Abstract
The observational determination of the electron density and velocity distributions in the solar corona is a basis to any physical modelling. In this context, our program, started in 1973, consists in deriving the large-scale electron density distribution from photographic observations of the polarized white-light corona during total solar eclipses. Since 1991, this program makes use of CCD technologies. We present here results of our 2D descriptive model of the electron density distribution.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have