LORRI_STEREO_Mosaic 2015-195_10:18:40 2016-272T04:16:47 Pluto PEMV_01_C_Color_2 2015-195_10:40:11 2016-188T12:48:30 Charon PEMV_01_P_Color2 2015-195_11:05:25 2016-191T14:52:18 Pluto PEMV_01_N_Mpan_CA 2015-195_11:14:32 2016-056T17:10:51 Nix PEMV_01_P_MP_Photoslew 2015-195_11:50:47 2016-087T20:01:12 Pluto PEMV_01_P_CharonLight 2015-195_12:08:13 2016-066T02:30:01 Pluto PEMV_01_N_Dep_Soonest 2015-195_15:00:28 2016-134T04:59:30 Nix PEMV_01_P_Multi_Dep_Long_1 2015-195_15:19:50 2016-184T18:29:24 Pluto PEMV_01_PC_Multi_Dep_Long_2 2015-195_19:09:43 2016-073T08:25:15 Pluto, Charon PEMV_01_U_TBD_4 2015-196_02:47:27 2016-190T07:22:45 Pluto System PEMV_02_U_TBD_4 2015-196_02:56:57 2016-190T10:08:55 Pluto System PEMV_01_PC_Multi_Dep_Long_3 2015-196_03:07:26 2016-187T15:48:11 Pluto, Charon PEMV_02_O_RingDep_A_1 2015-196_18:34:41 2016-190T17:32:38 Ring Search PEMV_01_PC_Ralph_Charon_270deg 2015-197_18:38:44 2016-185T13:45:33 P, C PEMV_01_PC_Ralph_N2_Bright 2015-198_07:43:29 2016-179T17:51:05 Pluto, Charon PEMV_01_PC_Ralph_Pluto_CO 2015-199_07:39:46 2016-181T03:54:13 Pluto, Charon PEMV_01_PC_Ralph_Enc_Hem_Dep 2015-199_15:41:45 2016-188T13:33:13 Pluto, Charon PEMV_01_PC_Ralph_Dark_Area 2015-200_07:39:47 2016-147T10:14:22 Pluto, Charon PEMV_01_PC_Ralph_Charon_90Deg 2015-200_23:38:49 2016-155T18:08:32 Pluto, Charon DPMV_01_O_RING_DEP_MVICFRAME_202 2015-202_13:59:37 2016-254T13:18:31 Ring Search DPMV_01_O_RING_DEP_MVICFRAME_211 2015-211_17:49:37 2016-261T04:34:22 Ring Search DPMV_O_RING_DEP_MVICFRAME_305A 2015-305_18:33:42 2016-040T00:34:57 Ring Search DPMV_O_RING_DEP_MVICFRAME_305B 2015-305_20:11:37 2016-040T00:19:39 Ring Search DPMV_O_RING_DEP_MVICFRAME_305C 2015-305_22:23:37 2016-063T06:43:20 Ring Search TRRL_X_RALPH_FUNCLITEA_182__021aFuncColor 2016-182_01:38:44 2016-182T14:33:15 TRRL_X_RALPH_FUNCLITEA_182__021aFuncPan1 2016-182_01:40:46 2016-182T14:36:29 TRRL_X_RALPH_FUNCLITEA_182__021aFuncPan2 2016-182_01:42:47 2016-182T14:39:45 TRRL_X_RALPH_FUNCLITEA_182__021aFuncPanFrame 2016-182_01:44:51 2016-182T15:26:06 TRRL_X_RALPH_FUNCLITEB_182__021bFuncColor 2016-182_02:13:44 2016-182T16:53:20 TRRL_X_RALPH_FUNCLITEB_182__021bFuncPan1 2016-182_02:15:46 2016-182T16:56:21 TRRL_X_RALPH_FUNCLITEB_182__021bFuncPan2 2016-182_02:17:47 2016-182T16:59:13 TRRL_X_RALPH_FUNCLITEB_182__021bFuncPanFrame 2016-182_02:19:51 2016-182T17:43:21 TRMV_M6M7_023A_CAL_197_Color 2016-197_21:59:27 2016-214T17:26:45 Calibration TRMV_M6M7_023A_CAL_197_Pan2 2016-197_22:08:43 2016-214T13:46:02 Calibration TRMV_M6M7_023A_CAL_197_Pan1 2016-197_22:15:43 2016-214T14:21:53 Calibration TRMV_M6M7_023A_CAL_197_PanFrame 2016-197_22:23:47 2016-209T12:50:08 Cal. TRMV_M6M7_023B_CAL_197_Color 2016-197_22:36:27 2016-215T04:56:48 Calibration TRMV_M6M7_023B_CAL_197_Pan2 2016-197_22:44:43 2016-214T14:38:08 Calibration TRMV_M6M7_023B_CAL_197_Pan1 2016-197_22:52:43 2016-214T14:53:57 Calibration TRMV_M6M7_023B_CAL_197_PanFrame 2016-197_23:00:47 2016-208T13:48:42 Cal. TRMV_HD205905_047A_01_CAL_197 2016-198_00:06:27 2016-202T10:24:00 Calibration TRMV_HD205905_047A_02_CAL_197 2016-198_00:14:45 2016-202T11:21:13 Calibration TRMV_HD205905_047B_01_CAL_197 2016-198_00:24:27 2016-202T13:30:42 Calibration TRMV_HD205905_047B_02_CAL_197 2016-198_00:33:45 2016-202T13:48:37 Calibration    Also, updates were made to the calibration files, documentation, and  catalog files.   For any data previously delivered as sub-frame windows, this delivery  will fill in the image data outside those windows.   Changes to the calibration involved only changes to the  spectrum-specific calibration constants provided in FITS headers and  in PDS labels; the calibrated Data Number values in the calibrated  data set, excluding image data outside the sub-frame windows  mentioned above, will not be substantively changed.   