Commit 290eefbe authored by AustinSanders's avatar AustinSanders Committed by Jesse Mapel
Browse files

Initial KaguyaMiIsisLabelNaifSpiceDriver (#435) 

* Initial KaguyaMiIsisLabelNaifSpiceDriver

* Initial kaguyamiisislabelnaifspicedriver and tests

* kaguyami test data

* Removed comment and conf files from data area

* Updated comments to propertly reflect MI instrument
parent eeab47ba

ale/drivers/selene_drivers.py

+332 −0
Original line number Diff line number Diff line
@@ -6,6 +6,7 @@ import spiceypy as spice 
from ale.base import Driver

from ale.base.data_naif import NaifSpice

from ale.base.label_pds3 import Pds3Label

from ale.base.label_isis import IsisLabel

from ale.base.type_sensor import LineScanner
@@ -558,6 +559,7 @@ class KaguyaMiPds3NaifSpiceDriver(LineScanner, Pds3Label, NaifSpice, Driver): 
        base_band = band_map[self.label.get("BASE_BAND")]

        return base_band





    @property

    def instrument_id(self):

        """
@@ -850,3 +852,333 @@ class KaguyaMiPds3NaifSpiceDriver(LineScanner, Pds3Label, NaifSpice, Driver): 
          ISIS sensor model version

        """

        return 1





class KaguyaMiIsisLabelNaifSpiceDriver(LineScanner, NaifSpice, IsisLabel, Driver):

    @property

    def base_band(self):

        """

        Which band the bands are registered to.



        Returns

        -------

        base_band : str

            The base band of the instrument

        """

        band_map = {

            "MV1" : "MI-VIS1",

            "MV2" : "MI-VIS2",

            "MV3" : "MI-VIS3",

            "MV4" : "MI-VIS4",

            "MV5" : "MI-VIS5",

            "MN1" : "MI-NIR1",

            "MN2" : "MI-NIR2",

            "MN3" : "MI-NIR3",

            "MN4" : "MI-NIR4"

        }

        base_band = band_map[self.label['IsisCube']['BandBin']['BaseBand']]

        return base_band



    @property

    def instrument_id(self):

        """

        Id takes the form of LISM_<BASE_BAND> where <BASE_BAND> is which band

        the bands were registered to.



        Returns

        -------

        : str

          instrument id

        """



        id = f"LISM_{self.base_band}"

        return id



    @property

    def sensor_model_version(self):

        """

        Returns ISIS instrument sensor model version number



        Returns

        -------

        : int

          ISIS sensor model version

        """

        return 2





    @property

    def spacecraft_clock_start_count(self):

        """

        The original SC_CLOCK_START_COUNT key is often incorrect and cannot be trusted.

        Therefore we get this information from CORRECTED_SC_CLOCK_START_COUNT



        Returns

        -------

        : float

          spacecraft clock start count in seconds

        """

        return self.label['IsisCube']['Instrument']['CorrectedScClockStartCount'].value







    @property

    def spacecraft_clock_stop_count(self):

        """

        The original SC_CLOCK_START_COUNT key is often incorrect and cannot be trusted.

        Therefore we get this information from CORRECTED_SC_CLOCK_STOP_COUNT



        Returns

        -------

        : float

          spacecraft clock start count in seconds

        """

        return self.label['IsisCube']['Instrument']['CorrectedScClockStopCount'].value





    @property

    def ephemeris_start_time(self):

        """

        Returns the ephemeris start time of the image. Expects spacecraft_id to

        be defined. This should be the integer naif ID code of the spacecraft.



        Returns

        -------

        : float

          ephemeris start time of the image

        """

        return spice.sct2e(self.spacecraft_id, self.spacecraft_clock_start_count)





    @property

    def ephemeris_stop_time(self):

        """

        Returns the ephemeris start time of the image. Expects spacecraft_id to

        be defined. This should be the integer naif ID code of the spacecraft.



        Returns

        -------

        : float

          ephemeris start time of the image

        """

        return spice.sct2e(self.spacecraft_id, self.spacecraft_clock_stop_count)





    @property

    def sensor_frame_id(self):

        """

        Returns the sensor frame id.  Depends on the instrument that was used to

        capture the image.



        Returns

        -------

        : int

          Sensor frame id

        """

        spectra = self.base_band[3]

        return spice.namfrm(f"LISM_MI_{spectra}_HEAD")





    @property

    def detector_center_line(self):

        """

        Returns the center detector line of the detector. Expects tc_id to be

        defined. This should be a string of the form LISM_MI1 or LISM_MI2.



