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SDO/EVE Level 4 Version 8 Data

(2024). SDO/EVE Level 4 Version 8 Data [Data set]. Laboratory for Atmospheric and Space Physics, University of Colorado Boulder.

ResourceID
spase://NASA/NumericalData/SDO/EVE/Level4/Version8/PT60S

Description

The Laboratory for Atmospheric and Space Physics in Boulder, Colorado created Level 4 data files for the NASA Solar Dynamics Observatory (SDO) Extreme Ultraviolet Variability Experiment (EVE). The Science Processing and Operations Center (SPOC) is responsible for maintaining access to all EVE products.

The level 4 spectra products consist of a model spectrum at a 1-minute cadence, with each product containing 1,440 spectra covering one UTC day. The model spectra are derived from the ESP quadrant diode irradiance and the isothermal plasma temperature from the GOES X-ray channel ratios. These measurements drive a model with components for quiet sun, active region, and flare spectrum contributions. A similar technique was used for TIMED-SEE and SORCE XPS level 4 products that utilized XPS soft x-ray measurements that are analogous to the ESP quadrant diode measurements.

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Details

Version:2.6.1

NumericalData

ResourceID
spase://NASA/NumericalData/SDO/EVE/Level4/Version8/PT60S
ResourceHeader
ResourceName
SDO/EVE Level 4 Version 8 Data
ReleaseDate
2024-06-13 00:00:00Z
RevisionHistory
RevisionEvent
ReleaseDate
2024-12-02 00:08:46
Note
Metadata created by SY
Description

The Laboratory for Atmospheric and Space Physics in Boulder, Colorado created Level 4 data files for the NASA Solar Dynamics Observatory (SDO) Extreme Ultraviolet Variability Experiment (EVE). The Science Processing and Operations Center (SPOC) is responsible for maintaining access to all EVE products.

The level 4 spectra products consist of a model spectrum at a 1-minute cadence, with each product containing 1,440 spectra covering one UTC day. The model spectra are derived from the ESP quadrant diode irradiance and the isothermal plasma temperature from the GOES X-ray channel ratios. These measurements drive a model with components for quiet sun, active region, and flare spectrum contributions. A similar technique was used for TIMED-SEE and SORCE XPS level 4 products that utilized XPS soft x-ray measurements that are analogous to the ESP quadrant diode measurements.

PublicationInfo
Authors
The EVE Consortium: Laboratory for Atmospheric and Space Physics (USA); Space Sciences Center, University of Southern California (USA); Naval Research Laboratory (USA); Space Systems Research Corporation (USA); NASA Goddard Space Flight Center (USA); Lincoln Laboratory, Massachusetts Institute of Technology (USA); Electrical and Computer Engineering Department, Virginia Tech (USA); CIRES University of Colorado (USA); NOAA Space Weather Prediction Center (USA); Center for Atmospheric and Space Sciences, Utah State University (USA); Space Environment Technologies (USA)
PublicationDate
2024-06-13 00:00:00
PublishedBy
Laboratory for Atmospheric and Space Physics, University of Colorado Boulder
Contacts
RolePersonStartDateStopDateNote
1.PrincipalInvestigatorspase://SMWG/Person/Thomas.N.Woods
2.GeneralContactspase://SMWG/Person/Don.Woodraska
InformationURL
Name
The SDO EVE Website
URL
InformationURL
Name
The SDO/EVE Instrument paper
URL
InformationURL
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Format
FITS
Encoding
GZIP
InstrumentIDs
MeasurementType
Irradiance
MeasurementType
Spectrum
TemporalDescription
TimeSpan
StartDate
2010-04-30 00:00:00
RelativeStopDate
-P1D
Cadence
PT60S
ObservedRegion
Sun