As of V3.0, targets for some stars and radio sources have been updated  so that the TARGET_NAME keyword in the label is accurate and more  descriptive than only STAR or CALIBRATION. However the user should  confirm that targets from the data FITS files, if applicable for a  given instrument, match the label name, as there are a few instances  where the FITS keywords for TARGET, SPCCBTNM, and PNTMTHD are not  accurate. The simplest way to check is to instead look at the RA  and Dec in the keywords SPCBRRA and SPCBRDEC in the FITS file.  This issue mostly only occurs with star targets.     MVIC updates for Pluto Encounter  Data Sets V2.0  :    This P2 Pluto Encounter dataset release provides updates to the Pluto  dataset between P1 (data on the ground by 7/31/2015) and P2 (data on  the ground by 1/31/2016). Some data that had been downlinked as a  subframe in the last delivery now has been re-downlinked for the full  frame image. All liens from the initial Pluto delivery have also now  been resolved. The dataset includes the additional observations below:  Obs. Name (Request ID), Obs Date, Downlink Start, Downlink End, Obs. Target DPMV_O_RING_DEP_MVICFRAME_305A 2015-11-01 2016/003 2016/030 Ring Search Observation PEMV_01_C_Color_2 2015-07-14 2015/266 2015/266 Charon Observation PEMV_01_C_MVIC_LORRI_CA 2015-07-14 2015/312 2015/312 Charon Observation PEMV_01_H_Color_1 2015-07-14 2015/283 2015/283 Hydra Observation PEMV_01_H_Color_Best 2015-07-14 2015/283 2015/283 Hydra Observation PEMV_01_N_Color_Best 2015-07-14 2015/283 2015/329 Nix Observation PEMV_01_N_Mpan_CA 2015-07-14 2015/347 2015/347 Nix Observation PEMV_01_PC_Color_1 2015-07-14 2015/283 2015/283 Pluto and Charon obs PEMV_01_PC_Multi_Dep_Long_3 2015-07-15 2015/283 2015/283 Pluto and Charon obs PEMV_01_PC_Multi_Long_1d2 2015-07-13 2015/282 2015/282 Pluto and Charon obs PEMV_01_PC_Multi_Map_A_18 2015-07-07 2015/279 2015/279 Pluto and Charon obs PEMV_01_PC_Multi_Map_A_3 2015-07-02 2015/229 2015/229 Pluto and Charon obs PEMV_01_PC_Multi_Map_A_5 2015-07-03 2015/229 2015/229 Pluto and Charon obs PEMV_01_PC_Multi_Map_B_15 2015-07-12 2015/282 2015/282 Pluto and Charon obs PEMV_01_PC_Multi_Map_B_17 2015-07-13 2015/286 2015/286 Pluto and Charon obs PEMV_01_PC_Multi_Map_B_3 2015-07-08 2015/279 2015/279 Pluto and Charon obs PEMV_01_PC_Multi_Map_B_6 2015-07-09 2015/279 2015/279 Pluto and Charon obs PEMV_01_PC_Ralph_Charon_270deg 2015-07-16 2015/283 2015/283 Pluto and Charon obs PEMV_01_PC_Ralph_Charon_90Deg 2015-07-19 2015/284 2015/284 Pluto and Charon obs PEMV_01_PC_Ralph_Dark_Area 2015-07-19 2015/284 2015/284 Pluto and Charon obs PEMV_01_PC_Ralph_Enc_Hem_Dep 2015-07-18 2015/283 2015/283 Pluto and Charon obsPEMV_01_PC_Ralph_N2_Bright 2015-07-17 2015/283 2015/283 Pluto and Charon obs PEMV_01_PC_Ralph_Pluto_CO 2015-07-18 2015/283 2015/283 Pluto and Charon obs PEMV_01_PC_VISUV_MAP_B_12 2015-06-29 2015/233 2015/233 Pluto and Charon obs PEMV_01_PC_VISUV_MAP_B_19 2015-07-01 2015/229 2015/229 Pluto and Charon obs PEMV_01_PC_VISUV_MAP_B_3 2015-06-26 2015/246 2015/246 Pluto and Charon obs PEMV_01_PC_VISUV_MAP_B_6 2015-06-27 2015/244 2015/244 Pluto and Charon obs PEMV_01_PC_VISUV_MAP_B_9 2015-06-28 2015/237 2015/237 Pluto and Charon obs PEMV_01_P_Color2 2015-07-14 2015/260 2015/262 Pluto Observation PEMV_01_P_HiPhase_HiRes 2015-07-14 2015/255 2015/255 Pluto Observation PEMV_01_P_MPan1 2015-07-14 2015/280 2015/280 Pluto Observation PEMV_01_P_Multi_Dep_Long_1 2015-07-14 2015/278 2015/278 Pluto Observation PEMV_01_P_MVICFlat_Col_1 2015-07-14 2015/253 2015/253 Pluto Observation PEMV_01_P_MVICFlat_Col_2 2015-07-14 2015/253 2015/253 Pluto Observation PEMV_01_P_MVICFlat_Pan_First 2015-07-14 2015/253 2015/253 Pluto Observation PEMV_01_P_MVICFlat_Pan_Second 2015-07-14 2015/253 2015/253 Pluto Observation PEMV_01_P_MVIC_LORRI_CA 2015-07-14 2015/272 2015/272 Pluto Observation PEMV_01_U_TBD_1 2015-07-13 2015/282 2015/283 Kerberos and Styx obs PEMV_02_PC_Multi_Map_B_9 2015-07-10 2015/279 2015/279 Pluto and Charon obs PEMV_02_P_MVICFlat_Col_1 2015-07-14 2015/253 2015/253 Pluto Observation PEMV_02_P_MVICFlat_Col_2 2015-07-14 2015/253 2015/253 Pluto Observation PEMV_02_P_MVICFlat_Pan_First 2015-07-14 2015/253 2015/253 Pluto Observation PEMV_02_P_MVICFlat_Pan_Second 2015-07-14 2015/253 2015/253 Pluto Observation    Processing  :   The data in this data set were created by a software data  processing pipeline on the Science Operations Center (SOC) at  the Southwest Research Institute (SwRI), Department of Space Operations. This SOC pipeline assembled data as FITS files from raw telemetry  packets sent down by the spacecraft and populated the data labels  with housekeeping and engineering values, and computed geometry  parameters using SPICE kernels. The pipeline did not resample  the data.    