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<Product_Observational
   xmlns="http://pds.nasa.gov/pds4/pds/v1"
   xmlns:msn="http://pds.nasa.gov/pds4/msn/v1"
   xmlns:pds="http://pds.nasa.gov/pds4/pds/v1"
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      https://pds.nasa.gov/pds4/msn/v1/PDS4_MSN_1K00_1300.xsd
     ">
    <Identification_Area>
        <logical_identifier>urn:nasa:pds:cassini-mag-cal:data-full-j3:00341_fgm_j3</logical_identifier>
        <version_id>1.0</version_id>
        <title>Cassini MAG Calibrated Full Res. Data in J3 Coords. 2000-12-06</title>
        <information_model_version>1.20.0.0</information_model_version>
        <product_class>Product_Observational</product_class>
        <Citation_Information>
            <author_list>Dougherty, Michele K.; Kellock, Stephen; Slootweg, A. Peter; Achilleos, Nicholas; Joy, Steven P.; Mafi, Joseph N.</author_list>
            <publication_year>2023</publication_year>
            <description>
                Cassini magnetic-field data in the highest time resolution          
                available, from the Fluxgate Magnetometer (FGM) instrument, 
                for 2000-12-06 (341) in J3 coordinates.
            </description>
        </Citation_Information>
        <Modification_History>
            <Modification_Detail>
                <modification_date>2023-10-27</modification_date>
                <version_id>1.0</version_id>
                <description>
                    This data file, 00341_FGM_J3.TAB, was originally not a part of the PDS3 
                    CO-E/SW/J/S-MAG-3-RDR-FULL-RES-V2.0 dataset like other data products in this collection.  
                    The meta-data have been migrated to PDS4.
                </description>
            </Modification_Detail>
        </Modification_History>
    </Identification_Area>
    <Observation_Area>
        <Time_Coordinates>
            <start_date_time>2000-12-06T00:02:40.130Z</start_date_time>
            <stop_date_time>2000-12-07T00:00:38.401Z</stop_date_time> 
        </Time_Coordinates>
        <Primary_Result_Summary>
            <purpose>Science</purpose>
            <processing_level>Calibrated</processing_level>
            <Science_Facets>
                <discipline_name>Fields</discipline_name>
                <facet1>Magnetic</facet1>
                <facet2>Background</facet2>
            </Science_Facets>
        </Primary_Result_Summary>
        <Investigation_Area>
                <name>Cassini-Huygens</name>
                <type>Mission</type>
                <Internal_Reference>
                    <lid_reference>urn:nasa:pds:context:investigation:mission.cassini-huygens</lid_reference>
                    <reference_type>data_to_investigation</reference_type>
                </Internal_Reference>
            </Investigation_Area>
            <Observing_System>
                <Observing_System_Component>
                    <name>Cassini Orbiter</name>
                    <type>Host</type>
                    <Internal_Reference>
                        <lid_reference>urn:nasa:pds:context:instrument_host:spacecraft.co</lid_reference>
                        <reference_type>is_instrument_host</reference_type>
                    </Internal_Reference>
                </Observing_System_Component>
                <Observing_System_Component>
                    <name>Dual Technique Magnetometer</name>
                    <type>Instrument</type>
                    <Internal_Reference>
                        <lid_reference>urn:nasa:pds:context:instrument:mag.co</lid_reference>
                        <reference_type>is_instrument</reference_type>
                    </Internal_Reference>
                </Observing_System_Component> 
            </Observing_System>
            <Target_Identification>
                <name>Jupiter</name>
                <type>Planet</type>
                <Internal_Reference>
                    <lid_reference>urn:nasa:pds:context:target:planet.jupiter</lid_reference>
                    <reference_type>data_to_target</reference_type>
                </Internal_Reference>
            </Target_Identification>
            <Target_Identification>
                <name>Solar Wind</name>
                <type>Plasma Stream</type>
                <Internal_Reference>
                    <lid_reference>urn:nasa:pds:context:target:plasma_stream.solar_wind</lid_reference>
                    <reference_type>data_to_target</reference_type>
                </Internal_Reference>
            </Target_Identification>
        <Discipline_Area>
            <msn:Mission_Information>
                <msn:mission_phase_name>Outer Cruise</msn:mission_phase_name>
            </msn:Mission_Information>
            <msn:Mission_Information>
                <msn:spacecraft_clock_start>1/1354752843.075</msn:spacecraft_clock_start>
                <msn:spacecraft_clock_stop>1/1354839122.041</msn:spacecraft_clock_stop>
                <msn:spacecraft_clock_partition>1</msn:spacecraft_clock_partition>
            </msn:Mission_Information>
        </Discipline_Area>        
    </Observation_Area>
    <Reference_List>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:cassini-mag-cal:document:data-full-j3-desc</lid_reference>
            <reference_type>data_to_document</reference_type>
            <comment>
                Document containing a description of the Cassini MAG 
                Calibrated Full Res. Data in J3 Coords. Collection.
            </comment>
        </Internal_Reference>
        <External_Reference>
            <doi>10.17189/1520114</doi>
            <reference_text>
                Elson, L.S., C.H. Acton, D.L. Conner and B.V. Semenov, Cassini
                SPICE Kernels V1.0, CO-S/J/E/V-SPICE-6-V1.0, NASA Planetary Data
                System, 2005. https://doi.org/10.17189/1520114
            </reference_text>
            <description>
                This product was processed using the following kernels using the data set
                referenced above:

