The Experimental Observations for the Spectrohe-liogram of Solar D2 Line
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Abstract
The observations showed, that the spectfoheliogram of the solar D2(λ5890 Å) line can provide some characteristics of an active object in a level under the chromosphere, but the resolutions of space and time of the photography was low. It should be better to use a higher collective receiver as a radiative received system.
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