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

<https://gcmd.earthdata.nasa.gov/kms/concept/e14a5672-7cea-4e59-9135-bc16b2b8d1d1>
  skos:inScheme <https://gcmd.earthdata.nasa.gov/kms/concepts/concept_scheme/instruments> ;
  skos:changeNote """2022-03-22 12:37:19.0 [sritz]  
insert WeightedRelation (id: null
related concept uuid: f2b0301b-2f33-4048-9381-25a92226ed66
relationship type: null
relationship value: null
generated by: null); 
""", """2021-10-26 16:37:11.0 [sritz] Insert Concept 
add broader relation (MXGS [e14a5672-7cea-4e59-9135-bc16b2b8d1d1,778249] - Spectrometers [055a79c7-61db-4250-abad-f1e09909f14c,769377]); 
""", """2022-03-22 12:37:47.0 [sritz]  
update WeightedRelation (Platform-Instrument); 
""", """2021-10-26 16:51:45.0 [sritz]  
insert Definition (id: null
text: The ASIM MXGS instrument carries two set of detectors for TGF. The low energy detector senstive in the spectrcal band from 15 keV to 400 keV and the high energy detector sensitive from 200 keV to 40 MeV. The low energy detector is pixellated in 128 by 128 channels, which, in combination with a high mass density coded mask in front of the detector, allows advanced post-processing algorithms to pin point the direction to the TGF source. Overlaying the TGF direction with the optical imaging by the MMIA instrument, the correllation with lightning and TLE is possible.
language code: en); 
""", """2021-10-26 16:38:03.0 [sritz]  
insert AltLabel (id: null
category: primary
text: Modular X and Gamma Ray Instrument
language code: en); 
""" ;
  skos:definition "The ASIM MXGS instrument carries two set of detectors for TGF. The low energy detector senstive in the spectrcal band from 15 keV to 400 keV and the high energy detector sensitive from 200 keV to 40 MeV. The low energy detector is pixellated in 128 by 128 channels, which, in combination with a high mass density coded mask in front of the detector, allows advanced post-processing algorithms to pin point the direction to the TGF source. Overlaying the TGF direction with the optical imaging by the MMIA instrument, the correllation with lightning and TLE is possible."@en ;
  a skos:Concept ;
  skos:prefLabel "MXGS"@en ;
  ns0:reference [ ] ;
  skos:broader <https://gcmd.earthdata.nasa.gov/kms/concept/055a79c7-61db-4250-abad-f1e09909f14c> ;
  ns0:altLabel [ ] .

<https://gcmd.earthdata.nasa.gov/kms/concept/055a79c7-61db-4250-abad-f1e09909f14c>
  skos:prefLabel "Spectrometers"@en ;
  a skos:Concept ;
  skos:narrower <https://gcmd.earthdata.nasa.gov/kms/concept/e14a5672-7cea-4e59-9135-bc16b2b8d1d1> .