        We subtract 0.5 from the center line because as per the IK:

        Center of the first pixel is defined as "1.0".



        Returns

        -------

        : int

          The detector line of the principle point

        """

        return spice.gdpool('INS{}_CENTER'.format(self.ikid), 0, 2)[1] - 0.5



    @property

    def detector_center_sample(self):

        """

        Returns the center detector sample of the detector. Expects tc_id to be

        defined. This should be a string of the form LISM_MI1 or LISM_MI2.



        We subtract 0.5 from the center sample because as per the IK:

        Center of the first pixel is defined as "1.0".



        Returns

        -------

        : int

          The detector sample of the principle point

        """

        return spice.gdpool('INS{}_CENTER'.format(self.ikid), 0, 2)[0] - 0.5





    @property

    def _odkx(self):

        """

        Returns the x coefficients of the optical distortion model.

        Expects tc_id to be defined. This should be a string of the form

        LISM_MI1 or LISM_MI2.



        Returns

        -------

        : list

          Optical distortion x coefficients

        """

        return spice.gdpool('INS{}_DISTORTION_COEF_X'.format(self.ikid),0, 4).tolist()





    @property

    def _odky(self):

        """

        Returns the y coefficients of the optical distortion model.

        Expects tc_id to be defined. This should be a string of the form

        LISM_MI1 or LISM_MI2.



        Returns

        -------

        : list

          Optical distortion y coefficients

        """

        return spice.gdpool('INS{}_DISTORTION_COEF_Y'.format(self.ikid), 0, 4).tolist()





    @property

    def boresight_x(self):

        """

        Returns the x focal plane coordinate of the boresight.

        Expects ikid to be defined. This should be the NAIF integer ID for the

        sensor.



        Returns

        -------

        : float

          Boresight focal plane x coordinate

        """

        return spice.gdpool('INS{}_BORESIGHT'.format(self.ikid), 0, 1)[0]





    @property

    def boresight_y(self):

        """

        Returns the y focal plane coordinate of the boresight.

        Expects ikid to be defined. This should be the NAIF integer ID for the

        sensor.



        Returns

        -------

        : float

          Boresight focal plane x coordinate

        """

        return spice.gdpool('INS{}_BORESIGHT'.format(self.ikid), 1, 1)[0]







    @property

    def usgscsm_distortion_model(self):

        """

        Kaguya uses a unique radial distortion model so we need to overwrite the

        method packing the distortion model into the ISD.



        from the IK:



        Line-of-sight vector of pixel no. n can be expressed as below.



        Distortion coefficients information:

        INS<INSTID>_DISTORTION_COEF_X  = ( a0, a1, a2, a3)

        INS<INSTID>_DISTORTION_COEF_Y  = ( b0, b1, b2, b3),



        Distance r from the center:

        r = - (n - INS<INSTID>_CENTER) * INS<INSTID>_PIXEL_SIZE.



        Line-of-sight vector v is calculated as

        v[X] = INS<INSTID>BORESIGHT[X] + a0 + a1*r + a2*r^2 + a3*r^3 ,

        v[Y] = INS<INSTID>BORESIGHT[Y] + r+a0 + a1*r +a2*r^2 + a3*r^3 ,

        v[Z] = INS<INSTID>BORESIGHT[Z]



        Expects odkx and odky to be defined. These should be a list of optical

        distortion x and y coefficients respectively.



        Returns

        -------

        : dict

          radial distortion model



        """

        return {

            "kaguyalism": {

                "x" : self._odkx,

                "y" : self._odky,

                "boresight_x" : self.boresight_x,

                "boresight_y" : self.boresight_y

            }

        }





    @property

    def line_exposure_duration(self):

        """

        Returns Line Exposure Duration



        Kaguya has an unintuitive key for this called CORRECTED_SAMPLING_INTERVAL.

        The original LINE_EXPOSURE_DURATION PDS3 keys is often incorrect and cannot

        be trusted.



        Returns

        -------

        : float

          Line exposure duration

        """

        # It's a list, but only sometimes.

        # seems to depend on whether you are using the original zipped archives or

        # if its downloaded from Jaxa's image search:

        # (https://darts.isas.jaxa.jp/planet/pdap/selene/product_search.html#)

        try:

            return self.label['IsisCube']['Instrument']['CorrectedSamplingInterval'][0].value * 0.001 # Scale to seconds

        except:

            return self.label['IsisCube']['Instrument']['CorrectedSamplingInterval'].value * 0.001  # Scale to seconds







    @property

    def focal2pixel_samples(self):

        """

        Calculated using 1/pixel pitch

        Expects ikid to be defined. This should be the NAIF integer ID code

        for the sensor.



