<?xml version="1.0" encoding="UTF-8"?>
<?xml-model 
    href="https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1J00.sch" 
    schematypens="http://purl.oclc.org/dsdl/schematron"?>
<?xml-model 
    href="https://pds.nasa.gov/pds4/ctli/v2/PDS4_CTLI_1J00_2000.sch"
    schematypens="http://purl.oclc.org/dsdl/schematron"?>
<Product_Context
    xmlns="http://pds.nasa.gov/pds4/pds/v1"
    xmlns:ctli="http://pds.nasa.gov/pds4/ctli/v2"
    xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
    xsi:schemaLocation="
        http://pds.nasa.gov/pds4/pds/v1
            https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1J00.xsd
            http://pds.nasa.gov/pds4/ctli/v2 
            https://pds.nasa.gov/pds4/ctli/v2/PDS4_CTLI_1J00_2000.xsd">
    <Identification_Area>
        <logical_identifier>urn:nasa:pds:context:instrument:clps_to_2ab_pll.nss</logical_identifier>
        <version_id>1.0</version_id>
        <title>CLPS Task Order 2AB Neutron Spectrometer System (NSS)</title>
        <information_model_version>1.19.0.0</information_model_version>
        <product_class>Product_Context</product_class>
        <Modification_History>
            <Modification_Detail>
                <modification_date>2024-05-13</modification_date>
                <version_id>1.0</version_id>
                <description>Initial version.</description>
            </Modification_Detail>
        </Modification_History>
    </Identification_Area>
    <Reference_List>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:context:instrument_host:spacecraft.clps_to_2ab_pll</lid_reference>
            <reference_type>instrument_to_instrument_host</reference_type>
        </Internal_Reference>
        <External_Reference>
            <doi>10.1016/j.nima.2023.168063</doi>
            <reference_text> 
                Peplowski, P.N., Elphic, R.C., Fritzler, E.L. and Wilson, J.T., 2023. Calibration of NASA's Neutron Spectrometer System 
                (NSS) for landed measurements of hydrogen content of the lunar subsurface. Nuclear Instruments and Methods in Physics 
                Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, p.168063. 
            </reference_text>
        </External_Reference>
    </Reference_List>
    <Instrument>
        <name>CLPS Task Order 2AB Neutron Spectrometer System (NSS)</name>
        <Type_List_Area>
            <ctli:Type_List>
                <ctli:type>Spectrometer</ctli:type>
                <ctli:subtype>Neutron Spectrometer</ctli:subtype>
            </ctli:Type_List>
        </Type_List_Area>
        <description>
            The Neutron Spectrometer System is an instrument designed to measure the leakage flux of low-energy neutrons out of the 
            lunar soil.  A key determinant of leakage flux in the epithermal energy range (>0.5 eV – 500 keV) is abundance of 
            hydrogen-bearing compounds. NSS gauges the fluxes of neutrons in two energy ranges: a) thermal neutrons, less than 0.5 eV, 
            which respond to both abundance and burial depth of hydrogenous materials, and b) epithermal neutrons, which vary in a 
            different way with hydrogen abundance and burial depth from the thermal neutron population.  Together, these two measurements 
            constrain not only water-equivalent hydrogen (WEH) abundance but permit a simple model of stratigraphy (burial depth and 
            lower-layer WEH abundance, assuming the overburden is hydrogen-free). Water-equivalent hydrogen is the weight percent of 
            water that a material would contain if all the detected hydrogen was in the form of H2O. For example, a material containing 
            1500 ppm H would have a water-equivalent hydrogen content of 1.35 wt.%.
            
            NSS consists of gas-proportional counter neutron detectors with a design based on the Lunar Prospector Neutron Spectrometer. 
            NSS will measure any temporal variations of at least 0.5 wt.% water-equivalent hydrogen (WEH) at the lander's location. NSS 
            measurements are also used to infer the probable burial depth and WEH wt.% of a buried layer below otherwise desiccated 
            regolith.               
        </description>
    </Instrument>
</Product_Context>
