@prefix skos: <http://www.w3.org/2004/02/skos/core#> .
@prefix ns0: <http://gcmd.gsfc.nasa.gov/kms#> .

<https://gcmd.earthdata.nasa.gov/kms/concept/1f7c6ae3-d38e-42b7-a874-60298b0fcfa1>
  skos:changeNote """2019-02-22 08:35:47.0 [mmorahan]  
insert WeightedRelation (id: null
related concept uuid: 598b6dc4-aff0-4e14-b7b7-039e58560dd0
relationship type: null
relationship value: null
generated by: null); 
insert WeightedRelation (id: null
related concept uuid: c143ee20-1d14-4003-9043-f028c19f0265
relationship type: null
relationship value: null
generated by: null); 
""", """2020-10-07 11:08:54.0 [mmorahan]  
insert AltLabel (id: null
category: primary
text: ODIN
language code: en); 
""" ;
  ns0:altLabel [ ] ;
  skos:definition """ODIN is a Swedish small satellite project for Astronomical and
Atmospheric Research. The Aeronomy research will address
scientific problem areas in the stratosphere and mesosphere by
making measurements of various trace species. The scientific
goals can be summarized as follows:

1. Stratospheric ozone science: To elucidate the geographical
extent of and mechanisms responsible for ozone depletion in the
"ozone hole" region and to study dilution effects and possible
heterogeneous chemistry even outside of the polar regions due to
sulphate aerosols

2. Mesospheric ozone science: To establish the relative role of
odd hydrogen chemistry and the effects of ordered and turbulent
transport and corpuscular radiation.

3. Summer mesospheric science: To establish the variability of
mesospheric water vapor including an assessment of the required
fluxes for aerosol formation in the polar mesosphere.

4. Coupling of atmospheric regions: To study some of the
mechanisms that provide coupling between the upper and lower
atmosphere, eg downward transport of aurorally enhanced NO with
its effects on ozone photo chemistry and the vertical exchange
of minor species such as odd oxygen, CO and H2O.

Odin will work in unexplored bands of the electromagnetic
spectrum, around wavelengths of 0.5 mm and 3 mm. These contain
emission lines from important molecules such as water vapor,
molecular oxygen, ozone and carbon monoxide. The lines will be
used as tools to study processes in the Earth's atmosphere and
in astronomical objects. Complementary information on the
atmosphere will come from spectral lines at ultraviolet and
optical wavelengths. Major scientific issues relate to star
formation processes interstellar chemistry and atmospheric ozone
balance.

Additional information available at
http://www.ssc.se/ssd/ssat/odin.html

[Summary provided by Swedish Space Corporation]"""@en ;
  skos:prefLabel "ODIN"@en ;
  skos:inScheme <https://gcmd.earthdata.nasa.gov/kms/concepts/concept_scheme/platforms> ;
  skos:broader <https://gcmd.earthdata.nasa.gov/kms/concept/3466eed1-2fbb-49bf-ab0b-dc08731d502b> ;
  a skos:Concept .

<https://gcmd.earthdata.nasa.gov/kms/concept/3466eed1-2fbb-49bf-ab0b-dc08731d502b>
  skos:prefLabel "Earth Observation Satellites"@en ;
  a skos:Concept ;
  skos:narrower <https://gcmd.earthdata.nasa.gov/kms/concept/1f7c6ae3-d38e-42b7-a874-60298b0fcfa1> .