@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/992cb370-d2d0-4a9f-a4d4-179f140f505a>
  skos:changeNote """2018-07-05 11:27:53.0 [mmorahan] Insert Concept 
add broader relation (GIS [992cb370-d2d0-4a9f-a4d4-179f140f505a,367767] - Cameras [d322ae9d-bde0-448f-948d-777aef096eb6,348777]); 
""", """2018-07-05 11:31:04.0 [mmorahan]  
insert AltLabel (id: null
category: primary
text: GeoEye Imaging System
language code: en); 
insert Definition (id: null
text: GIS is a pushbroom imaging system whose basic elements are the optics subsystem (telescope assembly), the focal plane assembly (CCD detector), and the digital electronics subsystem. The optics subsystem employs a TMA (Three Mirror Anastigmatic) telescope design with a primary mirror aperture of 1.1 m in diameter. Three mirrors are used to image and focus the light, and two additional mirrors to direct the image to the FPA (Focal Plane Assembly). The telescope is designed to give a near-perfect (diffraction limited) image to the FPA and to convert the analog pixels into digitized signals.

The FPA consists of an array of CCD detectors with 8 µm pixel size for PAN and 32 µm pixel size for multispectral imagery. ITT has included an outer barrel and door assembly to help protect the telescope and maintain its thermal environment.

Imager type

Pushbroom imager. Lline scan imaging system with TDI (Time Delay Integration) capability

Imaging mode

Panchromatic (Pan)

Multispectral (MS)

Spectral range

450-900 nm

450-510 nm (blue)
520-580 nm (green)
655-690 nm (red)
780-920 nm (near infrared)

Spatial resolution at nadir

0.41 m GSD

1.64 m GSD

Swath width

15.2 km (multiple adjoining paths can be imaged in a target area in a single orbit pass due to S/C agility)

Detectors

Pan: Si CCD array (8 µm pixel size) with a row of > 35,000 detectors
MS: Si CCD 4 arrays (32 µm pixel size) with a row of > 9,300 detectors

Data quantization

11 bit

Geolocation accuracy of imagery

≤ 3 m (using a GPS receiver, a gyroscope and a star tracker) without any GCP (Ground Control Points)

Optics

TMA telescope (5-element modified Cassegrain optical design)
Aperture diameter of 1.1 m, focal length = 13.3 m, f/12

FOV (Field of View)

> 1.28º

Instrument size

3 m tall (the volume is 5.3 m3)

Total instrument mass

452 kg
language code: en); 
""", """2019-02-19 13:00:06.0 [mmorahan]  
insert WeightedRelation (id: null
related concept uuid: 47943416-e045-4d6d-b18e-3d1cc51734e0
relationship type: null
relationship value: null
generated by: null); 
""" ;
  ns0:altLabel [ ] ;
  skos:definition """GIS is a pushbroom imaging system whose basic elements are the optics subsystem (telescope assembly), the focal plane assembly (CCD detector), and the digital electronics subsystem. The optics subsystem employs a TMA (Three Mirror Anastigmatic) telescope design with a primary mirror aperture of 1.1 m in diameter. Three mirrors are used to image and focus the light, and two additional mirrors to direct the image to the FPA (Focal Plane Assembly). The telescope is designed to give a near-perfect (diffraction limited) image to the FPA and to convert the analog pixels into digitized signals.

The FPA consists of an array of CCD detectors with 8 µm pixel size for PAN and 32 µm pixel size for multispectral imagery. ITT has included an outer barrel and door assembly to help protect the telescope and maintain its thermal environment.

Imager type

Pushbroom imager. Lline scan imaging system with TDI (Time Delay Integration) capability

Imaging mode

Panchromatic (Pan)

Multispectral (MS)

Spectral range

450-900 nm

450-510 nm (blue)
520-580 nm (green)
655-690 nm (red)
780-920 nm (near infrared)

Spatial resolution at nadir

0.41 m GSD

1.64 m GSD

Swath width

15.2 km (multiple adjoining paths can be imaged in a target area in a single orbit pass due to S/C agility)

Detectors

Pan: Si CCD array (8 µm pixel size) with a row of > 35,000 detectors
MS: Si CCD 4 arrays (32 µm pixel size) with a row of > 9,300 detectors

Data quantization

11 bit

Geolocation accuracy of imagery

≤ 3 m (using a GPS receiver, a gyroscope and a star tracker) without any GCP (Ground Control Points)

Optics

TMA telescope (5-element modified Cassegrain optical design)
Aperture diameter of 1.1 m, focal length = 13.3 m, f/12

FOV (Field of View)

> 1.28º

Instrument size

3 m tall (the volume is 5.3 m3)

Total instrument mass

452 kg"""@en ;
  skos:prefLabel "GIS"@en ;
  skos:inScheme <https://gcmd.earthdata.nasa.gov/kms/concepts/concept_scheme/instruments> ;
  skos:broader <https://gcmd.earthdata.nasa.gov/kms/concept/d322ae9d-bde0-448f-948d-777aef096eb6> ;
  a skos:Concept .

<https://gcmd.earthdata.nasa.gov/kms/concept/d322ae9d-bde0-448f-948d-777aef096eb6>
  skos:prefLabel "Cameras"@en ;
  a skos:Concept ;
  skos:narrower <https://gcmd.earthdata.nasa.gov/kms/concept/992cb370-d2d0-4a9f-a4d4-179f140f505a> .

