heliospheric current sheet

E941946

The heliospheric current sheet is a vast, wavy surface in the solar system where the Sun’s rotating magnetic field causes a thin electric current layer that separates regions of opposite magnetic polarity in the solar wind.

All labels observed (1)

Label Occurrences
heliospheric current sheet canonical 1

How this entity was disambiguated

Statements (48)

Predicate Object
instanceOf astrophysical structure ⓘ
current sheet ⓘ
plasma structure ⓘ
affects modulation of galactic cosmic rays at 1 AU ⓘ
alignedWith solar magnetic equator ⓘ
associatedWith interplanetary magnetic field ⓘ
solar wind ⓘ
boundaryBetween magnetic sectors of the solar wind ⓘ
composedOf ionized plasma ⓘ
discoveredBy spacecraft observations ⓘ
extendsFrom near the Sun ⓘ
extendsTo outer heliosphere ⓘ
governedBy magnetohydrodynamics ⓘ
hasCause Sun's rotating magnetic field ⓘ
hasCurrentDensity on the order of 10^-10 A/m^2 near Earth ⓘ
hasDiscoveryEra space age ⓘ
hasElectricCurrentDirection azimuthal ⓘ
hasMagneticPolarityChange across the sheet ⓘ
hasPhysicalProperty thin electric current layer ⓘ
hasPolarityReversalFrequency approximately every 11 years ⓘ
hasReferenceFrame heliographic coordinates ⓘ
hasSectorStructure four-sector configuration during some solar cycle phases ⓘ
two-sector configuration during some solar cycle phases ⓘ
hasShape wavy surface ⓘ
hasSynonym HCS ⓘ
interplanetary current sheet ⓘ
hasTemporalVariation changes with the solar cycle ⓘ
hasThickness on the order of 10,000 kilometers near Earth ⓘ
hasWarping ballerina skirt shape ⓘ
influences propagation of cosmic rays ⓘ
solar energetic particle transport ⓘ
structure of the interplanetary magnetic field ⓘ
isDynamic true ⓘ
isGlobalStructure true ⓘ
locatedIn solar system ⓘ
linked to: Solar System
observedBy ACE spacecraft ⓘ
Parker Solar Probe ⓘ
Pioneer spacecraft ⓘ
linked to: Pioneer 9

Solar Orbiter ⓘ
Ulysses spacecraft ⓘ
Voyager spacecraft ⓘ
Wind spacecraft ⓘ
partOf heliosphere ⓘ
relatedTo solar magnetic polarity reversal ⓘ
separates regions of opposite magnetic polarity in the solar wind ⓘ
studiedIn heliophysics ⓘ
space plasma physics ⓘ
tiltedRelativeTo solar rotational equator ⓘ

How these facts were elicited

Referenced by (1)

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