ResourceName
Wind 3DP 24-sec ESSA-HIGH Electron Omnidirectional Fluxes
DOI
https://doi.org/10.48322/c201-q577
ReleaseDate
2025-12-04 13:32:48Z
RevisionHistory
RevisionEvent
ReleaseDate
2021-05-31 12:34:56.789
Note
Updated to SPASE Version 2.3.2 if needed, Applied quality control for DOI usage, LFB
RevisionEvent
ReleaseDate
2025-09-30 14:25:25Z
Note
Updated PublishedBy name to match ROR Registry. Added ResourceType and NamingAuthority. Changed http to https in top-level schemaLocation attribute. Fixed version number separator in top-level schemaLocation attribute. Matched version number in schemaLocation attribute to updated value in Version tag. ZCB
RevisionEvent
ReleaseDate
2025-12-04 13:32:48Z
Note
Added MetadataRightsList and RightsList(s). Updated to 2.7.1. ZCB
Description
Electron omnidirectional fluxes 100 eV-30 keV, often at 24 sec, EESA High, Wind 3DP - R. Lin (UC Berkeley)
Acknowledgement
Principle Investigators Robert Lin and Stuart Bale, the Wind 3DP team, and the Space Physics Data Facility (SPDF)/NASA GSFC
PublicationInfo
Authors
Lin, Robert P.; Bale, Stuart D.; & Wilson III, Lynn B.
PublicationDate
2021-01-01 00:00:00
PublishedBy
Space Physics Data Facility; University of California, Berkeley
Contacts
InformationURL
Name
Caveats to the use of Wind 3DP data
URL
Description
Caveats for the correct use of Wind 3DP datasets
InformationURL
Name
Wind 3DP home page at UCB
URL
Description
home page at UCB (with plotting and digital data)
PriorIDs
spase://VSPO/NumericalData/Wind/3DP/EESA_HIGH/SP/PT24S
With respect to time resolution: 24 sec timing changes and is not necessarily constant, depending on the mode that the instrument happens to be in. Not only does the period/interval between each point change, the duration over which the data were taken can change as well.