PHI

E1047344

PHI is a scientific instrument designed to study the Sun’s magnetic fields and internal structure using polarimetric and helioseismic measurements.

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Statements (48)

Predicate Object
instanceOf helioseismology instrument
polarimetric instrument
scientific instrument
solar telescope instrument
acronymFor Polarimetric and Helioseismic Imager NERFINISHED
dataType high-cadence helioseismic data
high-precision polarimetric data
designedFor remote sensing of the Sun
enables helioseismic inversions
magnetic field inversions
fieldOfStudy helioseismology
solar magnetism
solar physics
fullName Polarimetric and Helioseismic Imager NERFINISHED
hasCapability intensity imaging
line-of-sight velocity measurements
vector magnetic field measurements
measurementGoal determine solar oscillation properties
determine solar surface magnetic field vector
observes solar line-of-sight velocities
solar photosphere
vector magnetic field at the solar surface
primaryObjective study the Sun’s internal structure
study the Sun’s magnetic field
provides Dopplergrams
continuum intensity images
magnetograms
scientificGoal characterize meridional flows in the solar interior
characterize solar internal rotation
constrain models of the solar dynamo
improve prediction of solar activity
understand coupling between solar interior and atmosphere
studies solar active regions
solar convection zone
solar dynamo processes
solar interior
solar magnetic fields
sunspots
supportsResearchOn solar cycle variability
solar interior dynamics
solar magnetism
space weather
targetBody Sun NERFINISHED
usesMeasurementType helioseismic measurements
polarimetric measurements
usesTechnique Doppler imaging
spectropolarimetry
time–distance helioseismology

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