Simple Magnetic Flux Balance as an Indicator of Neon VIII Doppler Velocity Partitioning in an Equatorial Coronal Hole

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dc.creatorMcIntosh, Scott W.
dc.creatorDavey, Alisdair R.
dc.creatorMcIntosh, Scott W.
dc.date2006-05-22
dc.date.accessioned2026-07-07T07:08:33Z
dc.date.available2026-07-07T07:08:33Z
dc.descriptionWe present a novel investigation into the relationship between simple estimates of magnetic flux balance and the Ne VIII Doppler velocity partitioning of a large equatorial coronal hole observed by the Solar Ultraviolet Measurements of Emitted Radiation spectrometer (SUMER) on the Solar and Heliospheric Observatory (SOHO) in November 1999. We demonstrate that a considerable fraction of the large scale Doppler velocity pattern in the coronal hole can be qualitatively described by simple measures of the local magnetic field conditions, i.e., the relative unbalance of magnetic polarities and the radial distance required to balance local flux concentrations with those of opposite polarity.
dc.descriptionTo appear ApJL (June)
dc.identifierhttps://arxiv.org/abs/astro-ph/0605565
dc.identifierhttp://arxiv.org/abs/astro-ph/0605565
dc.identifierAstrophys.J. 644 (2006) L87-L91
dc.identifierdoi:10.1086/505488
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/110745
dc.subjectAstrophysics
dc.titleSimple Magnetic Flux Balance as an Indicator of Neon VIII Doppler Velocity Partitioning in an Equatorial Coronal Hole
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