Imaging the structure of the low K-corona

摘要

The first 2-D distributions of the polarization angle and of the relative color index for the K-corona of 29 March 2006 are presented. The distributions illustrate the efficiency of the total solar eclipse approach for high-precision measurements of the K-corona continuum in the range 0.91 can be observed from Lagrange points L2 for Mercury, Venus, and Earth.