EVE

E399072

EVE is an instrument on NASA’s Solar Dynamics Observatory that measures the Sun’s extreme ultraviolet irradiance to study solar variability and its effects on Earth’s atmosphere.

All labels observed (1)

Label Occurrences
EVE canonical 2

How this entity was disambiguated

Statements (47)

Predicate Object
instanceOf extreme ultraviolet spectrograph
solar irradiance monitor
space-based solar instrument
acronymFor Extreme Ultraviolet Variability Experiment
cadence about 10-second measurements (nominal)
calibration designed for long-term irradiance stability
countryOfOperator United States of America
surface form: United States
dataArchive SDO data archives
dataFormat FITS files (commonly used in solar physics)
dataUsedBy ionospheric models
thermospheric density models
upper atmosphere models
field heliophysics
solar physics
space weather research
fullName Extreme Ultraviolet Variability Experiment
hasSubsystem EUV photometers
Multiple EUV spectrographs
hostAgency Goddard Space Flight Center
surface form: NASA Goddard Space Flight Center
launchDate 2010-02-11
launchSite Cape Canaveral Space Force Station
surface form: Cape Canaveral Air Force Station
launchVehicle Atlas V 401
measures solar extreme ultraviolet irradiance
spectral solar irradiance in the EUV band
mission Solar Dynamics Observatory mission
onboard Solar Dynamics Observatory
operatedBy NASA
orbits Earth
orbitType geosynchronous transfer orbit (via SDO)
partOf Solar Dynamics Observatory
primaryObjective quantify solar EUV input to Earth’s upper atmosphere
study solar EUV variability
program Living With a Star program
surface form: NASA Living With a Star program
provides high-cadence EUV irradiance measurements
spectrally resolved EUV irradiance
relatedTo Atmospheric Imaging Assembly
surface form: AIA (Atmospheric Imaging Assembly)

Helioseismic and Magnetic Imager
surface form: HMI (Helioseismic and Magnetic Imager)
scienceTeamLeadInstitution Laboratory for Atmospheric and Space Physics
University of Colorado Boulder
spacecraft Solar Dynamics Observatory
studies solar flares in EUV wavelengths
solar variability
space weather drivers
supports climate and atmospheric change studies related to solar forcing
usedFor modeling Earth’s thermosphere and ionosphere
space weather forecasting research
wavelengthRange approximately 0.1–105 nm

How these facts were elicited

Referenced by (2)

Full triples — surface form annotated when it differs from this entity's canonical label.