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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-rtn:00341_fgm_rtn</logical_identifier>
        <version_id>1.0</version_id>
        <title>Cassini MAG Calibrated Full Res. Data in RTN 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 RTN coordinates.
            </description>
        </Citation_Information>
        <Modification_History>
            <Modification_Detail>
                <modification_date>2023-11-09</modification_date>
                <version_id>1.0</version_id>
                <description>
                    This data file, 00341_FGM_RTN.TAB, was originally archived as part of the PDS3 
                    CO-E/SW/J/S-MAG-3-RDR-FULL-RES-V2.0 dataset.
                </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-rtn-desc</lid_reference>
            <reference_type>data_to_document</reference_type>
            <comment>
                Document containing a description of the Cassini MAG
                Calibrated Full Res. Data in RTN 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>
        <Source_Product_External>
            <external_source_product_identifier>CO-E/SW/J/S-MAG-3-RDR-FULL-RES-V2.0:00341_FGM_RTN:00341_FGM_RTN.TAB</external_source_product_identifier>
            <reference_type>data_to_calibrated_source_product</reference_type>
            <doi>10.17189/1521151</doi>
            <curating_facility>PDS Planetary Plasma Interactions Node</curating_facility>
            <description>
                This is the first version converted to PDS4. The DOI provided
                references the PDS3 source data set. 
            </description>
        </Source_Product_External>
    </Reference_List>
    <File_Area_Observational>
        <File>
            <file_name>00341_FGM_RTN.TAB</file_name>
            <creation_date_time>2019-06-03T14:44:59.000Z</creation_date_time>
            <file_size unit="byte">61194176</file_size>
            <md5_checksum>525e9544fb7aeaeb5a3188d06e4ba5d0</md5_checksum>
            <comment>
                RTN coordinates consist of R (radial component, Sun to the 
      spacecraft), T (tangential component, parallel to the Solar Equatorial 
      plane and perpendicular to R), and N (normal component, completes right 
      handed set).
                
      These MAG data were processed (calibrated, and rotated into RTN        
      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 collection contained 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-rtn-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>BR</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>                                             
      RTN radial component of the magnetic-field component in nT.             
      The radial component (R) points from the Sun to the spacecraft,         
      positive away from the Sun.
                        </description>
                        <Special_Constants>
                            <valid_maximum>44000.000</valid_maximum> 
                            <valid_minimum>-44000.000</valid_minimum>
                        </Special_Constants>
                    </Field_Character>
                    <Field_Character>
                        <name>BT</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>                                             
      RTN tangential component of the magnetic field component in nT.         
      The tangential component (T) is parallel to the Solar Equatorial        
      plane (Omega Sun x R).
                        </description>
                        <Special_Constants>
                            <valid_maximum>44000.000</valid_maximum> 
                            <valid_minimum>-44000.000</valid_minimum>
                        </Special_Constants>
                    </Field_Character>
                    <Field_Character>
                        <name>BN</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>                                             
      RTN normal component of the magnetic field component in nT.             
      The normal component (N) completes the right handed set, and            
      is roughly normal to the Solar Equatorial plane (R x Phi).
                        </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>
