Commit eda174ce authored by Amy Stamile's avatar Amy Stamile
Browse files

Clean up comparison notebooks and fix vis.py

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README.md

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@@ -59,21 +59,3 @@ To build the docs: 
1. Browse to the `index.html` file in `docs/public` to open the docs.  If needed, run a utility like `http-server` in the `docs/public` directory to serve the docs on localhost.

1. Browse to the `index.html` file in `docs/public` to open the docs.  If needed, run a utility like `http-server` in the `docs/public` directory to serve the docs on localhost.





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## Status Report - November 2019



For full testing reports and example usage, please see the linked example Jupyter notebooks in the table below. 



|       Instrument      |                      Jupyter Notebooks                     |  Production Ready |    Difference CSM -> ISIS (in pixels)   |    Difference ISIS -> CSM (in pixels)   |

|:---------------------:|:-------------------------------------------------:|:-----------------:|:---------------------------------------:|:---------------------------------------:|

|       MRO HiRISE      |     [link](examples/mro_hirise_isis_cmp.ipynb)    |     sub-pixel; in testing for production    | sample mean=-2.0e-05; line mean=2.5e-08 | sample mean=-3.0e-08; line mean=1.2e-04 |

|        MRO CTX        |      [link](examples/mro_ctx_isis_cmp.ipynb)      | nearly sub-pixel; still in research |  gross error in line  |     sample mean=0.0002; line mean=-0.07     |

|        MEX HRSC       |      [link](examples/mex_hrsc_isis_cmp.ipynb)     |         sub-pixel; in testing for production        |      sample mean=0.000038; line mean=-0.000072      |       sample mean=-0.000038 ; line mean=-7.512e-05       |

|        LROC NAC       |      [link](examples/lrocnac_isis_cmp.ipynb)      | sub-pixel; in testing for production |      sample mean=-0.003; line mean=-0.0006      |                   sample mean=0.0005	line mean=0.003                   |

| Kaguya Terrain Camera |     [link](examples/kaguya_tc_isis_cmp.ipynb)     | barely sub-pixel; in testing |     sample mean=0.0001; line mean=0.00003    |      sample mean=0.009; line mean=-1.242      |

|   Messenger MDIS NAC  | [link](examples/messenger_mdisnac_isis_cmp.ipynb) |  sub-pixel; in testing for production |      sample mean=-0.01; line mean=-0.003     |       sample mean=0.01; line mean=0.003      |

|  Cassini ISS NAC      |      [link](examples/cassini_isis_nac_cmp.ipynb)      |  sub-pixel; in testing for production  |    sample mean=-0.001; line mean=0.01    |     sample mean=0.001; line mean=-0.01     |

|  Cassini ISS WAC      |      [link](examples/cassini_isis_wac_cmp.ipynb)      |  sub-pixel; in testing for production  |    sample mean=0.001; line mean=0.004    |     sample mean=-0.001; line mean=-0.004     |

|  Dawn Framing Camera  |      [link](examples/dawn_fc_isis_cmp.ipynb)      |     sub-pixel; in testing for production    | sample mean=-0.02; line mean=0.003 | sample mean=0.02; line mean=-0.003 |



The Difference column (CSM -> ISIS) represents the mean difference in pixels from running usgscsm's *image2ground* and then back to the camera using ISIS3's *campt* (ground2image). The Difference column (ISIS -> CSM) is simply the reverse starting with ISIS3 first with *campt* (image2ground) and then usgscsm's *ground2image*.

examples/cassini_isis_nac_cmp.ipynb

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PDS_VERSION_ID = PDS3



/* FILE CHARACTERISTICS */



RECORD_TYPE = FIXED_LENGTH

RECORD_BYTES = 1048

FILE_RECORDS = 1028



/* POINTERS TO DATA OBJECTS */



^IMAGE_HEADER = ("N1702360370_1.IMG",1)

^TELEMETRY_TABLE = ("N1702360370_1.IMG",4)

^LINE_PREFIX_TABLE = ("N1702360370_1.IMG",5)

^IMAGE = ("N1702360370_1.IMG",5)



/* IDENTIFICATION DATA ELEMENTS */



ANTIBLOOMING_STATE_FLAG = "OFF"

BIAS_STRIP_MEAN = 8.850293

CALIBRATION_LAMP_STATE_FLAG = "N/A"

COMMAND_FILE_NAME = "trigger_3618_1.ioi"

COMMAND_SEQUENCE_NUMBER = 3618

DARK_STRIP_MEAN = 0.269221

DATA_CONVERSION_TYPE = "TABLE"

DATA_SET_ID = "CO-S-ISSNA/ISSWA-2-EDR-V1.0"

DELAYED_READOUT_FLAG = "NO"

DESCRIPTION = "Incomplete product finalized due to truncated lines."

DETECTOR_TEMPERATURE = -89.243546 <DEGC>

EARTH_RECEIVED_START_TIME = 2011-346T22:30:08.981

EARTH_RECEIVED_STOP_TIME = 2011-346T22:30:49.765

ELECTRONICS_BIAS = 112

EXPECTED_MAXIMUM = (62.996498,69.454498)

EXPECTED_PACKETS = 576

EXPOSURE_DURATION = 4600.000000

FILTER_NAME = ("CL1","UV3")

FILTER_TEMPERATURE = 0.248629

FLIGHT_SOFTWARE_VERSION_ID = "1.4"

GAIN_MODE_ID = "29 ELECTRONS PER DN"

IMAGE_MID_TIME = 2011-346T05:02:22.073

IMAGE_NUMBER = "1702360370"

IMAGE_OBSERVATION_TYPE = {"SCIENCE"}

IMAGE_TIME = 2011-346T05:02:24.373

INSTRUMENT_DATA_RATE = 182.783997

INSTRUMENT_HOST_NAME = "CASSINI ORBITER"

INSTRUMENT_ID = "ISSNA"

INSTRUMENT_MODE_ID = "FULL"

INSTRUMENT_NAME = "IMAGING SCIENCE SUBSYSTEM - NARROW ANGLE"

INST_CMPRS_PARAM = ("N/A","N/A","N/A","N/A")

INST_CMPRS_RATE = (5.333330,3.631307)

INST_CMPRS_RATIO = 2.203063

INST_CMPRS_TYPE = "LOSSLESS"

LIGHT_FLOOD_STATE_FLAG = "ON"

METHOD_DESC = "ISSPT2.7;Enceladus;ISS_158EN_ENCEL001_PRIME"

MISSING_LINES = 31

MISSING_PACKET_FLAG = "NO"

MISSION_NAME = "CASSINI-HUYGENS"

MISSION_PHASE_NAME = "EXTENDED-EXTENDED MISSION"

OBSERVATION_ID = "ISS_158EN_ENCEL001_PRIME"

OPTICS_TEMPERATURE = (0.627499,1.905708)

ORDER_NUMBER = 16

PARALLEL_CLOCK_VOLTAGE_INDEX = 9

PREPARE_CYCLE_INDEX = 4

PRODUCT_CREATION_TIME = 2011-346T15:34:07.000

PRODUCT_ID = "1_N1702360370.120"

PRODUCT_VERSION_TYPE = "FINAL"

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SENSOR_HEAD_ELEC_TEMPERATURE = 1.633024

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SHUTTER_MODE_ID = "NACONLY"

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SOFTWARE_VERSION_ID = "ISS 11.00 05-24-2006"

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OBJECT = LINE_PREFIX_TABLE

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END_OBJECT = LINE_PREFIX_TABLE

OBJECT = IMAGE

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END_OBJECT = IMAGE

END