<?xml version="1.0" encoding="UTF-8"?>
<?xml-model href="https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1B00.sch" schematypens="http://purl.oclc.org/dsdl/schematron"?>
<Product_Context xmlns="http://pds.nasa.gov/pds4/pds/v1"
    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_1B00.xsd">
    
    <Identification_Area>
        <logical_identifier>urn:nasa:pds:context:instrument:sbu_cpex.raman</logical_identifier>
        <version_id>1.0</version_id>
        <title>Raman Spectrometer</title>
        <information_model_version>1.11.0.0</information_model_version>
        <product_class>Product_Context</product_class>
        <Modification_History>
            <Modification_Detail>
                <modification_date>2019-04-22</modification_date>
                <version_id>1.0</version_id>
                <description>
                    Initial creation of the context product.
                </description>
            </Modification_Detail>
        </Modification_History>
    </Identification_Area>
    
    <Reference_List>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:context:facility:laboratory.sbu_cpex</lid_reference>
            <reference_type>instrument_to_facility</reference_type>
        </Internal_Reference>
        <External_Reference>
            <doi>10.1029/2018JE005523</doi>
            <reference_text>Jaret, S.J., Johnson, J.R., Sims, M., DiFrancesco, N., and Glotch, T.D., Microscopic and petrographic 
                comparison of experimentally shocked albite, andesine, and bytownite, Journal of Geophysical Research, 123, 
                1701-1722, 2018, doi:10.1029/2018JE005523. 
            </reference_text>
        </External_Reference>
    </Reference_List>
    
    <Instrument>
        <name>Raman Spectrometer</name>
        <type>Spectrometer</type>
        <subtype>Raman Spectrometer</subtype>
        <description>
            Micro-Raman spectra for this project were obtained by the Center for Planetary Exploration at 
            Stony Brook University using a a WiTec alpha300R confocal imaging system equipped with 532 nm 
            neodymium: yttrium/aluminum/garnet (Nd:YAG) laser with 2.24 mW nominal power at the sample 
            surface, and a 50X (NA = 0.8) objective (spot size of 763 nm). Each analysis consisted of 240 
            one-second integrations that were averaged. For Raman and micro-FTIR spot analyses, multiple 
            locations were analyzed per sample. 
        </description>
    </Instrument>
</Product_Context>
