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STEREO-B/SECCHI/EUVI FITS data

(2006). STEREO-B/SECCHI/EUVI FITS data [Data set]. Goddard Space Flight Center. https://doi.org/10.48322/xd10-f786. 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/EUVI/PT5M

Description

The Extreme Ultraviolet Imager (EUVI) 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.

EUVI measured emission lines at 30.4 nm (He II), 17.1 nm (Fe IX), 19.5 nm (Fe XII), and 21.1 nm (Fe XIV). The EUVI's 2048 x 2048 pixel detectors have a field of view out to 1.7 solar radii, and observe in four spectral channels that span the 0.1 to 20 MK temperature range. In addition to its view from two vantage points, the EUVI will provide a substantial improvement in image resolution and image cadence over its predecessor SOHO-EIT, while complying with the more restricted mass, power, and volume allocations on the STEREO mission.

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Details

Version:2.7.1

MetadataRightsList

Rights
SchemeURI
https://spdx.org/licenses/
RightsIdentifierScheme
SPDX
RightsIdentifier
CC0-1.0
RightsURI
https://spdx.org/licenses/CC0-1.0.html
RightsName
Creative Commons Zero v1.0 Universal
Note
CC0 1.0 Universal is the Creative Commons license applicable to all publicly available SPASE metadata descriptions

Version:2.7.1

NumericalData

ResourceID
spase://NASA/NumericalData/STEREO-B/SECCHI/EUVI/PT5M
NamingAuthority
NASA
ResourceType
NumericalData
ResourceHeader
ResourceName
STEREO-B/SECCHI/EUVI FITS data
DOI
https://doi.org/10.48322/xd10-f786
ReleaseDate
2025-12-04 13:31:40Z
RevisionHistory
RevisionEvent
ReleaseDate
2020-07-07 21:15:23Z
Note
Only known prior ReleaseDate of the metadata
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
A separated SPASE record for STEREO-B/SECCHI/EUVI NumericalData
RevisionEvent
ReleaseDate
2024-03-28 00:08:46
Note
Added DOI by SY
RevisionEvent
ReleaseDate
2025-09-18 12:12:35Z
Note
Added ResourceType and NamingAuthority. Changed http to https in top-level schemaLocation attribute. Matched version number in schemaLocation attribute to updated value in Version tag. ZCB
RevisionEvent
ReleaseDate
2025-09-30 14:25:28Z
Note
Updated PublishedBy name to match ROR Registry. ZCB
RevisionEvent
ReleaseDate
2025-12-04 13:31:40Z
Note
Added MetadataRightsList and RightsList(s). Updated to 2.7.1. ZCB
Description

The Extreme Ultraviolet Imager (EUVI) 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.

EUVI measured emission lines at 30.4 nm (He II), 17.1 nm (Fe IX), 19.5 nm (Fe XII), and 21.1 nm (Fe XIV). The EUVI's 2048 x 2048 pixel detectors have a field of view out to 1.7 solar radii, and observe in four spectral channels that span the 0.1 to 20 MK temperature range. In addition to its view from two vantage points, the EUVI will provide a substantial improvement in image resolution and image cadence over its predecessor SOHO-EIT, while complying with the more restricted mass, power, and volume allocations on the STEREO mission.

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
Goddard Space Flight Center
Contacts
RolePersonStartDateStopDateNote
1.InstrumentScientistspase://SMWG/Person/James.R.Lemen
2.PrincipalInvestigatorspase://SMWG/Person/Brian.Wood
3.ProjectScientistspase://SMWG/Person/Angelos.Vourlidas
4.FormerPIspase://SMWG/Person/Russell.A.Howard
5.GeneralContactspase://SMWG/Person/William.T.Thompson
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
Availability
Online
AccessRights
Open
RightsList
Rights
SchemeURI
https://spdx.org/licenses/
RightsIdentifierScheme
SPDX
RightsIdentifier
CC0-1.0
RightsURI
https://spdx.org/licenses/CC0-1.0.html
RightsName
Creative Commons Zero v1.0 Universal
Note
CC0 1.0 Universal is the Creative Commons license applicable to all publicly available NASA Heliophysics data products
AccessURL
Format
FITS
AccessInformation
RepositoryID
RightsList
Rights
SchemeURI
https://spdx.org/licenses/
RightsIdentifierScheme
SPDX
RightsIdentifier
CC0-1.0
RightsURI
https://spdx.org/licenses/CC0-1.0.html
RightsName
Creative Commons Zero v1.0 Universal
Note
CC0 1.0 Universal is the Creative Commons license applicable to all publicly available NASA Heliophysics data products
AccessURL
Name
Virtual Solar Observaroty
URL
Style
Search
Format
FITS
ProcessingLevel
Raw
InstrumentIDs
MeasurementType
ImageIntensity
TemporalDescription
TimeSpan
StartDate
2006-10-01 00:00:00Z
StopDate
2014-09-27 15:56:15
SpectralRange
ExtremeUltraviolet
ObservedRegion
Sun.Corona