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Data Access

STEREO-B/SECCHI/HI-1 FITS data

(2006). STEREO-B/SECCHI/HI-1 FITS data [Data set]. STEREO Science Center. https://doi.org/10.48322/zstc-3d34. Accessed on .

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

ResourceID
spase://NASA/NumericalData/STEREO-B/SECCHI/HI-1/PT40M

Description

The Heliospheric Imager-1 (HI-1) telescope is part of the Sun Earth Connection Coronal and Heliospheric Investigations (SECCHI) instrument suite on the NASA STEREO mission. The SECCHI on the two STEREO spacecraft are identical suites of remote sensing instruments designed to observe coronal mass ejections (CMEs) at the Sun and in transit outwards to 1 AU. The HI-1 telescope observes the inner heliosphere from 12 to 84 solar radii with the band-pass wavelength of 450-750 nm.

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Details

Version:2.6.0

NumericalData

ResourceID
spase://NASA/NumericalData/STEREO-B/SECCHI/HI-1/PT40M
ResourceHeader
ResourceName
STEREO-B/SECCHI/HI-1 FITS data
DOI
https://doi.org/10.48322/zstc-3d34
ReleaseDate
2020-07-07 21:15:23Z
RevisionHistory
RevisionEvent
ReleaseDate
2024-01-03 00:08:46
Note
Added STEREO Science Center to the AccessURL; Updated the Contacts
RevisionEvent
ReleaseDate
2024-03-04 00:08:46
Note
Created a separated SPASE record for STEREO-A/SECCHI/HI-1 NumericalData
RevisionEvent
ReleaseDate
2024-03-28 00:08:46
Note
Added DOI by SY
Description

The Heliospheric Imager-1 (HI-1) telescope is part of the Sun Earth Connection Coronal and Heliospheric Investigations (SECCHI) instrument suite on the NASA STEREO mission. The SECCHI on the two STEREO spacecraft are identical suites of remote sensing instruments designed to observe coronal mass ejections (CMEs) at the Sun and in transit outwards to 1 AU. The HI-1 telescope observes the inner heliosphere from 12 to 84 solar radii with the band-pass wavelength of 450-750 nm.

PublicationInfo
Authors
The SECCHI Consortium: Naval Research Laboratory (USA); Lockheed Martin Solar and Astrophysics Laboratory (USA); NASA Goddard Space Flight Center (USA); Johns Hopkins University Applied Physics Laboratory (USA); Rutherford Appleton Laboratory (UK); University of Birmingham (UK); Max-Planck-Institut für Sonnensystemforschung (Germany); Centre Spatiale de Liege (Belgium); Institut d'Optique Théorique et Appliqueé (France); Institut d'Astrophysique Spatiale (France)
PublicationDate
2006-12-06 00:00:00
PublishedBy
STEREO Science Center
Contacts
RolePersonStartDateStopDateNote
1.InstrumentScientistspase://SMWG/Person/Jackiei.Davies
2.InstrumentScientistspase://SMWG/Person/Richard.A.Harrison
3.PrincipalInvestigatorspase://SMWG/Person/Brian.Wood
4.ProjectScientistspase://SMWG/Person/Angelos.Vourlidas
5.FormerPIspase://SMWG/Person/Russell.A.Howard
6.MetadataContactspase://SMWG/Person/Seiji.Yashiro
PriorIDs
spase://VSPO/NumericalData/P_STEREO_HDR_SECCHI
spase://VSPO/NumericalData/STEREO/SECCHI
spase://NASA/NumericalData/STEREO/SECCHI
AccessInformation
RepositoryID
spase://SMWG/Repository/NASA/GSFC/STEREO_SC
Availability
Online
AccessRights
Open
AccessURL
Name
STEREO Science Center
URL
https://stereo-ssc.nascom.nasa.gov/data/ins_data/secchi/L0_YMD/b/img/hi_1/
Format
FITS
AccessInformation
RepositoryID
spase://SMWG/Repository/SDAC
AccessURL
Name
Virtual Solar Observaroty
URL
https://sdac.virtualsolar.org/cgi/search
Style
Search
Format
FITS
ProcessingLevel
Raw
InstrumentIDs
spase://NASA/Instrument/STEREO-B/SECCHI/HI-1
MeasurementType
ImageIntensity
TemporalDescription
TimeSpan
StartDate
2006-10-01 00:00:00Z
StopDate
2014-09-27 15:29:01
SpectralRange
WhiteLight
ObservedRegion
Sun.Corona