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    <Identification_Area>
        <logical_identifier>urn:nasa:pds:context:instrument:xrs.near</logical_identifier>
        <version_id>1.1</version_id>
        <title>XRAY SPECTROMETER for NEAR</title>
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        <product_class>Product_Context</product_class>
        <Modification_History>
            <Modification_Detail>
                <modification_date>2023-05-12</modification_date>
                <version_id>1.1</version_id>
                <description>
                    Removed extraneous external references, replaced description with a short summary, 
                    and added NAIF instrument ID and Type List Area
                </description>
            </Modification_Detail>
            <Modification_Detail>
                <modification_date>2016-10-01</modification_date>
                <version_id>1.0</version_id>
                <description>
                    extracted metadata from PDS3 catalog and
                    modified to comply with PDS4 Information Model
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    <Reference_List>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:context:instrument_host:spacecraft.near</lid_reference>
            <reference_type>instrument_to_instrument_host</reference_type>
        </Internal_Reference>
        <External_Reference>
            <reference_text>
                Goldsten, J.O., The NEAR X-Ray/Gamma-Ray Spectrometer, Johns Hopkins APL Technical 
                Digest, Vol. 19, pp. 126-135, 1998.
            </reference_text>
            <description>reference.GOLDSTEN1998</description>
        </External_Reference>
        <External_Reference>
            <reference_text>
                   Goldsten, J.O., R.L. McNutt, R.E. Gold, S.A. Gary, E. Fiore, S.E. Schneider,
                   J.R. Hayes, J.I. Trombka, S.R. Floyd, W.V. Boynton, S. Bailey, J. Bruckner,
                   S.W. Squyres, L.G. Evans, P.E. Clark, and R. Starr, The X-Ray/Gamma-Ray
                   Spectrometer on the Near Earth Asteroid Rendezvous Mission, Space Sciences 
                   Review, Vol. 82, pp. 169-216, 1997.
            </reference_text>
            <description>reference.GOLDSTENETAL1997</description>
        </External_Reference>
        <External_Reference>
            <reference_text>
                   Starr, R., P.E. Clark, L.G. Evans, S.R. Floyd, T.P. McClanahan, J.I. Trombka,
                   J.O. Goldsten, R.H. Maurer, R.L. McNutt, Jr., and D.R. Roth, Radiation effects
                   in the Si-PIN detector on the Near Earth Asteroid Rendezvous Mission, Nuclear
                   Instruments and Methods in Physics Research Section A, Vol. 428, pp. 209-215,
                   1999.
            </reference_text>
            <description>reference.STARRETAL1999</description>
        </External_Reference>
        <External_Reference>
            <reference_text>
                   Trombka, J., S. Floyd, W. Boynton, S. Bailey, J. Bruckner, S. Squyres, L.
                   Evans, P. Clear, R. Starr, E. Fiore, R. Gold, J. Goldsten, and R. McNutt,
                   Compositional Mapping With The Near X-ray/Gamma-ray Spectrometer, J. Geophys.
                   Res., Vol. 102, pp. 23729-23750, 1997.
            </reference_text>
            <description>reference.TROMBKAETAL1997</description>
        </External_Reference>
    </Reference_List>
    
    <Instrument>
        <name>XRAY SPECTROMETER</name>
        <Type_List_Area>
            <ctli:Type_List>
                <ctli:type>Spectrometer</ctli:type>
            </ctli:Type_List>
        </Type_List_Area>
        <naif_instrument_id>-93003</naif_instrument_id>
        <description>
 The NEAR XRS is part of the X-Ray/Gamma-Ray Spectrometer (XGRS) suite on the NEAR mission.  It is 
 an X-ray resonance fluorescence spectrometer that detects the characteristic X-ray line emissions 
 excited by solar X-rays from major elements in the asteroid's surface. It covers X-rays in the 
 energy range from 1 to 10 keV using three gas proportional counters.  The balanced, differential 
 filter technique is used to separate the closely spaced Mg, Al, and Si lines lying below 2 keV. The 
 gas proportional counters directly resolve higher energy line emissions from Ca and Fe. A mechanical     
 collimator gives the XRS a 5 deg FOV, with which it will map the chemical composition of the asteroid 
 at spatial resolutions as great as 2 km in the low orbits. It also includes a separate solar monitor 
 system to measure continuously the incident spectrum of solar X-rays, using both a gas proportional 
 counter and a high-spectral-resolution silicon X-ray detector. The XRS performs in-flight calibration 
 using a calibration rod with Fe-55 sources that can be rotated into or out of the detector FOV. 
        </description>
    </Instrument>
</Product_Context>
