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Add new attributes for some L'LORRI CDP keywords (#9)
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* Add Radiometric_Conversion_Constants class and associated children
* Auto-generated LDDs by PDSEN CI Bot
* Add a missing factor of "1/pixel" to diffuse source units
* Auto-generated LDDs by PDSEN CI Bot
* Add attributes for L'LORRI detector parameters (gain, bias, etc.)
* Auto-generated LDDs by PDSEN CI Bot
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@cgobat
cgobat authored Aug 20, 2024
1 parent eb74b88 commit 0ad16d6
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1 change: 0 additions & 1 deletion build/development/afc8a7fa0a46780780f48e6059dffc6e1d0c1c11/1.18.0.0/PDS4_LUCY_1I00_1000.JSON
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24 changes: 24 additions & 0 deletions ...1d0c1c11/1.18.0.0/PDS4_LUCY_1I00_1000.csv → ...9ac289ed/1.18.0.0/PDS4_LUCY_1I00_1000.csv
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"Sort Key","Type","Name","Version","Name Space Id","Description","Steward","Value Type","Minimum Cardinality","Maximum Cardinality","Minimum Value","Maximum Value","Minimum Characters","Maximum Characters","Unit of Measure Type","Specified Unit Id","Attribute Concept","Conceptual Domain"
"lucy:Diffuse_Source:1 ","Class","Diffuse_Source","1.0.0.0","lucy"," The lucy:Point_Source class presents radiometric conversion constants for converting calibrated pixel values into physical units for resolved/extended sources. ","katecrombie","","","","","","","","","","",""
"lucy:Diffuse_Source:2 lucy:units_of_conversion_constants:1 ","Attribute","units_of_conversion_constants","n/a","lucy"," For resolved sources, the radiometric conversion produces data in units of radiance. For unresolved sources, the conversion results in units of flux (irradiance). The lucy:units_of_conversion_constants attribute contains the appropriate physical units for the conversion constants in the class in which it is contained to produce either radiance or flux units, as appropriate, when the conversion is applied. ","katecrombie","ASCII_Short_String_Collapsed","1","1","Unbounded","Unbounded","1","255","Units_of_None","none","TBD_classConcept","SHORT_STRING"
"lucy:Diffuse_Source:2 lucy:units_of_conversion_constants:2 Value:(DN/s)/(erg/cm^2/s/A","Value","(DN/s)/(erg/cm^2/s/Angstrom)","",""," Units for conversion factors for unresolved (point) sources, to produce units of flux (irradiance). "
"lucy:Diffuse_Source:2 lucy:units_of_conversion_constants:2 Value:(DN/s/pixel)/(erg/cm","Value","(DN/s/pixel)/(erg/cm^2/s/Angstrom/sr)","",""," Units for conversion factors for resolved (diffuse) sources, to produce units of radiance. "
"lucy:Diffuse_Source:2 lucy:solar_constant:1 ","Attribute","solar_constant","n/a","lucy"," The lucy:solar_constant attribute supplies the constant to be used for sources with a spectral distribution similar to the Sun to convert calibrated pixel values to physical units. ","katecrombie","ASCII_Real","1","1","-1.7976931348623157e308","1.7976931348623157e308","Unbounded","Unbounded","Units_of_None","none","TBD_classConcept","REAL"
"lucy:Diffuse_Source:2 lucy:red_trojan_constant:1 ","Attribute","red_trojan_constant","n/a","lucy"," The lucy:red_trojan_constant attribute supplies the constant to be used for sources with a spectral distribution similar to that of ""red"" Trojans to convert calibrated pixel values to physical units. ","katecrombie","ASCII_Real","1","1","-1.7976931348623157e308","1.7976931348623157e308","Unbounded","Unbounded","Units_of_None","none","TBD_classConcept","REAL"