Calibration  :    Detailed information about calibration of MVIC data is available  in the SOC Instrument Interface Control Document (ICD) in the  DOCUMENT section of this data set. The MVIC calibration will only  be briefly summarized here; refer to the ICD for details about  what is summarized here.   The calibration of MVIC images comprises the following steps:   1) Remove bias and flat-field pattern  1.1) The result is an absolute calibration in raw DATA NUMBER units  (DN), with pixel values proportional to the incoming signal  2) Supply target source spectrum-dependent factors to scale from  absolute DN to scientific (flux and radiance) units; refer to the  DOCUMENT/SOC_INST_ICD*.* for more detail.   In addition, the calibration procedure calculates the error and  a data quality flag for each pixel and includes those results  in the calibrated data product as additional PDS OBJECTs (FITS  extensions) appended to the main OBJECT with the data image.  The quality flag PDS OBJECT is an image of values of the same  size as the main IMAGE product, with each quality flag pixel  mapped to the corresponding pixel in the main product. A quality  flag value of zero indicates a valid pixel; a non-zero value  indicates an invalid pixel (e.g. missing data outside the  window(s) of data intended to be downlinked).   Note that for windowed products, all pixels in an image are not  returned in the downlink telemetry. In the raw data, the pipeline  sets such pixels to zero DN (Data Number); the calibration processes  those zero-DN pixels as if they were real raw values, but also flags  them as missing data in the quality flag PDS OBJECT (FITS extension).  Displaying such images using an automatic stretch (contrast  enhancement) may result in a confusing result with the majority of  the displayed image appearing as an inverse of the calibration  (calibration of zero values); therefore the quality flag PDS OBJECT  should always be checked when looking at these data.   Note also that, at the time these data were created (late 2014), the  Science Operations Center (SOC) data processing pipeline did not have  the capability to merge multiple windows from a single observation.  As a result, in some cases one observation's products in raw and  and calibrated data sets may come from different windows. This is  normal, but it can have some noticeable side-effects:   i) Mismatches in windowing parameters between raw and calibrated  products for the same observation. Either the windowing parameters  differ, or one may be windowed and the other a non-windoed, full  image.   ii) START_TIME and STOP_TIME mismatches between versions of the same  TDI observations with different windows. The start and stop times  of TDI MVIC products are dependent on the start and stop lines of  the window: if the first line of the window is not the first line  of the observation, the START_TIME of the product will be delayed  from the start time of the observation; similarly the last line of  a window that is not the last line of the observation results in a  STOP_TIME that is earlier than the stop time of the observation.  Since there is only one version of each observation in any single  MVIC data set, this will not be noticeable within any single data  set. However, when comparing versions of the same observation from  raw and calibrated data sets, it is possible that the START_TIME  and STOP_TIME values for that observation will differ between the  data sets.   iii) The shift in start and stop times will also affect the  calculation of mid-observation times.   