Electrons in the solar corona. I - Electron density models of streamers at eclipse 15 February 1961

Details Electrons in the solar corona. I - Electron density models of streamers at eclipse 15 February 1961 Electrons in the solar corona. I - Electron density models of streamers at eclipse 15 February 1961

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...37..367d&link_type=abstract

Solar Physics, vol. 37, Aug. 1974, p. 367-394.

Physics

10

Astronomical Models, Electron Density Profiles, Solar Corona, Solar Eclipses, Solar Electrons, Astronomical Photometry, Atmospheric Models, Coronagraphs, K Lines, Solar Limb

Scientific paper

Accurate locations, shapes, and photometry of streamers during a solar eclipse are obtained by combining photometric measurements of the inner and outer corona with K-coronameter observations and morphological pictures of the streamers obtained by a gradient compensation technique. The electron density distribution in four streamers situated near the limb plane is calculated by an approach proposed by Van de Hulst (1950). Local increases in electron density at the neck of helmet-shaped streamers with an almost local zero gradient are discussed.

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