SDO in Pulkovo observatory

Abstract

We discuss effective applications of data obtained by both instruments of the Solar Dynamics Observatory: The Helioseismic & Magnetic Imager (HMI) and The Atmospheric Imaging Assembly (AIA). The purpose of this presentation is to show the most important problems of solar activity which are the main subjects in Pulkovo Observatory of the Russian Academy of Science. For these investigations uniform data sets of magnetic fields and coronal emissions in extreme ultra-violet bands are needed. Thus, we are planning to create SDO center in Pulkovo Observatory, which will help us in collaboration with existing SDO centers and provide more effective way of access to data for studies of the Sun.