iv) The mid-observation time is used as the lookup in SPICE calls, so  the shift in time will affect calculated geometry values   As part of the preparation for the Pluto flyby in Spring, 2015, the SOC  pipeline was updated to all it to merge multiple windows and/or full  images of the same observation into a single product. so it is  expected that future MVIC data sets will have raw and calibrated  products with consistent windowing parameters, times and geometries.   A PDS OBJECT CALGEOM (FITS extension) with a correction for geometric  distortion, present in previous versions of MVIC data sets, has been  removed from these and future PDS calibrated data sets. Geometric  distorion will be addressed in higher-level products, as it involves  resampling the data.     Data  :   The observations in this data set are stored in data files using  standard Flexible Image Transport System (FITS) format. Each FITS  file has a corresponding detached PDS label file, named according  to a common convention. The FITS files may have image and/or table  extensions. See the PDS label plus the DOCUMENT files for a  description of these extensions and their contents.   This Data section comprises the following sub-topics:   - Filename/Product IDs  - Instrument description  - Other sources of information useful in interpreting these Data  - Visit Description, Visit Number, and Target in the Data Labels    Filename/Product IDs  --------------------   The filenames and product IDs of observations adhere to a  common convention e.g.   MC0_0123456789_0X530_ENG.FIT  ^^^ ^^^^^^^^^^ ^^^^^ ^^^\__/  | | | | ^^  | | | | |  | | | | +--File type (includes dot)  | | | | - .FIT for FITS file  | | | | - .LBL for PDS label  | | | | - not part of product ID  | | | |  | | | +--ENG for CODMAC Level 2 data  | | | SCI for CODMAC Level 3 data  | | |  | | +--Application ID (ApID) of the telemetry data  | | packet from which the data come  | | N.B. ApIDs are case-insensitive  | |  | +--MET (Mission Event Time) i.e. Spacecraft Clock  |  +--Instrument designator    Note that, depending on the observation, the MET in the data filename  and in the Product ID may be similar to the Mission Event Time (MET)  of the actual observation acquisition, but should not be used as an  analog for the acquisition time. The MET is the time that the data are  transferred from the instrument to spacecraft memory and is therefore  not a reliable indicator of the actual observation time. The PDS label  and the index tables are better sources to use for the actual timing of  any observation. The specific keywords and index table column names for which to look are   * START_TIME  * STOP_TIME  * SPACECRAFT_CLOCK_START_COUNT  * SPACECRAFT_CLOCK_STOP_COUNT    Instrument Instrument designators ApIDs **  : : :  MVIC MC0, MC1, MC2, MC3, MP1, MP2, MPF 0X530 - 0X54A *   * Not all values in this range are in this data set  ** ApIDs are case insensitive   There are other ApIDs that contain housekeeping values and  other values. See SOC Instrument ICD (/DOCUMENT/SOC_INST_ICD.*)  for more details.    Here is a summary of the meanings of each instrument designator:   Instr  Dsgn. Description  : :  MC0 MVIC, Color TDI, Red filter  MC1 MVIC, Color TDI, Blue filter  MC2 MVIC, Color TDI, Near-InfraRed (NIR) filter  MC3 MVIC, Color TDI, Methane (CH4) filter  MP1 MVIC, Panchromatic TDI CCD 1  MP2 MVIC, Panchromatic TDI CCD 2  MPF MVIC, Panchromatic frame (5024 pixels)   See SOC Instrument ICD (/DOCUMENT/SOC_INST_ICD.