        Returns

        -------

        : list

          focal plane to detector samples

        """

        pixel_size = spice.gdpool('INS{}_PIXEL_SIZE'.format(self.ikid), 0, 1)[0]

        return [0, 0, -1/pixel_size]





    @property

    def focal2pixel_lines(self):

        """

        Calculated using 1/pixel pitch

        Expects ikid to be defined. This should be the NAIF integer ID code

        for the sensor.



        Returns

        -------

        : list

          focal plane to detector lines

        """

        pixel_size = spice.gdpool('INS{}_PIXEL_SIZE'.format(self.ikid), 0, 1)[0]

        return [0, 1/pixel_size, 0]





    def spacecraft_direction(self):

        """

        Gets the moving direction of the spacecraft from the label, where -1 is moving

        as intended and 1 is moving inverted.



        Returns

        -------

        : int

          Moving direction of the spacecraft

        """

        return int(self.label['SatelliteMovingDirection'])

tests/pytests/data/MNA_2B2_01_04192S136E3573/MNA_2B2_01_04192S136E3573_0.xsp

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 ~NAIF/SPC BEGIN COMMENTS~

; /users/arsanders/pds/kaguya_mi/out/MNA_2B2_01_04192S136E3573_0.bsp LOG FILE



; Created 2022-01-12/22:33:30.00.

;

; BEGIN SPKMERGE COMMANDS



LEAPSECONDS_KERNEL = /Volumes/pkgs/isis3/isis_data/base/kernels/lsk/naif0012.tls



SPK_KERNEL = /users/arsanders/pds/kaguya_mi/out/MNA_2B2_01_04192S136E3573_0.bsp

SOURCE_SPK_KERNEL = /Volumes/pkgs/isis3/isis_data/kaguya/kernels/tspk/de421.bsp

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SOURCE_SPK_KERNEL = /Volumes/pkgs/isis3/isis_data/kaguya/kernels/spk/SEL_M_071020_090610_SGMH_02.BSP

    INCLUDE_COMMENTS = NO

    BODIES           = -131

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; END SPKMERGE COMMANDS

 ~NAIF/SPC END COMMENTS~

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'-18258F16700DE9^2'

'5C448CEB6E90E^-1'

'15C646FF470027^-1'

'F1C7E8F8F776D8^-3'

'10F78FEF5E806C^-3'

'C0A8464498B058^-5'

'-7DF174E569D61^-6'

'-8A9DB034929B6^-6'

'-796BD7A9A35C6C^-7'

'44020271F3FA4C^5'

'-3366C4B3508D06^3'

'-A8E947E9D2D51^1'

'-B4754CEBF58558^-2'

'9947725CB810E^-2'

'81B89F9DC79B48^-3'

'A7F59511813CA^-4'

'9B69DD6C4D3FE8^-5'

'181FA062006DDA^-6'

'-3BDBCACFD626D6^-6'

'-3E584A962C06A8^-7'

'105A734^8'

'1518^6'

'23^2'

'1^1'

END_ARRAY 2 39

BEGIN_ARRAY 3 45

'DE-0421LE-0421                          '

'106226B2B0BF8E^8'

'106226C1F9B55^8'

'3'

'0'

'1'

'2'

45

'1064FF4^8'

'A8C^5'

'8E22B794F90008^7'

'EEE8D6D81E5A1^5'

'-AABE6F657249A8^5'

'-5FE57B533AAB28^3'

'10A5EB002DE6A5^3'

'10B84FB0EEE394^1'

'-8CD1BA726A1888^-1'

'82CF47E97B1878^-3'

'-7374F2420EB8FC^-4'

'-1EE0E376C39766^-3'

'-BCDF1E7533038^-6'

'1767DFE716A895^-4'

'-5AA83C40B0E84^-6'

'-7CD01731C8E9^6'

'11DDF620B1685D^7'

'A145364DE5254^4'

'-38DE3A1CCB63CA^4'

'-27CEC30CD5D37C^2'

'32E725D2ADAE76^1'

'56E66012BE5428^-1'

'-F5EEDD595F80D^-3'

'-470BB6A9D4CAB4^-3'

'757723E61765FC^-5'

'30F8A540C86366^-4'

'-80026ACD2AD2E8^-6'

