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Carruthers NFI Level 0 Images

(2026). Carruthers NFI Level 0 Images. [Data set]. Space Physics Data Facility. https://doi.org/10.48322/2tde-1r42. Accessed on .

Note: Proper references, including or other formats, should include the "Accessed on date" to identify the version of the resource being cited in a given publication.

ResourceID
spase://NASA/NumericalData/Carruthers/GCI/NFI/L0

Description
The Narrow Field Imager (NFI) channel of the Carruthers GeoCoronal Imager (GCI) provides better than 250 km resolution at nadir from the Lagrange point #1 halo orbit of the Carruthers Geocoronal Observatory. The Level 0 data contain all of the images obtained using the NFI channel. Science imaging began on February 16, 2026, and was regularly scheduled after March 3, 2026. The NFI has filter options including open, Lyman Alpha Narrow, Lyman Alpha Extra Narrow, Calcium Fluoride, Strontium Fluoride, and Blocked. Baseline integration times are 30 minutes in NFI. Stellar observations for calibration are obtained when opportunity arrives with near anti-sun position of the stars, and blocked images for detector bias and dark current are obtained several times daily.

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Details

Version:2.7.2

NumericalData

ResourceID
spase://NASA/NumericalData/Carruthers/GCI/NFI/L0
NamingAuthority
NASA
ResourceType
NumericalData
ResourceHeader
ResourceName
Carruthers NFI Level 0 Images
DOI
https://doi.org/10.48322/2tde-1r42
ReleaseDate
2026-08-14 15:25:15
Description
The Narrow Field Imager (NFI) channel of the Carruthers GeoCoronal Imager (GCI) provides better than 250 km resolution at nadir from the Lagrange point #1 halo orbit of the Carruthers Geocoronal Observatory. The Level 0 data contain all of the images obtained using the NFI channel. Science imaging began on February 16, 2026, and was regularly scheduled after March 3, 2026. The NFI has filter options including open, Lyman Alpha Narrow, Lyman Alpha Extra Narrow, Calcium Fluoride, Strontium Fluoride, and Blocked. Baseline integration times are 30 minutes in NFI. Stellar observations for calibration are obtained when opportunity arrives with near anti-sun position of the stars, and blocked images for detector bias and dark current are obtained several times daily.
PublicationInfo
Authors
Jason McPhate and Lara Waldrop
PublicationDate
2026-08-14 15:25:15Z
PublishedBy
Space Physics Data Facility
Contacts
Role Person StartDate StopDate Note
1. InstrumentScientist spase://SMWG/Person/Jason.McPhate
2. PrincipalInvestigator spase://SMWG/Person/Lara.Waldrop

InformationURL
AccessInformation
InstrumentIDs
MeasurementType
ImageIntensity
ObservedRegion
Earth.NearSurface