Observations of a surge prominence as a continuum event

Details Observations of a surge prominence as a continuum event Observations of a surge prominence as a continuum event

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...48..149r&link_type=abstract

Solar Physics, vol. 48, May 1976, p. 149-158.

Physics

Free Electrons, Light Scattering, Photosphere, Solar Prominences, Acceleration (Physics), Continuous Radiation, Electron Density Profiles, Emission Spectra, Solar Physics, Surges

Scientific paper

Observations of a surge prominence event on 31 May 1971 are discussed. The continuum emission observed during the upward acceleration of the surge is attributed to the scattering of photospheric radiation by free electrons. The observed scattered light intensity amounts to a few times 10 to the -5th that of the central disk intensity leading to a column density of 10 to the 20th per sq cm. The actual electron density when taking into account the presence of inhomogeneities is about 10 to the 12th per cu cm. The dynamic and morphological behavior of the surge is considered.

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