'-224EACF88FF4A8^-5'

'-3637D409B11BB4^6'

'7BEFD3A3C13FB^6'

'45EC114469A534^4'

'-18A76F6977E21^4'

'-11425F704D47C5^2'

'1612B48A9069A3^1'

'26226CC069C5DC^-1'

'-898CAA2CC2B57^-3'

'-28024902FFCE78^-3'

'1F64C2D26A07C6^-4'

'1D8A4502AEE38B^-4'

'-191771B4FAC53D^-5'

'-14E65A64A9A4D2^-5'

'105A734^8'

'1518^6'

'29^2'

'1^1'

END_ARRAY 3 45

BEGIN_ARRAY 4 86

'SPK_STATES_09                           '

'106226B2B0BF8E^8'

'106226C1F9B55^8'

'-83'

'12D'

'1'

'9'

86

'-6201C397B3B11C^3'

'-1433219E69454F^2'

'-3DEAC7F6760A7^3'

'-C7A16FEE4758C^0'

'-B46704C2B72BF8^0'

'13B20780700DBF^1'

'-64CB5CACE73808^3'

'-3E6F505C9672D^2'

'-3937B01D1C148C^3'

'-B4DEA7545A405^0'

'-B3EBB1EE45C4F^0'

'1465F9D22ACD79^1'

'-674DAE2187B6A^3'

'-687FAE6099BFE8^2'

'-345C1E551A328E^3'

'-A19F9752703C08^0'

'-B2F143226AA17^0'

'150B59AB742983^1'

'-6986FF20787F24^3'

'-92468CF2A9E17^2'

'-2F5B8A4EBB3FC4^3'

'-8DF1C3F94BC29^0'

'-B178AEDFC4419^0'

'15A1B6FEB7C59C^1'

'-6B75CA770151FC^3'

'-BBA67B1173684^2'

'-2A398485CE5374^3'

'-79E33762749C08^0'

'-AF830F04851298^0'

'1628AEF312EF2C^1'

'-6D18C001BAF634^3'

'-E482555591BBF^2'

'-24F9B2ACC124B8^3'

'-65820EB7C95F74^0'

'-AD11E8557B27E^0'

'169FEF25AE68A2^1'

'-6E6EC3F103E5B8^3'

'-10CBD5D6A0723C^3'

'-1F9FCC794028B6^3'

'-50DC22F49C8A7^0'

'-AA270992E4D01^0'

'17072F0197ECB1^1'

'-6F76EE7880D0E4^3'

'-1343B473FDDCAF^3'

'-1A2F99D289FC7F^3'

'-3BFF6415137964^0'

'-A6C473081F613^0'

'175E2CC7E91C3A^1'

'-70308CAA7DE708^3'

'-15AE0476E8E0FC^3'

'-14ACF117B8913B^3'

'-26FA11060CCD08^0'

'-A2EC7A262183D8^0'

'17A4AFE0B7A9D8^1'

'-709B2103BA211^3'

'-180912AB29094E^3'

'-F1BB48D3F4FA2^2'

'-11DA60F45D0DF7^0'

'-9EA1D269C6A078^0'

'17DA8ACFD34168^1'

'-70B663456036E^3'

'-1A53365953EF17^3'

'-97FD004674DE88^2'

'3517C4E96C29FA^-1'

'-99E757C00B181^0'

'17FF99073C3F86^1'

'-708240C771A99C^3'

'-1C8AD1A9A8DE26^3'

'-3DD375394CD92C^2'

'187B001CF430DF^0'

'-94C005CCA8EB7^0'

'1813BAF466EB76^1'

'1062256D2EB344^8'

'106225A92EB344^8'

'106225E52EB344^8'

'106226212EB344^8'

'1062265D2EB344^8'

'106226992EB344^8'

'106226D52EB344^8'

'106227112EB344^8'

'1062274D2EB344^8'

'106227892EB343^8'

'106227C52EB343^8'

'106228012EB343^8'

'B^1'

'C^1'

END_ARRAY 4 86

TOTAL_ARRAYS 4

 ~NAIF/SPC BEGIN COMMENTS~

; /users/arsanders/pds/kaguya_mi/out/MNA_2B2_01_04192S136E3573_1.bsp LOG FILE



; Created 2022-01-12/22:33:34.00.

