diff --git a/ale/drivers/selene_drivers.py b/ale/drivers/selene_drivers.py
index bad772432016753ed25c2c5312e67b3d61f69cdb..ba7eff426d872ecbc446c4d15842ba5d790e7c7d 100644
--- a/ale/drivers/selene_drivers.py
+++ b/ale/drivers/selene_drivers.py
@@ -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'])
diff --git a/tests/pytests/data/MNA_2B2_01_04192S136E3573/MNA_2B2_01_04192S136E3573_0.xsp b/tests/pytests/data/MNA_2B2_01_04192S136E3573/MNA_2B2_01_04192S136E3573_0.xsp
new file mode 100644
index 0000000000000000000000000000000000000000..2d06eb51a0cf38cc0680235e1cb9868db206788f
--- /dev/null
+++ b/tests/pytests/data/MNA_2B2_01_04192S136E3573/MNA_2B2_01_04192S136E3573_0.xsp
@@ -0,0 +1,284 @@
+DAFETF NAIF DAF ENCODED TRANSFER FILE
+'DAF/SPK '
+'2'
+'6'
+'SPKMERGE '
+BEGIN_ARRAY 1 45
+'DE-0421LE-0421 '
+'106224BBF61FD^8'
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+'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_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
+ INCLUDE_COMMENTS = NO
+ BODIES = 3, 10, 301
+ BEGIN_TIME = 2008 SEP 16 20:02:02.779
+ END_TIME = 2008 SEP 16 20:02:19.045
+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 20:02:02.779
+ END_TIME = 2008 SEP 16 20:02:19.045
+
+; END SPKMERGE COMMANDS
+ ~NAIF/SPC END COMMENTS~
diff --git a/tests/pytests/data/MNA_2B2_01_04192S136E3573/MNA_2B2_01_04192S136E3573_1.xsp b/tests/pytests/data/MNA_2B2_01_04192S136E3573/MNA_2B2_01_04192S136E3573_1.xsp
new file mode 100644
index 0000000000000000000000000000000000000000..1cc733dfa9f02f078ab06e8e0f16d49211e339ea
--- /dev/null
+++ b/tests/pytests/data/MNA_2B2_01_04192S136E3573/MNA_2B2_01_04192S136E3573_1.xsp
@@ -0,0 +1,284 @@
+DAFETF NAIF DAF ENCODED TRANSFER FILE
+'DAF/SPK '
+'2'
+'6'
+'SPKMERGE '
+BEGIN_ARRAY 1 45
+'DE-0421LE-0421 '
+'106226B2B0BF8E^8'
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+; /users/arsanders/pds/kaguya_mi/out/MNA_2B2_01_04192S136E3573_1.bsp LOG FILE
+
+; Created 2022-01-12/22:33:34.00.
+;
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+
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+
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+ END_TIME = 2008 SEP 16 20:10:40.793
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+ 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~
diff --git a/tests/pytests/data/MNA_2B2_01_04192S136E3573/MNA_2B2_01_04192S136E3573_isis3.lbl b/tests/pytests/data/MNA_2B2_01_04192S136E3573/MNA_2B2_01_04192S136E3573_isis3.lbl
new file mode 100644
index 0000000000000000000000000000000000000000..62856b59f4ebf7630a111038607477a01869ce57
--- /dev/null
+++ b/tests/pytests/data/MNA_2B2_01_04192S136E3573/MNA_2B2_01_04192S136E3573_isis3.lbl
@@ -0,0 +1,447 @@
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diff --git a/tests/pytests/data/MNA_2B2_01_04192S136E3573/SEL_M_ALL_D_V02_0_sliced_-131000.xc b/tests/pytests/data/MNA_2B2_01_04192S136E3573/SEL_M_ALL_D_V02_0_sliced_-131000.xc
new file mode 100644
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+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~
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new file mode 100644
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+This CK was generated using the following command: {}
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index d5217c172df4fc2339263902ac94738e14948699..d7eda47ba946c2f7e2c161dc8a2182c24dd79051 100644
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diff --git a/tests/pytests/test_kaguya_drivers.py b/tests/pytests/test_kaguya_drivers.py
index 3b8b70bd9b600512370d2a24047739ab27fde7a5..50ebe3b766020e78952a565f635f0f94d76ad747 100644
--- a/tests/pytests/test_kaguya_drivers.py
+++ b/tests/pytests/test_kaguya_drivers.py
@@ -13,11 +13,11 @@ from conftest import get_isd, get_image_label, get_image_kernels, convert_kernel
import ale
-from ale.drivers.selene_drivers import KaguyaTcPds3NaifSpiceDriver
