<?xml version='1.0' encoding='utf-8'?>
<?xml-model href="https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1O00.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_1O00.xsd">
  <Identification_Area>
    <logical_identifier>urn:nasa:pds:context:investigation:individual.lab_atm-opt-const-titan</logical_identifier>
    <version_id>1.0</version_id>
    <title>Optical Constants of Laboratory Generated Titan Atmospheric Aerosol Analogs</title>
    <information_model_version>1.24.0.0</information_model_version>
    <product_class>Product_Context</product_class>
    <Modification_History>
      <Modification_Detail>
        <modification_date>2026-04-13</modification_date>
        <version_id>1.0</version_id>
        <description>Initial setup of the product.</description>
      </Modification_Detail>
    </Modification_History>
  </Identification_Area>
  <Reference_List>
    <Internal_Reference>
      <lid_reference>urn:nasa:pds:context:facility:laboratory.arc-cosmic</lid_reference>
      <reference_type>investigation_to_facility</reference_type>
    </Internal_Reference>
    <Internal_Reference>
      <lid_reference>urn:nasa:pds:context:facility:laboratory.arc-ocf</lid_reference>
      <reference_type>investigation_to_facility</reference_type>
    </Internal_Reference>
  </Reference_List>
  <Investigation>
    <name>Optical Constants of Laboratory Generated Titan Atmospheric Aerosol Analogs</name>
    <type>Individual Investigation</type>
    <start_date>2026-04-08</start_date>
    <stop_date nilReason="unknown" xsi:nil="true"/>
    <description>
      This archive contains experimentally measured complex refractive indices of laboratory-generated organic refractory materials (tholins) 
      produced at low temperature (150 K) using plasma chemistry in the stream of a supersonic expansion in NASA Ames’ COsmic SImulation 
      Chamber (COSmIC) facility. The COSmIC tholin samples were produced from various gas mixtures representative of Titan, Pluto, Jupiter, 
      and exoplanet atmospheric compositions with a high voltage of -700V. The real (n) and imaginary (k) parts of the complex index of 
      refraction were determined from reflectance and transmission spectroscopic measurements conducted with the Optical Constants Facility 
      and/or the Soleil Synchrotron AILES beamline facility.
        </description>
  </Investigation>
</Product_Context>