"lucy:Diffuse_Source:2 lucy:gray_trojan_constant:1 ","Attribute","gray_trojan_constant","n/a","lucy"," The lucy:gray_trojan_constant attribute supplies the constant to be used for sources with a spectral distribution similar to that of ""gray"" Trojans to convert calibrated pixel values to physical units. ","katecrombie","ASCII_Real","1","1","-1.7976931348623157e308","1.7976931348623157e308","Unbounded","Unbounded","Units_of_None","none","TBD_classConcept","REAL"
"lucy:Diffuse_Source:2 lucy:dinkinesh_constant:1 ","Attribute","dinkinesh_constant","n/a","lucy"," The lucy:dinkinesh_constant attribute supplies the constant to be used for sources with a spectral distribution similar to that of Dinkinesh to convert calibrated pixel values to physical units. ","katecrombie","ASCII_Real","0","1","-1.7976931348623157e308","1.7976931348623157e308","Unbounded","Unbounded","Units_of_None","none","TBD_classConcept","REAL"
"lucy:Lucy_Observation_Time_Information:1","Class","Lucy_Observation_Time_Information","1.0.0.0","lucy","Lucy Mission observation identification and timing information.","katecrombie","","","","","","","","","","",""
"lucy:Lucy_Observation_Time_Information:2 lucy:observation_id:1 ","Attribute","observation_id","n/a","lucy","The Lucy Mission observation identifier. ","katecrombie","ASCII_Integer","1","*","0","99999","Unbounded","Unbounded","Units_of_None","none","TBD_classConcept","INTEGER"
"lucy:Lucy_Observation_Time_Information:2 lucy:observation_id_count:1 ","Attribute","observation_id_count","n/a","lucy","The Lucy Mission observation identifier counter. This number increments by 1 with each planned observation sequence (L'LORRI only). ","katecrombie","ASCII_Integer","0","1","0","99999","Unbounded","Unbounded","Units_of_None","none","TBD_classConcept","INTEGER"
Expand Down Expand Up @@ -63,6 +71,11 @@
"lucy:LLORRI_Instrument_Parameters:2 lucy:latch_count:1 ","Attribute","latch_count","n/a","lucy","The number of times a latchup has occurred.","katecrombie","ASCII_Integer","0","1","0","9223372036854775807","Unbounded","Unbounded","Units_of_None","none","TBD_classConcept","INTEGER"
"lucy:LLORRI_Instrument_Parameters:2 lucy:calibration_lamp_level_1:1 ","Attribute","calibration_lamp_level_1","n/a","lucy","The Digital Number (DN) setting for calibration lamp one.","katecrombie","ASCII_Integer","0","1","-9223372036854775808","9223372036854775807","Unbounded","Unbounded","Units_of_Misc","none","TBD_classConcept","INTEGER"
"lucy:LLORRI_Instrument_Parameters:2 lucy:calibration_lamp_level_2:1 ","Attribute","calibration_lamp_level_2","n/a","lucy","The Digital Number (DN) setting for calibration lamp two.","katecrombie","ASCII_Integer","0","1","-9223372036854775808","9223372036854775807","Unbounded","Unbounded","Units_of_Misc","none","TBD_classConcept","INTEGER"
"lucy:LLORRI_Instrument_Parameters:2 lucy:bias_level:1 ","Attribute","bias_level","n/a","lucy","The lucy:bias_level attribute appears in calibrated L'LORRI data products and contains the mean bias level of the detector's dark columns.","katecrombie","ASCII_Real","0","1","0","1.7976931348623157e308","Unbounded","Unbounded","Units_of_Misc","none","TBD_classConcept","REAL"
"lucy:LLORRI_Instrument_Parameters:2 lucy:read_noise:1 ","Attribute","read_noise","n/a","lucy","The lucy:read_noise attribute appears in calibrated L'LORRI data products and provides the CCD read noise for the image.","katecrombie","ASCII_Real","0","1","0","1.7976931348623157e308","Unbounded","Unbounded","Units_of_Misc","none","TBD_classConcept","REAL"
"lucy:LLORRI_Instrument_Parameters:2 lucy:ccd_gain:1 ","Attribute","ccd_gain","n/a","lucy","The lucy:ccd_gain attribute appears in calibrated L'LORRI data products and provides the CCD gain setting for the image.","katecrombie","ASCII_Real","0","1","0","1.7976931348623157e308","Unbounded","Unbounded","Units_of_Misc","none","TBD_classConcept","REAL"
