Giant coronal streamers registered during the solar
eclipse in 1999 from a sky fighter Mig-21 on Kodak Ektachrome
IR film EIR 200. Blue color is due to blue or green light emission.
Photograph by D. Petrov and Y. Shopov
Structure of the solar dust corona and its interaction with the
other coronal components
Additional evidences that giant coronal streamers
emitted only blue and green light during the eclipse
on the 11 August 1999 (Fig. 14), were obtained
directly from a hypersonic fighter flying at 13,000m altitude with speeds of 1600–1700 km/h
Y.Y. Shopova,, D.A. Stoykovaa, K. Stoitchkovaa, L.T. Tsankova, A. Taneva,
Kl. Burina, St. Belchevb, V. Rusanova, D. Ivanova, A. Stoevc, P. Muglovad, I. Iliev
Journal of Atmospheric and Solar-Terrestrial Physics 70 (2008) 356–364