Solar Ultraviolet Spectral Irradiance Monitor

E451727

The Solar Ultraviolet Spectral Irradiance Monitor is a spaceborne instrument designed to measure the Sun’s ultraviolet radiation across multiple wavelengths to study solar variability and its effects on Earth’s atmosphere and climate.

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Statements (41)

Predicate Object
instanceOf solar ultraviolet radiometer
spaceborne instrument
applicationDomain Earth science
climate science
heliophysics
category remote sensing instrument
solar monitoring payload
contributesTo radiative forcing estimates
understanding of ozone layer dynamics
understanding of solar cycle variability
dataType calibrated solar UV flux measurements
spectral irradiance time series
designedFor study of Sun–Earth interactions
study of effects of solar UV on Earth’s atmosphere
study of effects of solar UV on climate
study of solar variability
environment space
hasCapability monitoring temporal variability of solar UV output
spectral resolution in ultraviolet band
impactOn ionospheric modeling
satellite drag prediction
studies of upper atmosphere heating
measures solar spectral irradiance
solar ultraviolet radiation
ultraviolet irradiance across multiple wavelengths
monitors long-term trends in solar UV output
short-term solar UV fluctuations
observes Sun NERFINISHED
observesProperty solar spectral energy distribution in UV
variability of solar UV irradiance over time
operatesIn ultraviolet wavelength range
platformType satellite-borne
requires long-term instrument stability
precise radiometric calibration
supports assessment of solar forcing in climate models
climate change attribution studies
usedFor atmospheric chemistry studies
climate modeling
long-term solar irradiance records
space weather research
validation of solar irradiance models

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STS-45 payload Solar Ultraviolet Spectral Irradiance Monitor
Atmospheric Laboratory for Applications and Science 3 hasInstrument Solar Ultraviolet Spectral Irradiance Monitor