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Observation of the high latitude auroral activity, during the winter season, by means of automatic all-sky camera(s). Study of the high-latitude auroral activity, focusing on the so-called “dayside auroras”: a particular phenomenon concerning the direct precipitation of the thermalised solar wind plasma through the geomagnetic cusps, favourably observable from the Svalbard. The analysis of the data, mainly devoted to the “dayside auroras”, will concern the comparison of the optical images obtained from both the station of Ny-Alesund and the new one of Daneborg (Greenland) with the data collected by Wind, ACE, DSMP, Polar, and Cluster satellites. Starting from the 2002 season, the joint auroral observations from Ny-Alesund and Daneborg allows the monitoring of a relevant area involved in the “dayside aurora” phenomena.