Using color photometry to search for the solar corona ``reddening'' effect

Details Using color photometry to search for the solar corona ``reddening'' effect Using color photometry to search for the solar corona ``reddening'' effect

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996r%26qe...39..862k&link_type=abstract

Radiophysics and Quantum Electronics, Volume 39, Issue 10, pp.862-864

Physics

1

Scientific paper

The problems of searching for the solar corona “reddening” effect are analyzed. A new method is proposed for quantitative color photometry using a color film with significantly reduced sensitivity in the green spectral region. The results of the photometry of the solar corona slides obtained during the total solar eclipse of November 3, 1994 are presented. From the coronal intensity dependences on the distance in the red (λ eff=660 nm) and blue (λ eff=440 nm) spectral regions for a helmet-shaped streamer (P=70°) and in the region of reduced brightness (P=160°) the “reddening” effect was not detected up to a distance of (3.5 4) R &sun;.

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