Parker spiral model

E278346

The Parker spiral model is a theoretical description of the Sun’s magnetic field being wound into a spiral shape throughout the heliosphere by the combination of solar rotation and the outward-flowing solar wind.

All labels observed (2)

Label Occurrences
Parker spiral 1
Parker spiral model canonical 1

How this entity was disambiguated

Statements (48)

Predicate Object
instanceOf heliospheric magnetic field model
solar physics concept
theoretical model
alsoKnownAs Parker spiral model
surface form: Parker spiral
appliesTo heliosphere
solar wind
approximationOf large-scale heliospheric magnetic field
assumes frozen-in magnetic field in the solar wind plasma
steady, spherically symmetric solar wind
basedOn radial outflow of the solar wind
solar rotation
describes large-scale configuration of the Sun’s magnetic field in the heliosphere
structure of the interplanetary magnetic field
developedBy Eugene N. Parker
domain astrophysics
space plasma physics
explains orientation of the heliospheric magnetic field at 1 AU
sector structure of the interplanetary magnetic field near Earth
fieldComponent azimuthal magnetic field component
radial magnetic field component
fieldLineEquation r = (V_sw / Ω_sun) · (φ − φ_0)
geometricType Archimedes' spiral
surface form: Archimedean spiral
historicalContext introduced in the late 1950s
implies magnetic field lines are carried outward by the solar wind
magnetic field lines are wound into a spiral by solar rotation
includesParameter heliocentric distance
solar rotation rate
solar wind speed
influenced design and interpretation of heliophysics missions
namedAfter Eugene N. Parker
neglects small-scale magnetic turbulence
time-dependent solar wind structures
predicts Archimedean spiral geometry of field lines
angle between magnetic field and radial direction increases with distance from the Sun
azimuthal component of the heliospheric magnetic field
radial decrease of magnetic field strength with heliocentric distance
spiral shape of the interplanetary magnetic field lines
relatedTo interplanetary magnetic field
magnetohydrodynamics
solar wind theory
relevantTo interplanetary space
planetary magnetospheric interaction with the solar wind
solar-terrestrial relations
testedBy in-situ magnetic field measurements by spacecraft
spacecraft observations at different heliocentric distances
usedIn cosmic ray transport studies
interpretation of in-situ spacecraft magnetic field measurements
space weather modeling

How these facts were elicited

Referenced by (2)

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

Eugene N. Parker notableWork Parker spiral model
Parker spiral model alsoKnownAs Parker spiral model
this entity surface form: Parker spiral