Three-dimensional image of the solar corona from white-light observations of the 1991 eclipse

Details Three-dimensional image of the solar corona from white-light observations of the 1991 eclipse Three-dimensional image of the solar corona from white-light observations of the 1991 eclipse

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992natur.360..717k&link_type=abstract

Nature (ISSN 0028-0836), vol. 360, no. 6406, p. 717-719.

Physics

18

Coronal Holes, Solar Corona, Solar Eclipses, Solar Instruments, Solar Magnetic Field, Emission Spectra, Line Of Sight, Line Spectra, Solar Temperature

Scientific paper

Two white-light images taken about three hrs apart during July 1991 total eclipse of the sun are used here in an attempt to deduce directly the 3D structure of the corona. Prominent coronal structures are observed, including broad threads, rays, and streamers. The structures are used to calibrate a model based on solid-body rotation and bulk coronal outflow. The deduced coronal structure is illustrated by a stereogram.

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