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NASA NTRS · 19910036453

A three-dimensional simulation of a coronal streamer

Abstract

A time-dependent MHD simulation was used to investigate the magnetic topology of an idealized streamerlike configuration in three dimensions. Starting from an initially current-free multipole field and a transonic flow, a quasi-steady, streamerlike configuration forms. The simulated streamer exhibits a closed magnetic field region bounded by a current layer and surrounded by open fields. This helmet region is surmounted by a current layer, with an enhanced density in the closed field and current sheet regions. The simulated streamer has a finite longitudinal extent, with the closed field region primarily confined to the center of the structure.

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BibTeXRIS

Linker, Jon A., Van Hoven, Gerard, Schnack, Dalton D.. 1990-12-01. A three-dimensional simulation of a coronal streamer. https://ntrs.nasa.gov/citations/19910036453

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