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It is analytically shown that the passage of comet nuclei through the solar chromosphere with velocities more than 600 km/s is accompanied by aerodynamic crushing of the nuclei and transversal expansion of the crushed matter due to gradient of aerodynamic pressure across the frontal surface of the nuclei. Observations of such comet impact-generated photospheric solar flares are of interest for the physics/prognosis of solar flares // Session SpS10: Dynamics of the star-planet relations.