                SPICE spacecraft orientation kernels:
                00334_00344ra.bc

                Leapsecond (LSK) kernels:
                naif0012.tls

                PCK kernels:
                cpck15Dec2017.tpc

                Spacecraft clock kernels:
                cas00172.tsc
            </description>
        </External_Reference>
    </Reference_List>
    <File_Area_Observational>
        <File>
            <file_name>00341_FGM_J3.TAB</file_name>
            <creation_date_time>2019-06-03T14:59:22.000Z</creation_date_time>
            <file_size unit="byte">61194176</file_size>
            <md5_checksum>94d9ffb7072b85a9de46a8782d1abb66</md5_checksum>
            <comment>
      J3 (IAU_JUPITER) is a Jovicentric cartesian coordinate system 
      consistent with the IAU 1997 definition of the System 3 prime meridian. 
      It consists of X (in Jovian equatorial plane, along S3 1997 prime meridian), 
      Y (completes right handed set), and Z (parallel to the Jovian spin axis).
      
      These MAG data were processed (calibrated, and rotated into J3        
      coordinates) by the Cassini MAG team at Imperial College. They were     
      acquired by the PDS PPI node at UCLA where they were converted from     
      binary to ASCII, and the B-field magnitude, and position data removed. These
      data have been processed using an updated calibration that was produced using 
      the Proximal Orbit data. 
      
      Note that some of the data files from this data set contain timing errors. 
      This file, however, contains no identified timing errors. 
      
      For more information on the timing errors, and on this and previous versions of 
      the data, please refer to the collection description document (data-full-j3-desc.txt).
                
      These spice kernels were used to process these data but are not archived:
      171215R_SCPSEops_97288_17258.bsp
            </comment>
        </File>
        <Table_Character>
            <offset unit="byte">0</offset>
            <records>1055072</records>
            <record_delimiter>Carriage-Return Line-Feed</record_delimiter>
            <Record_Character>
                <fields>4</fields>
                <groups>0</groups>
                <record_length unit="byte">58</record_length>
                <Field_Character>
                    <name>TIME</name>
                    <field_number>1</field_number>
                    <field_location unit="byte">1</field_location>
                    <data_type>ASCII_Date_Time_YMD</data_type>
                    <field_length unit="byte">23</field_length>  
                    <description>                                             
      Spacecraft event time of the sample.
                    </description>
                </Field_Character>
                <Field_Character>
                    <name>BX</name>
                    <field_number>2</field_number>
                    <field_location unit="byte">25</field_location>
                    <data_type>ASCII_Real</data_type>
                    <field_length unit="byte">10</field_length>  
                    <unit>nT</unit>
                    <description>                                             
      J3 X component of the magnetic-field component in nT.                   
      X is in the Jovian equatorial plane along the line through the          
      System 3 (1997), positive away from Jupiter.
                    </description>
                    <Special_Constants>
                        <valid_maximum>44000.000</valid_maximum> 
                        <valid_minimum>-44000.000</valid_minimum>
                    </Special_Constants>
                </Field_Character>
                <Field_Character>
                    <name>BY</name>
                    <field_number>3</field_number>
                    <field_location unit="byte">36</field_location>
                    <data_type>ASCII_Real</data_type>
                    <field_length unit="byte">10</field_length>  
                    <unit>nT</unit>
                    <description>                                             
      J3 Y component of the magnetic field component in nT.                   
      Y completes the right handed set (Z x X).
                    </description>
                    <Special_Constants>
                        <valid_maximum>44000.000</valid_maximum> 
                        <valid_minimum>-44000.000</valid_minimum>
                    </Special_Constants>
                </Field_Character>
                <Field_Character>
                    <name>BZ</name>
                    <field_number>4</field_number>
                    <field_location unit="byte">47</field_location>
                    <data_type>ASCII_Real</data_type>
                    <field_length unit="byte">10</field_length>  
                    <unit>nT</unit>
                    <description>                                             
      J3 Z component of the magnetic field component in nT.                   
      Z is parallel to Jovian spin axis, Omega, positive north of             
      the equator.
                    </description>
                    <Special_Constants>
                        <valid_maximum>44000.000</valid_maximum> 
                        <valid_minimum>-44000.000</valid_minimum>
                    </Special_Constants>
                </Field_Character>
            </Record_Character>
            </Table_Character>
    </File_Area_Observational> 
</Product_Observational>
