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Published online by Cambridge University Press: 25 April 2016
The Working Group was organized in order to promote and develop the cooperative studies of flare stars. Up to the present time our observation programmes were restricted to the UV Ceti-type stars only. Organizational activities followed the aims:
(1) To extend the existing network of photoelectric observers in order to provide 24-hour coverage of a star during selected sessions lasting usually 14 days.
(2) To collect data using standardized techniques in order to study frequency of stellar flares and secondary variations.
(3) To provide optical coverage for simultaneous radio, spectroscopic and polarimetric observations.