+from ale.drivers.selene_drivers import KaguyaTcPds3NaifSpiceDriver, KaguyaMiIsisLabelNaifSpiceDriver
image_dict = {
'TC1S2B0_01_06691S820E0465' : get_isd("kaguyatc"),
- 'MVA_2B2_01_02329N002E0302' : get_isd("kaguyami")
+ 'MNA_2B2_01_04192S136E3573' : get_isd("kaguyami")
}
@@ -33,9 +33,13 @@ def test_kernels():
for kern in kern_list:
os.remove(kern)
-@pytest.mark.parametrize("label_type", ['pds3'])
-@pytest.mark.parametrize("image", image_dict.keys())
+@pytest.mark.xfail()
+@pytest.mark.parametrize("label_type", ['pds3', 'isis3'])
def test_kaguya_load(test_kernels, label_type, image):
+ if label_type == 'pds3':
+ image = 'TC1S2B0_01_06691S820E0465'
+ else:
+ image = 'MNA_2B2_01_04192S136E3573'
label_file = get_image_label(image, label_type)
isd_str = ale.loads(label_file, props={'kernels': test_kernels[image]})
@@ -123,3 +127,67 @@ class test_pds_naif(unittest.TestCase):
def test_spacecraft_direction(self):
assert self.driver.spacecraft_direction == 1
+
+# ========= Test kaguyami isis3label and naifspice driver =========
+class test_kaguyami_isis3_naif(unittest.TestCase):
+
+ def setUp(self):
+ label = get_image_label("MNA_2B2_01_04192S136E3573", "isis3")
+ self.driver = KaguyaMiIsisLabelNaifSpiceDriver(label)
+
+ def test_instrument_id(self):
+ assert self.driver.instrument_id == 'LISM_MI-NIR1'
+
+ def test_sensor_frame_id(self):
+ with patch('ale.drivers.selene_drivers.spice.namfrm', return_value=12345) as namfrm:
+ assert self.driver.sensor_frame_id == 12345
+ namfrm.assert_called_with('LISM_MI_N_HEAD')
+
+ def test_ikid(self):
+ with patch('ale.drivers.selene_drivers.spice.bods2c', return_value=12345) as bods2c:
+ assert self.driver.ikid == 12345
+ bods2c.assert_called_with('LISM_MI-NIR1')
+
+ def test_spacecraft_name(self):
+ assert self.driver.spacecraft_name == 'KAGUYA'
+
+ def test_spacecraft_clock_start_count(self):
+ assert self.driver.spacecraft_clock_start_count == 905631021.135959
+
+ def test_spacecraft_clock_stop_count(self):
+ assert self.driver.spacecraft_clock_stop_count == 905631033.576935
+
+ def test_ephemeris_start_time(self):
+ with patch('ale.drivers.selene_drivers.spice.sct2e', return_value=12345) as sct2e, \
+ patch('ale.drivers.selene_drivers.spice.bods2c', return_value=-12345) as bods2c:
+ assert self.driver.ephemeris_start_time == 12345
+ sct2e.assert_called_with(-12345, 905631021.135959)
+
+ def test_detector_center_line(self):
+ with patch('ale.drivers.selene_drivers.spice.gdpool', return_value=np.array([54321, 12345])) as gdpool, \
+ patch('ale.drivers.selene_drivers.spice.bods2c', return_value=-12345) as bods2c:
+ assert self.driver.detector_center_line == 12344.5
+ gdpool.assert_called_with('INS-12345_CENTER', 0, 2)
+
+ def test_detector_center_sample(self):
+ with patch('ale.drivers.selene_drivers.spice.gdpool', return_value=np.array([54321, 12345])) as gdpool, \
+ patch('ale.drivers.selene_drivers.spice.bods2c', return_value=-12345) as bods2c:
+ assert self.driver.detector_center_sample == 54320.5
+ gdpool.assert_called_with('INS-12345_CENTER', 0, 2)
+
+ def test_focal2pixel_samples(self):
+ with patch('ale.drivers.selene_drivers.spice.gdpool', return_value=np.array([2])) as gdpool, \
+ patch('ale.drivers.selene_drivers.spice.bods2c', return_value=-12345) as bods2c:
+ assert self.driver.focal2pixel_samples == [0, 0, -1/2]
+ gdpool.assert_called_with('INS-12345_PIXEL_SIZE', 0, 1)
+
+ def test_focal2pixel_lines(self):
+ with patch('ale.drivers.selene_drivers.spice.gdpool', return_value=np.array([2])) as gdpool, \
+ patch('ale.drivers.selene_drivers.spice.bods2c', return_value=-12345) as bods2c, \
+ patch('ale.drivers.selene_drivers.KaguyaTcPds3NaifSpiceDriver.spacecraft_direction', \
+ new_callable=PropertyMock) as spacecraft_direction:
+ spacecraft_direction.return_value = 1
+ assert self.driver.focal2pixel_lines == [0, 1/2, 0]
+ spacecraft_direction.return_value = -1
+ assert self.driver.focal2pixel_lines == [0, 1/2, 0]
+ gdpool.assert_called_with('INS-12345_PIXEL_SIZE', 0, 1)