The white light corona and photospheric magnetic fields

Details The white light corona and photospheric magnetic fields The white light corona and photospheric magnetic fields

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2442..263m&link_type=abstract

In NASA. Goddard Space Flight Center Coronal and Prominence Plasmas p 263-267 (SEE N87-20871 13-92)

Physics

Brightness Distribution, Photosphere, Solar Corona, Solar Limb, Solar Magnetic Field, White Light Holography, H Alpha Line, Magnetic Field Configurations, Solar Prominences, Synoptic Measurement

Scientific paper

In this paper some results are presented from a continuing investigation of the coronal structure vs. the photospheric magnetic field relationship. Two approaches to the problem are considered. First, the individual coronal features recorded at each limb were located on a chart of the magnetic field measured with low spatial resolution, depicting the large-scale or global field configuration. Second, the characteristics of neutral line segments - defined by the presence of Hα filaments - with no associated coronal structure were investigated. Preliminary results are discussed.

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