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        <logical_identifier>urn:nasa:pds:nh_pepssi:kem1cruise_raw</logical_identifier>
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        <title>New Horizons Pluto Energetic Particle Spectrometer Science Investigation KEM1 Cruise Raw Data</title>
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        <Citation_Information>
            <author_list>McNutt, R. Jr.</author_list>
            <editor_list>Sharkey, Benjamin; Gicquel, Adeline; Gobat, Caden; Redfern, Jillian</editor_list>
            <publication_year>2026</publication_year>
            <doi>10.26007/pd9m-8160</doi>
            <description>
                This data set contains Raw data taken by the                     
                New Horizons Pluto Energetic Particle Spectrometer Science Investigation
                instrument during the CRUISE TO FIRST KBO ENCOUNTER mission phase. These data 
                were migrated from the PDS3 dataset: NH-X-PEPSSI-2-KEMCRUISE1-V2.0.      
                
                Some data from PLUTO ENCOUNTER has been included. This is due to data   
                being replayed after the PLUTO ENCOUNTER PDS Deliveries.                
                
                PEPSSI (Pluto Energetic Particles Spectrometer Science Investigation)   
                is a particle telescope and a time-of-flight (TOF) spectrometer that    
                measures ions and electrons over a broad range of energies and          
                angles. Particle composition and energy spectra are measured for H to   
                Fe from ~ 30 keV to ~1 MeV (but not all species are uniquely separated) 
                and for electrons from ~30 keV to 700 keV. PEPSSI comprises a           
                time-of-flight (TOF) section and a solid-state detector (SSD) array     
                that measures particle energy. The combination of measured energy and   
                TOF provides unique particle identification by mass and particle energy 
                depending on the range: for protons from ~30 keV to ~1 MeV; for heavy   
                (CNO) ions from ~80 keV to ~1 MeV. Lower-energy (&gt;3 keV) ion fluxes are 
                measured by TOF only, but without the SSD signal, providing velocity    
                spectra at these energies as well. Due to storage and bandwidth         
                limitations, all event data cannot be stored or telemetered to the      
                ground. Instead, a round-robin algorithm is used to save Energy, TOF,   
                and timing data for select events. The common data products contain     
                these event and summary measurements, accumulated over fixed periods of 
                86,400 seconds, with each period in a single file comprising multiple   
                binary tables.  The documentation provided with this data set describes 
                the data format.                                                        
                
                PEPSSI was powered on for most of the time frame during this mission    
                phase, taking data in its low rate mode. Other than normal operations   
                one EEPROM check was performed.
                
                Labels were redesigned during migration using the .FIT header and PDS3 .LBL
                files, but the data files are unchanged from their PDS3 version.
            </description>
        </Citation_Information>
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                <modification_date>2025-01-28</modification_date>
                <version_id>1.0</version_id>
                <description>Created during PDS4 migration by PDS-SBN (B. Sharkey)</description>
            </Modification_Detail>
        </Modification_History>  
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        <Time_Coordinates>
            <start_date_time>2016-10-22T23:00:00.000Z</start_date_time>
            <stop_date_time>2018-08-13T00:08:02.009Z</stop_date_time>
        </Time_Coordinates>
        <Primary_Result_Summary>
            <purpose>Science</purpose>
            <processing_level>Calibrated</processing_level>
            <Science_Facets>
                <discipline_name>Particles</discipline_name>
                <facet1>Ions</facet1>
                <facet2>Energetic</facet2>
            </Science_Facets>
        </Primary_Result_Summary>
        <Investigation_Area>
            <name>New Horizons Kuiper Belt Extended Mission</name>
            <type>Mission</type>
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            <Observing_System_Component>
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        </Observing_System>
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            <name>Solar Wind</name>
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              <lid_reference>urn:nasa:pds:context:resource:resource.nh_pepssi_colxn_kem1cruise_raw_online</lid_reference>
              <reference_type>has_resource</reference_type>
           </Internal_Reference>
           <Internal_Reference>
            <lidvid_reference>urn:nasa:pds:nh_pepssi:kem1cruise_raw:overview::1.0</lidvid_reference>
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        </Internal_Reference> 
        <Internal_Reference>
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        </Internal_Reference>
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        </Internal_Reference>
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            <lid_reference>urn:nasa:pds:nh_pepssi:kem1cruise_cal</lid_reference>
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            <comment>PEPSSI KEM1 Cruise Calibrated Data Collection</comment>
        </Internal_Reference>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:nh_pepssi:calibration_files</lid_reference>
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            <comment>PEPSSI Calibration Files Collection</comment>
        </Internal_Reference>
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