Analysis of an elongated narrow coronal streamer observed at the 1973 solar eclipse

Details Analysis of an elongated narrow coronal streamer observed at the 1973 solar eclipse Analysis of an elongated narrow coronal streamer observed at the 1973 solar eclipse

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..103...41t&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 103, Jan. 1986, p. 41-46.

Physics

1

Astronomical Photometry, Solar Activity, Solar Corona, Solar Eclipses, Electron Density (Concentration), Solar Electrons

Scientific paper

A detailed photometric analysis has been made of a narrow elongated coronal streamer observed at the 1973 total eclipse. After deriving real intensity distributions, the electron density has been deduced under the assumption that the distribution is axially symmetric and that the decrease in density from the central axis follows the gaussian law. The results show that the gradient of the electron density is much steeper at the lower part, nearest to the solar limb, than those reported previously for larger scale streamers.

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