PFS

E394671

PFS is a planetary Fourier spectrometer used on the Venus Express mission to analyze the composition and structure of Venus’s atmosphere.

All labels observed (1)

Label Occurrences
PFS canonical 2

How this entity was disambiguated

Statements (31)

Predicate Object
instanceOf infrared spectrometer
planetary Fourier spectrometer
application climate studies of Venus
remote sensing of planetary atmospheres
validation of atmospheric models
dataType infrared spectra
radiance measurements
designedFor long-term monitoring of Venus atmosphere
environment space environment around Venus
fullName Planetary Fourier Spectrometer
locatedOn Venus Express
surface form: Venus Express orbiter
missionType orbiter payload instrument
observes day-side atmosphere of Venus
night-side atmosphere of Venus
operatedByAgency European Space Agency
operatedOnMission Venus Express
platformOrbit Venus orbit
primaryTarget Venus
scientificObjective characterize Venus atmospheric composition
characterize Venus atmospheric thermal structure
detect and quantify minor atmospheric species
investigate Venus cloud layers
measure vertical profiles of temperature
spectralRegion infrared
studies Venus atmosphere
atmospheric composition
atmospheric structure
cloud structure
temperature profiles
trace gases
usesTechnique Fourier transform infrared spectroscopy
surface form: Fourier transform spectroscopy

How these facts were elicited

Referenced by (2)

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

VEX instrument PFS
subject surface form: Venus Express