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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Statements (47)

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

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