*) for details    Here is a summary of the types of files generated by each ApID  (N.B. ApIDs are case-insensitive) along with the instrument  designator that go with each ApID:    ApIDs Data product description/Prefix(es)  : :  0x530 - MVIC Panchromatic TDI Lossless (CDH 1)/MP1,MP2  0x53f - MVIC Panchromatic TDI Lossless (CDH 2)/MP1,MP2  0x531 - MVIC Panchromatic TDI Packetized (CDH 1)/MP1,MP2  0x540 - MVIC Panchromatic TDI Packetized (CDH 2)/MP1,MP2  0x532 - MVIC Panchromatic TDI Lossy (CDH 1)/MP1,MP2  0x541 - MVIC Panchromatic TDI Lossy (CDH 2)/MP1,MP2  0x533 - MVIC Panchromatic TDI 3x3 Binned Lossless (CDH 1)/MP1,MP2 *  0x542 - MVIC Panchromatic TDI 3x3 Binned Lossless (CDH 2)/MP1,MP2 *  0x534 - MVIC Panchromatic TDI 3x3 Binned Packetized (CDH 1)/MP1,MP2 * 0x543 - MVIC Panchromatic TDI 3x3 Binned Packetized (CDH 2)/MP1,MP2 * 0x535 - MVIC Panchromatic TDI 3x3 Binned Lossy (CDH 1)/MP1,MP2 *  0x544 - MVIC Panchromatic TDI 3x3 Binned Lossy (CDH 2)/MP1,MP2 *  0x536 - MVIC Color TDI Lossless (CDH 1)/MC0,MC1,MC2,MC3  0x545 - MVIC Color TDI Lossless (CDH 2)/MC0,MC1,MC2,MC3  0x537 - MVIC Color TDI Packetized (CDH 1)/MC0,MC1,MC2,MC3  0x546 - MVIC Color TDI Packetized (CDH 2)/MC0,MC1,MC2,MC3  0x538 - MVIC Color TDI Lossy (CDH 1)/MC0,MC1,MC2,MC3  0x547 - MVIC Color TDI Lossy (CDH 2)/MC0,MC1,MC2,MC3  0x539 - MVIC Panchromatic Frame Transfer Lossless (CDH 1)/MPF  0x548 - MVIC Panchromatic Frame Transfer Lossless (CDH 2)/MPF  0x53a - MVIC Panchromatic Frame Transfer Packetized (CDH 1)/MPF  0x549 - MVIC Panchromatic Frame Transfer Packetized (CDH 2)/MPF  0x53b - MVIC Panchromatic Frame Transfer Lossy (CDH 1)/MPF  0x54a - MVIC Panchromatic Frame Transfer Lossy (CDH 2)/MPF   * as of October, 2014, 3x3 modes have not been used    Instrument description  ----------------------   Refer to the following files for a description of this instrument.   CATALOG   MVIC.CAT   DOCUMENTS   RALPH_SSR.*  SOC_INST_ICD.*  NH_RALPH_V###_TI.TXT (### is a version number)    Other sources of information useful in interpreting these Data  --------------------------------------------------------------   Refer to the following files for more information about these data   NH Trajectory tables:   /DOCUMENT/NH_MISSION_TRAJECTORY.* - Heliocentric   RALPH Field Of View definitions:   /DOCUMENT/NH_FOV.*  /DOCUMENT/NH_RALPH_V###_TI.TXT     Visit Description, Visit Number, and Target in the Data Labels  ---------------------------------------------------------------   The observation sequences were defined in Science Activity Planning  (SAP) documents, and grouped by Visit Description and Visit Number.  The SAPs are spreadsheets with one Visit Description & Number per row.  A nominal target is also included on each row and included in the data  labels, but does not always match with the TARGET_NAME field's value in  the data labels. In some cases, the target was designated as RA,DEC  pointing values in the form ``RADEC:123.45,-12.34'' indicating Right  Ascension and Declination, in degrees, of the target from the  spacecraft in the Earth Equatorial J2000 inertial reference frame.  This indicates either that the target was either a star, or that the  target's ephemeris was not loaded into the spacecraft's attitude and  control system which in turn meant the spacecraft could not be pointed  at the target by a body identifier and an inertial pointing value had  to be specified as Right Ascension and Declination values. PDS-SBN  practices do not allow putting a value like RADEC:... in the PDS  TARGET_NAME keyword's value. In those cases the PDS TARGET_NAME value  is set to CALIBRATION. TARGET_NAME may be N/A (Not Available or Not  Applicable) for a few observations in this data set; typically that  means the observation is a functional test so N/A is an appropriate  entry for those targets, but the PDS user should also check the  NEWHORIZONS:OBSERVATION_DESC and NEWHORIZONS:SEQUENCE_ID keywords in  the PDS label, plus the provided sequence list (see Ancillary Data  below) to assess the possibility that there was an intended target.  These two keywords are especially useful for STAR targets as often  stars are used as part of instrument calibrations, and are  included as part of the sequencing description which is captured  in these keywords.     