;

; BEGIN SPKMERGE COMMANDS



LEAPSECONDS_KERNEL = /Volumes/pkgs/isis3/isis_data/base/kernels/lsk/naif0012.tls



SPK_KERNEL = /users/arsanders/pds/kaguya_mi/out/MNA_2B2_01_04192S136E3573_1.bsp

SOURCE_SPK_KERNEL = /Volumes/pkgs/isis3/isis_data/kaguya/kernels/tspk/de421.bsp

    INCLUDE_COMMENTS = NO

    BODIES           = 3, 10, 301

    BEGIN_TIME       = 2008 SEP 16 20:10:25.508

    END_TIME         = 2008 SEP 16 20:10:40.793

SOURCE_SPK_KERNEL = /Volumes/pkgs/isis3/isis_data/kaguya/kernels/spk/SEL_M_071020_090610_SGMH_02.BSP

    INCLUDE_COMMENTS = NO

    BODIES           = -131

    BEGIN_TIME       = 2008 SEP 16 20:10:25.508

    END_TIME         = 2008 SEP 16 20:10:40.793



; END SPKMERGE COMMANDS

 ~NAIF/SPC END COMMENTS~

tests/pytests/data/MNA_2B2_01_04192S136E3573/MNA_2B2_01_04192S136E3573_isis3.lbl

0 → 100644
+447 −0

File added.

Preview size limit exceeded, changes collapsed.

tests/pytests/data/MNA_2B2_01_04192S136E3573/SEL_M_ALL_D_V02_0_sliced_-131000.xc

0 → 100644
+104 −0
Original line number Diff line number Diff line 
DAFETF NAIF DAF ENCODED TRANSFER FILE

'DAF/CK  '

'2'

'6'

'SELENE CK file                                              '

BEGIN_ARRAY 1 83

'SELENE CK data type 3                   '

'35FAD331^8'

'35FAD342^8'

'-1FFB8'

'1'

'3'

'1'

83

'309C3E01E638E8^0'

'6837EA03D0857C^0'

'-1E11F49A20E54^0'

'E2BB5C80C74E18^0'

'AD03DA5119CE08^-2'

'-100E6B367A0F91^-2'

'38088538EF34D8^-2'

'30A09140DA89B2^0'

'6852874A8E7408^0'

'-1E0B80AA3AB7F1^0'

'E2AF0C6A85D028^0'

'189374BC6A7EFA^-1'

'-5BC01A36E2EB1C^-2'

'75F6FD21FF2E4C^-2'

'30A99CD8DD994^0'

'68856EE1D6B164^0'

'-1DFF93BED778EA^0'

'E2973B946DEF1^0'

'16872B020C49BB^-1'

'-AA64C2F837B4A8^-2'

'902DE00D1B7178^-2'

'30B2F85843E6A6^0'

'68B871137351B4^0'

'-1DF3FAFDCADB67^0'

'E27F33331FF9C^0'

'-624DD2F1A9FBE8^-2'

'-20C49BA5E353F8^-2'

'68DB8BAC710CB4^-2'

'30BC1E6501D784^0'

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'624DD2F1A9FBE8^-2'

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'-624DD2F1A9FBE8^-2'

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'346DC5D638865A^-2'

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'6951712AF6D2B^0'

'-1DD438BB7034B6^0'

'E237351C51E5E8^0'

'-346DC5D638865A^-2'

'3AFB7E90FF9726^-2'

'0^0'

'30D0A2605FB4DC^0'

'69840F7B59C4E^0'

'-1DCA8298A37CC5^0'

'E21FB469855F58^0'

'624DD2F1A9FBE8^-2'

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'30D50B5552FDC2^0'

'69B691E9E4A8E4^0'

'-1DC0C2EFBC53C6^0'

'E20870B0AD27D8^0'

'9D495182A9931^-2'

'346DC5D638865A^-2'

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'-1C0442D0E56042^-2'

'7B35295E9E1B0C^-3'

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'35FAD331^8'

'35FAD3320CCCCC^8'

'35FAD3340CCCCC^8'

'35FAD3360CCCCC^8'

'35FAD3380CCCCC^8'

'35FAD33A0CCCCC^8'

'35FAD33C0CCCCC^8'

'35FAD33E0CCCCC^8'

'35FAD3400CCCCC^8'

'35FAD342^8'

'35FAD331^8'

'1^1'

'A^1'

END_ARRAY 1 83

TOTAL_ARRAYS 1

 ~NAIF/SPC BEGIN COMMENTS~

This CK is for testing with the image: /users/arsanders/pds/kaguya_mi/MNA_2B2_01_04192S136E3573.cub



This CK was generated using the following command: {}

 ~NAIF/SPC END COMMENTS~