"lucy:LLORRI_Instrument_Parameters:2 lucy:bias_offset:1 ","Attribute","bias_offset","n/a","lucy","The lucy:bias_offset attribute appears in calibrated L'LORRI data products and provides the CCD bias offset between the active and inactive regions of the detector.","katecrombie","ASCII_Real","0","1","0","1.7976931348623157e308","Unbounded","Unbounded","Units_of_Misc","none","TBD_classConcept","REAL"
"lucy:LLORRI_Instrument_Parameters:2 lucy:frame_transfer_scrub_time:1 ","Attribute","frame_transfer_scrub_time","n/a","lucy"," The lucy:frame_transfer_scrub_time attribute appears in calibrated L'LORRI data products and contains the instrument's frame transfer/scrub time. For the L'LORRI instrument, these two quantities (transfer and scrub times) are exactly equal. ","katecrombie","ASCII_Real","0","1","11.0","12.0","Unbounded","Unbounded","Units_of_Time","none","TBD_classConcept","REAL"
"lucy:LRalph_Instrument_Common_Parameters:1","Class","LRalph_Instrument_Common_Parameters","1.0.0.0","lucy","The Lucy LRalph instrument class that contains the common (LEISA and MVIC) instrument specific attributes relevant to the labeled data product.","katecrombie","","","","","","","","","","",""
"lucy:LRalph_Instrument_Common_Parameters:2 lucy:playback_start:1 ","Attribute","playback_start","n/a","lucy","Playback science header timstamp of the first m4 packet used in spacecraft clock seconds.","katecrombie","ASCII_Integer","0","1","-9223372036854775808","9223372036854775807","Unbounded","Unbounded","Units_of_Time","none","TBD_classConcept","INTEGER"
"lucy:LRalph_Instrument_Common_Parameters:2 lucy:playback_end:1 ","Attribute","playback_end","n/a","lucy","Playback science header timstamp of the last m4 packet used in spacecraft clock seconds.","katecrombie","ASCII_Integer","0","1","-9223372036854775808","9223372036854775807","Unbounded","Unbounded","Units_of_Time","none","TBD_classConcept","INTEGER"
Expand Down Expand Up @@ -128,3 +141,14 @@
"lucy:MVIC_Instrument_Parameters:2 lucy:mvic_fpe_vis_temperature:1 ","Attribute","mvic_fpe_vis_temperature","n/a","lucy","The MVIC FPE VIS Temperature","katecrombie","ASCII_Real","0","1","-1.7976931348623157e308","1.7976931348623157e308","Unbounded","Unbounded","Units_of_Temperature","none","TBD_classConcept","REAL"
"lucy:MVIC_Instrument_Parameters:2 lucy:mvic_observation_allocation:1 ","Attribute","mvic_observation_allocation","n/a","lucy","MVIC allocated observation duration","katecrombie","ASCII_Real","0","1","-1.7976931348623157e308","1.7976931348623157e308","Unbounded","Unbounded","Units_of_Time","none","TBD_classConcept","REAL"
"lucy:MVIC_Instrument_Parameters:2 lucy:mvic_tdi_row_integration_time:1 ","Attribute","mvic_tdi_row_integration_time","n/a","lucy","MVIC allocated observation duration","katecrombie","ASCII_Real","0","1","-1.7976931348623157e308","1.7976931348623157e308","Unbounded","Unbounded","Units_of_Time","none","TBD_classConcept","REAL"
"lucy:Point_Source:1 ","Class","Point_Source","1.0.0.0","lucy"," The lucy:Point_Source class presents radiometric conversion constants for converting calibrated pixel values into physical units for unresolved/point sources. ","katecrombie","","","","","","","","","","",""
"lucy:Point_Source:2 lucy:units_of_conversion_constants:1 ","Attribute","units_of_conversion_constants","n/a","lucy"," For resolved sources, the radiometric conversion produces data in units of radiance. For unresolved sources, the conversion results in units of flux (irradiance). The lucy:units_of_conversion_constants attribute contains the appropriate physical units for the conversion constants in the class in which it is contained to produce either radiance or flux units, as appropriate, when the conversion is applied. ","katecrombie","ASCII_Short_String_Collapsed","1","1","Unbounded","Unbounded","1","255","Units_of_None","none","TBD_classConcept","SHORT_STRING"
