The analysis was performed of the data level of the scattered light according to the daily observations on the solar corona at Kislovodsk mountian astrionomical station in the period 1957-2010 yrs. near the coronal spectral lines 5303 A and 6374 A. The observations were made near the solar limb and normalized to the intensity at the center of the solar disk. Revealed variations are of different durations: in particular, seasonal variations, local maxima of the last several years, and long-term trends. It was established that local changes in the level of scattered light can be caused by volcanic eruptions. The analysis established a tendency to increase the value of the scattered light by about 40% over the past 50 years. Variations in the level of scattered light were compared with the concentration of atmospheric aerosol. Long-term increase in the level of scattered light is close to changes of surface temperature of the Earth, and possibly is linked to the global climate change.
atmospheric aerosol, solar corona, seasonal variations, volcanes