Ancillary Data  :   The geometry items included in the data labels were computed  using the SPICE kernels archived in the New Horizons SPICE  data set, NH-X-SPICE-6-PLUTO-V1.0.   Every observation provided in this data set was taken as a part of a  particular sequence. A list of these sequences has been provided in  file DOCUMENT/SEQ_MVIC_PLUTO.TAB. In addition, the  sequence identifier (ID) and description are included in the PDS label  for every observation. N.B. While every observation has an associated  sequence, every sequence may not have associated observations. Some  sequences may have failed to execute due to spacecraft events (e.g.  safing). No attempt has been made during the preparation of this data  set to identify such empty sequences, so it is up to the user to  compare the times of the sequences to the times of the available  observations from INDEX/INDEX.TAB to identify such sequences.    Time  :   There are several time systems, or units, in use in this dataset:  New Horizons spacecraft MET (Mission Event Time or Mission Elapsed  Time), UTC (Coordinated Universal Time), and TDB Barycentric  Dynamical Time.   This section will give a summary description of the relationship  between these time systems. For a complete explanation of these  time systems the reader is referred to the documentation  distributed with the Navigation and Ancillary Information  Facility (NAIF) SPICE toolkit from the PDS NAIF node, (see  http://naif.jpl.nasa.gov/).   The most common time unit associated with the data is the spacecraft  MET. MET is a 32-bit counter on the New Horizons spacecraft that  runs at a rate of about one increment per second starting from a  value of zero at   19.January, 2006 18:08:02 UTC   or   JD2453755.256337 TDB.   The leapsecond adjustment (DELTA_ET : ET - UTC) was 65.184s at  NH launch, and the first three additional leapseconds occurred  in at the ends of December, 2009, June, 2012 and June, 2015.  Refer to the NH SPICE data set, NH-J/P/SS-SPICE-6-V1.0, and the  SPICE toolkit documentation, for more details about leapseconds.   The data labels for any given product in this dataset usually  contain at least one pair of common UTC and MET representations  of the time at the middle of the observation. Other portions  of the products, for example tables of data taken over periods  of up to a day or more, will only have the MET time associated  with a given row of the table.   For the data user's use in interpreting these times, a reasonable  approximation (+/- 1s) of the conversion between Julian Day (TDB)  and MET is as follows:   JD TDB : 2453755.256337 + ( MET / 86399.9998693 )   For more accurate calculations the reader is referred to the  NAIF/SPICE documentation as mentioned above.    Reference Frame  :    Geometric Parameter Reference Frame  -----------------------------------   Earth Mean Equator and Vernal Equinox of J2000 (EMEJ2000) is the  inertial reference frame used to specify observational geometry items  provided in the data labels. Geometric parameters are based on best  available SPICE data at time of data creation.    Epoch of Geometric Parameters  -----------------------------   All geometric parameters provided in the data labels were computed at  the epoch midway between the START_TIME and STOP_TIME label fields.     Software  :   The observations in this data set are in standard FITS format  with PDS labels, and can be viewed by a number of PDS-provided  and commercial programs. For this reason no special software is  provided with this data set.    Contact Information  :   For any questions regarding the data format of the archive,  contact   New Horizons RALPH Principal Investigator:   Alan Stern, Southwest Research Institute   S. Alan Stern   Southwest Research Institute (SwRI)  Department of Space Studies  1050 Walnut Street, Suite 400  Boulder, CO 80302  USA