"lucy:Point_Source:2 lucy:units_of_conversion_constants:2 Value:(DN/s)/(erg/cm^2/s/A","Value","(DN/s)/(erg/cm^2/s/Angstrom)","",""," Units for conversion factors for unresolved (point) sources, to produce units of flux (irradiance). "
"lucy:Point_Source:2 lucy:units_of_conversion_constants:2 Value:(DN/s/pixel)/(erg/cm","Value","(DN/s/pixel)/(erg/cm^2/s/Angstrom/sr)","",""," Units for conversion factors for resolved (diffuse) sources, to produce units of radiance. "
"lucy:Point_Source:2 lucy:solar_constant:1 ","Attribute","solar_constant","n/a","lucy"," The lucy:solar_constant attribute supplies the constant to be used for sources with a spectral distribution similar to the Sun to convert calibrated pixel values to physical units. ","katecrombie","ASCII_Real","1","1","-1.7976931348623157e308","1.7976931348623157e308","Unbounded","Unbounded","Units_of_None","none","TBD_classConcept","REAL"
"lucy:Point_Source:2 lucy:red_trojan_constant:1 ","Attribute","red_trojan_constant","n/a","lucy"," The lucy:red_trojan_constant attribute supplies the constant to be used for sources with a spectral distribution similar to that of ""red"" Trojans to convert calibrated pixel values to physical units. ","katecrombie","ASCII_Real","1","1","-1.7976931348623157e308","1.7976931348623157e308","Unbounded","Unbounded","Units_of_None","none","TBD_classConcept","REAL"
"lucy:Point_Source:2 lucy:gray_trojan_constant:1 ","Attribute","gray_trojan_constant","n/a","lucy"," The lucy:gray_trojan_constant attribute supplies the constant to be used for sources with a spectral distribution similar to that of ""gray"" Trojans to convert calibrated pixel values to physical units. ","katecrombie","ASCII_Real","1","1","-1.7976931348623157e308","1.7976931348623157e308","Unbounded","Unbounded","Units_of_None","none","TBD_classConcept","REAL"
"lucy:Point_Source:2 lucy:dinkinesh_constant:1 ","Attribute","dinkinesh_constant","n/a","lucy"," The lucy:dinkinesh_constant attribute supplies the constant to be used for sources with a spectral distribution similar to that of Dinkinesh to convert calibrated pixel values to physical units. ","katecrombie","ASCII_Real","0","1","-1.7976931348623157e308","1.7976931348623157e308","Unbounded","Unbounded","Units_of_None","none","TBD_classConcept","REAL"
"lucy:Radiometric_Conversion_Constants:1","Class","Radiometric_Conversion_Constants","1.0.0.0","lucy"," The lucy:Radiometric_Conversion_Constants class provides the values needed to perform the conversion from the calibrated pixel values to physical units. This conversion is dependent on the spectral distribition of the source, the detector wavelength range, and whether or not the source is resolved. A description of how to convert from data values to physical units is provided in the LLORRI SIS document. ","katecrombie","","","","","","","","","","",""
"lucy:Radiometric_Conversion_Constants:2 lucy:pivot_wavelength:1 ","Attribute","pivot_wavelength","n/a","lucy"," The value contained in the lucy:pivot_wavelength attribute is used when converting L'LORRI calibrated pixel values to physical units. ","katecrombie","ASCII_Real","1","1","0.0","1.7976931348623157e308","Unbounded","Unbounded","Units_of_Length","none","TBD_classConcept","REAL"
"lucy:Radiometric_Conversion_Constants:2 lucy:photometric_zero_point:1 ","Attribute","photometric_zero_point","n/a","lucy"," The lucy:photometric_zero_point attribute supplies the photometric zero point to be used to convert between units of (ir)radiance and visual magnitude, V. ","katecrombie","ASCII_Real","1","1","-1.7976931348623157e308","1.7976931348623157e308","Unbounded","Unbounded","Units_of_None","none","TBD_classConcept","REAL"
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