Phenomena Accompanying the Birth of Sunspot Pores

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Abstract
Disturbances in the photospheric granulation accompanying the birth and development of some sunspot pores are illustrated (Plate 1) and described. The disturbances last for about 3 hr and take the form of a number of dark lanes lying between two groups of pores whose location with respect to the rest of the spot group suggests that they are of opposite magne1;ic polarities.

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