Confidence Level Overview  :  During the processing of the data in preparation for  delivery with this volume, the packet data associated with each  observation were used only if they passed a rigorous verification  process including standard checksums.   In addition, raw (Level 2) observation data for which adequate  contemporary housekeeping and other ancillary data are not available  may not be reduced to calibrated (Level 3) data. This issue is raised  here to explain why some data products in the raw data set,   NH-P-MVIC-2-PLUTO-V3.0,   may not have corresponding data products in the calibrated data set,   NH-P-MVIC-3-PLUTO-V3.0.    Data coverage and quality  :  Every observation provided in this data set was taken as a part of a  particular sequence. A list of these sequences has been provided in  file DOCUMENT/SEQ_MVIC_PLUTO.TAB. N.B. Some sequences  provided may have zero corresponding observations.   Refer to the Confidence Level Overview section above for a summary  of steps taken to assure data quality.   During functional tests, some TDI images with prefixes like mc0,  mc1, mc2, mc3, mp1, and mp2 will have a height (PDS keyword LINES)  of less than 100 lines (values of 32, 33, 52, and 96 are common)  and a width (LINE_SAMPLES) of 5024, giving the impression of a  noodle-like image. These images were only generated to confirm  proper operation of MVIC and are unlikely to have any scientific  value. Functional test images can usually be identified by the  case-insensitive string 'func' in the value of the  NEWHORIZONS:SEQUENCE_ID keyword in the PDS label.    Observation descriptions in this data set catalog  :   Some users will expect to find descriptions of the observations  in this data set here, in this Confidence Level Note. This data  set follows the more common convention of placing those  descriptions under the Data Set Description (above, if the user is  reading this in the DATASET.CAT file) of this data set catalog.    Caveat about TARGET_NAME in PDS labels and observational intent  :   The downlink team on New Horizons has  created an automated system to take various uplink products, decode  things like Chebyshev polynomials in command sequences representing  celestial body ephemerides for use on the spacecraft to control  pointing, and infer from those data what the most likely intended  target was at any time during the mission. This works well during  flyby encounters and less so during cruise phases and hibernation.   The user of these PDS data needs to  be cautious when using the TARGET_NAME and other target-related  parameters stored in this data set. This is less an issue for the  plasma and particle instruments, more so for pointing instruments.  To this end, the heliocentric ephemeris of the spacecraft, the  spacecraft-relative ephemeris of the inferred target, and the  inertial attitude of the instrument reference frame are provided  with all data, in the J2000 inertial reference frame, so the user  can check where that target is in the Field Of View (FOV) of the  instrument.   Finally, note that, within the FITS headers of the data products,  the sequence tables, and other NH Project-internal documents used  in this data set and/or inserted into the data set catalog,  informal names are often used for targets instead of the canonical  names required for the TARGET_NAME keyword. For example, during  the Pluto mission phase, instead of the TARGET_NAME '15810 ARAWN  (1994 JR1)' there might be found any of the following: 1994JR1;  1994 JR1; JR1. For all values where the PDS keyword TARGET_NAME  is used (e.g. in PDS labels and in index tables), the canonical,  PDS-approved names are used (if not, please bring this to the  attention of PDS so it can be rectified). However, within the  context of this data set, these project abbreviations are not  ambiguous (e.g. there is only one NH target with 'JR1' in its  name), so there has been, and will be, no attempt to expand such  abbreviations where they occur outside formal PDS keyword values.    Review  :  This dataset was peer reviewed and certified for scientific use on  June 19, 2017.