<?xml version="1.0" encoding="utf-8"?>
<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" 
  xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_2_2.xsd">
  <Version>2.2.2</Version>
  <Instrument>
    <ResourceID>spase://SMWG/Instrument/Ground/MaunaLoaSO/ACOS</ResourceID>
    <ResourceHeader>
      <ResourceName>MLSO_ACOS</ResourceName>
      <ReleaseDate>2015-10-23T00:00:00Z</ReleaseDate>
      <Description>ACOS is the Advanced Coronal Observation System at
Mauna Loa Solar Observatory.  It is a suite of instruments designed to 
observe the solar atmosphere, including the Chromospheric Helium Imaging 
Photometer (CHIP, 1083.0nm), H-alpha prominence and solar disk monitor 
(PICS, 656.3nm), and the Mk4 K-coronameter, which observes the white 
light K-corona from 1.12-2.79 solar radii (700-950 nm).</Description>
      <Contact>
        <PersonID>spase://SMWG/Person/Thomas.E.Holzer</PersonID>
        <Role>GeneralContact</Role>
      </Contact>
      <PriorID>spase://SMWG/Instrument/MaunaLoaSO/ACOS</PriorID>
    </ResourceHeader>
    <InstrumentType>Imager</InstrumentType>
    <InvestigationName>ACOS at MLSO</InvestigationName>
    <ObservatoryID>spase://SMWG/Observatory/Ground/MaunaLoaSO</ObservatoryID>
  </Instrument>
</Spase>