Recent Developments in Improving Daytime Angular Resolution from the Ground
The subject of this symposium is the fine structure of the solar chromosphere. Progress in this field of reserach will depend to a high degree of the quality of seeing, resp. on the effective angular resolution available on the ground. Today's situation of solar ground seeing has changed distinctly in the last years. I would like to report here a few new aspects, which could be condensed into 3 questions: (1)Are there on the ground ‘good seeing windows’, comparable in quality with stratosphere results obtained from balloon borne equipment?(2)Is there a chance to resolve from the ground the solar scale height, corresponding to about 0.1″.(3)Is there a residual fundamental atmospheric seeing noise resp. a basic limit to the atmospheric Modulation Transfer Function (MTF)?