Ubiquitous Open Magnetic Field Lines in the Inner Corona

Details Ubiquitous Open Magnetic Field Lines in the Inner Corona Ubiquitous Open Magnetic Field Lines in the Inner Corona

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679...55w&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 55-58

Computer Science

4

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind, Interplanetary Magnetic Fields, Electric And Magnetic Fields, Solar Magnetism

Scientific paper

The notion that density structure reflects magnetic field lines makes it possible to deduce information on coronal magnetic fields from density measurements. The purpose of this paper is to summarize the observational evidence for ubiquitous open magnetic field lines in the inner corona from density measurements. Based on both global and filamentary structures, these density measurements explain the unexpected predominance of the radial component of coronal magnetic field discovered in polarimetric observations over three decades ago.

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