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STEREO-B/SECCHI/Cor1 FITS data

(2006). STEREO-B/SECCHI/Cor1 FITS data [Data set]. STEREO Science Center. https://doi.org/10.48322/yscr-4569. 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/Cor1/PT5M

Description

The COR1 telescope is the inner coronagraph of the Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) instrument suite aboard the twin Solar Terrestrial Relations Observatory (STEREO) spacecraft. Like all coronagraphs, COR1 is designed to measure the weak light from the solar corona in the presence of scattered light from the much brighter solar photosphere. It designed to observe the white light corona from 1.4 to 4 solar radii.

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Details

Version:2.6.0

NumericalData

ResourceID
spase://NASA/NumericalData/STEREO-B/SECCHI/Cor1/PT5M
ResourceHeader
ResourceName
STEREO-B/SECCHI/Cor1 FITS data
DOI
https://doi.org/10.48322/yscr-4569
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-B/SECCHI/Cor1 NumericalData
RevisionEvent
ReleaseDate
2024-03-28 00:08:46
Note
Added DOI by SY
Description

The COR1 telescope is the inner coronagraph of the Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) instrument suite aboard the twin Solar Terrestrial Relations Observatory (STEREO) spacecraft. Like all coronagraphs, COR1 is designed to measure the weak light from the solar corona in the presence of scattered light from the much brighter solar photosphere. It designed to observe the white light corona from 1.4 to 4 solar radii.

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/Charles.N.Arge
2.InstrumentScientistspase://SMWG/Person/Joseph.M.Davila
3.CoInvestigatorspase://SMWG/Person/O.Chris.St.Cyr
4.CoInvestigator
GeneralContact
spase://SMWG/Person/William.T.Thompson
5.CoInvestigatorspase://SMWG/Person/Nat.Gopalswamy
6.CoInvestigatorspase://SMWG/Person/Barbara.J.Thompson
7.CoInvestigatorspase://SMWG/Person/Hong.Xie
8.PrincipalInvestigatorspase://SMWG/Person/Brian.Wood
9.ProjectScientistspase://SMWG/Person/Angelos.Vourlidas
10.FormerPIspase://SMWG/Person/Russell.A.Howard
11.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
AccessURL
Format
FITS
AccessInformation
RepositoryID
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 15:55:24
SpectralRange
WhiteLight
ObservedRegion
Sun.Corona