Parker spiral model of the interplanetary magnetic field

E278344

The Parker spiral model of the interplanetary magnetic field describes how the Sun’s rotating, magnetized solar wind stretches the solar magnetic field into an Archimedean spiral shape throughout the heliosphere.

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Predicate Object
instanceOf heliospheric magnetic field model
physical model
solar wind model
theoretical model
appliesTo heliosphere
solar wind
assumes constant solar rotation rate
magnetic field lines are frozen into the solar wind plasma
radial solar wind velocity
spherically symmetric solar wind outflow
steady-state solar wind
basedOn Sun’s rotation
frozen-in magnetic field approximation
ideal magnetohydrodynamics
radial outflow of the solar wind
coordinateSystem heliocentric inertial frame
describes Archimedean spiral configuration of solar magnetic field lines
shape of the heliospheric magnetic field lines
structure of the interplanetary magnetic field
formulatedBy Eugene N. Parker
hasKeyParameter heliocentric distance
solar rotation angular velocity
solar wind speed
implies magnetic field lines are nearly radial close to the Sun
magnetic field lines become more azimuthal at larger heliocentric distances
influences design of heliospheric magnetic field simulations
models of energetic particle transport in the heliosphere
namedAfter Eugene N. Parker
neglects coronal mass ejections
small-scale magnetic turbulence
time-dependent solar wind variations
predicts Archimedean spiral magnetic field lines in the ecliptic plane
angle between magnetic field and radial direction increases with distance from the Sun
azimuthal component of the interplanetary magnetic field
magnetic field lines lag behind radial direction due to solar rotation
radial decrease of magnetic field strength with heliocentric distance
sector structure of the interplanetary magnetic field
publicationYear 1958
relatedTo Parker solar wind model
heliospheric current sheet
interplanetary magnetic field
space weather
usedIn interpretation of in-situ spacecraft magnetic field measurements
modelling of cosmic ray propagation in the heliosphere
solar–terrestrial physics
space physics
validIn supersonic solar wind region

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Eugene N. Parker knownFor Parker spiral model of the interplanetary magnetic field