TITLE:
The white-light solar corona in the 2013, 2015 and 2017 solar eclipses

AUTHOR:
V. Rusin, AI SAS

ABSTRACT:
Structures of the white-light corona (scattered light of the solar photosphere on free electrons) 
will be discussed. This solar eclipses were observed in the solar maximum (2013) and 
on a descending branch of a solar cycle 24 (2015 and 2017) at different places on the globe 
(Gabon, Svabard and USA). Different structures, e.g. helmet streamers, coronal holes, polar plumes 
and loops of the corona are a result of a magnetic field distribution, as observed and anchored 
in the photosphere or deeper below photosphere.  Distribution of individual coronal structures 
and their dynamics are very important for properties of the solar wind in the heliosphere.