<?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:facility:laboratory.arc-cosmic</logical_identifier>
    <version_id>1.0</version_id>
    <title>NASA Ames - COsmic SImulation Chamber (COSmIC)</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 version.
                </description>
      </Modification_Detail>
    </Modification_History>
  </Identification_Area>
  <Reference_List>
    <Internal_Reference>
      <lid_reference>urn:nasa:pds:context:investigation:individual.lab_atm-opt-const-titan</lid_reference>
      <reference_type>facility_to_investigation</reference_type>
    </Internal_Reference>

  </Reference_List>
  <Facility>
    <name>NASA Ames - COsmic SImulation Chamber (COSmIC)</name>
    <type>Laboratory</type>
    <description>The Cosmic Simulation Chamber Simulation Chamber (COSmIC) was developed to generate, process and analyze interstellar, circumstellar, 
      and (exo)planetary analogs in the laboratory. COSmIC is dedicated to the study of neutral/ionized molecules, and nanoparticles/grains under temperature 
      and vacuum conditions that are representative of astrophysical environments. It consists of a pulsed discharge nozzle (PDN) mounted on a vacuum chamber
      and coupled to a cavity ringdown spectrometer (CRDS) and a quadrupole mass spectrometer (QMS) for gas phase analysis. The PDN is used to generate a 
      free supersonic expansion by injecting a gas mixture into the vacuum chamber through a very thin slit (127 µm × 10 cm). The expansion lowers the gas 
      temperature (50–150 K) and the pressure (0.1–30 mbar). A cold plasma discharge (1–2 eV energy) can be generated in the stream of the expansion by 
      applying a high voltage (600–1000 V) onto electrodes placed along the slit. This plasma discharge then generates cold isolated neutral, ions, radicals 
      in the gas phase, as well as solid particles in a setting that realistically simulates astrophysical and (exo)planetary environments. 
      Cavity Ringdown Spectroscopy (CRDS) is an ultrasensitive direct absorption technique based on the measurement of the lifetime of probe photons trapped 
      into an optical cavity formed by two high reflectivity (>99.99%) mirrors facing each other. Mass spectrometry is another in situ, non-intrusive technique 
      that allows monitoring in real time the neutral and ionized (positive and negative) species produced in the plasma expansion in COSmIC. The solid phase 
      products are in the form of grains, 50-500 nm in diameter, formed in the volume of the plasma. Solid samples can be collected by jet deposition onto various 
      substrates, then collected under inert atmosphere in a glovebox connected to the chamber, before further ex-situ characterization. 
      COSmIC is located at NASA Ames Research Center, Moffett Field, CA 94035, USA.
    </description>
  </Facility>
</Product_Context>
